European Space Agency Research and Science Support Department Planetary Missions Division Rosetta - MIRO To Planetary Science Archive Interface Control Document RO-MIR-IF-0001 Version 1.8 (May 2009) ______________________________ Prepared by: Michael A Janssen and Lucas Kamp __________________________ Approved by: Samuel Gulkis Distribution List Recipient Organisation Recipient Change Log Date Sections Changed Reasons for Change 2003-Aug-12 all Initial version 2003-Sep-09 many EDITS AS A RESULT OF PDS TELECON 2003-Nov 2,4 2003-Dec Changed doc.ID from UoB-IF- 1234 to MIR-IF-0001. Updated keywords in 4.2 & App.1 per latest Archive Plan. 2004-Jul 3-6 Corrections after review of sample label 2005-Dec All Revisions for delivery of groundtesting archive 2006-Nov All Revisions after PDS Internal Review and for delivery of calbrated data. 2006-Dec-11 Section 3.4.2l Updated delivery dates and added items per email from Maud Barthelemy 2007-May-09 Sections 3.2.3 and 4.2 Section 5 Added documentation of coordinate systems used. Changed VOLUME keywords per revised Archive Conventions 2007-Oct-22 1.5, 2.3.4, 3.2.2, 3.4, 4.2, 6, 5 Added explanation of Times in data files, changes to labels and delivery contents, and revised structure files. 2008-Sep-02 Section 4.4 added, Section 7 revised PDS review requested more documentation of data formats. 2009-May-15 Section 6.4 Removed GMT field from Level-3 continuum files TABLE OF CONTENTS 1 INTRODUCTION 6 1.1 PURPOSE AND SCOPE 6 1.2 ARCHIVING AUTHORITIES 6 1.3 CONTENTS 6 1.4 INTENDED READERSHIP 7 1.5 APPLICABLE DOCUMENTS 7 1.6 RELATIONSHIPS TO OTHER INTERFACES 7 1.7 ACRONYMS AND ABBREVIATIONS 7 1.8 CONTACT NAMES AND ADDRESSES 9 2 OVERVIEW OF PROCESS AND PRODUCT GENERATION 10 2.1 MIRO OVERVIEW AND OBJECTIVES 10 2.2 INSTRUMENT DESCRIPTION SUMMARY 10 2.3 DATA PRODUCTS DESCRIPTION 11 2.3.1 Introduction 11 2.3.2 Major Data Modes 12 2.3.3 Calibration and Test Data 13 2.3.3.1 Thermal-Vacuum Ground Tests 13 2.3.3.2 Radiometric Calibration 13 2.3.3.3 Frequency Calibration 14 2.3.3.4 Geometric Calibration 14 2.3.4 Operational Scenarios 15 2.3.5 Data Flows 15 3 ARCHIVE FORMAT AND CONTENT 17 3.1 FORMAT 17 3.1.1 Volume Format 17 3.1.2 Data Set Naming 17 3.1.3 File Name Formats 17 3.2 STANDARDS USED IN DATA PRODUCT GENERATION 18 3.2.1 PDS Standards 18 3.2.2 Time Standards 18 3.2.3 Reference Systems 19 3.3 DATA VALIDATION 19 3.4 CONTENT 19 3.4.1 Volume Set 19 3.4.2 Data Set 19 3.4.3 Directories 21 3.4.3.1 Root Directory 21 3.4.3.2 Calibration Directory 22 3.4.3.3 Catalog Directory 22 3.4.3.4 Data Directory 22 3.4.3.5 Index Directory 23 3.4.3.6 Label Directory 23 3.4.3.7 Document Directory 23 3.4.3.8 Geometry Directory 24 3.4.3.9 Software Directory 24 3.4.4 Data and Label Files 24 4. DETAILED INTERFACE SPECIFICATIONS 25 4.1 Data Product Identification 25 4.2 PDS Label Structure, Definition and Format 25 4.3 Overview of Detectors 27 4.3.1 Spectrometer data 27 4.3.2 Radiometer data. 27 4.3.3 Engineering data. 27 4.4 Data Format Description 27 5. APPENDIX 1: VOLDESC.CAT 29 6. APPENDIX 2: STRUCTURE FILES 30 6.1 Spectroscopic Level 2 Data 31 6.2 Spectroscopic Level 3 Data 32 6.3 Continuum Level 2 Data 37 6.4 Continuum Level 3 Data 40 6.5 Housekeeping Data 43 7. APPENDIX 3: AVAILABLE SOFTWARE TO READ PDS FILES 63 8. APPENDIX 4: DIRECTORY LISTING OF DATA SET MIRO_THERMALVAC 63 1 Introduction 1.1 Purpose and Scope The purpose of this EAICD (Experimenter to Planetary Science Archive Interface Control Document) is twofold. First it provides users of the MIRO instrument with detailed description of the products and a description of how they were generated, including data sources and destinations. Secondly, the EAICD describes the interface to the Planetary Science Archive (PSA) of ESA and is the official document between each experimenter team and the PSA. 1.2 Archiving Authorities The Planetary Data System (PDS) Standard is used as archiving standard by * NASA for U.S. planetary missions, implemented by PDS * ESA for European planetary missions, implemented by the Research and Scientific Support Department (RSSD) of ESA ESA's online Planetary Science Archive (PSA) was implemented * to support and ease data ingestion * to offer additional services to the scientific user community and science operations teams as e.g. o search queries that allow searches across instruments, missions and scientific disciplines o several data delivery options as _ direct download of data products, linked files and data sets _ ftp download of data products, linked files and data sets The PSA aims for online ingestion of logical archive volumes and will offer the creation of physical archive volumes on request. 1.3 Contents This document describes the data flow of the MIRO instrument on Rosetta from the s/c until the insertion into the PSA. It includes information on how data were processed, formatted, labeled and uniquely identified. The document discusses general naming schemes for data volumes, data sets, data and label files. Standards used to generate the product are explained. Software that may be used to access the product is explained. The design of the data set structure and the data product is given. Examples of these are given in the appendix. 1.4 Intended Readership The MIRO science, software development and engineering team, the staff of the Planetary Science Archive design team, and any potential user of MIRO data. 1.5 Applicable Documents AD1 Rosetta Archive Generation, Validation and Transfer Plan, 10 January 2006, RO-EST-PL-5011, Issue 2, Revision 3 AD2 Planetary Data System Standards Reference, 1 August 2003, Version 3.6, JPL D-7669, Part 2 AD3 Planetary Data System Data Dictionary Document, 28 August 2002, Revision E, JPL D-7116 AD4 MIRO Users Manual, RO-MIR-PR-0030 AD5 Acton, C.H.; "Ancillary Data Services of NASA's Navigation and Ancillary Information Facility;" Planetary and Space Science, Vol. 44, No. 1, pp. 65-70, 1996. AD6 Backus, C. and Gulkis, S., "CTS: Frequency Response as a Function of Temperature" AD7 Rosetta Time Handling, 28 February 2006, RO-EST-TN-3165, Issue 1, Revision 1 1.6 Relationships to Other Interfaces The controlling document of the interfaces discussed here is AD1. For further details on the MIRO instrument and its usage, see AD4. 1.7 Acronyms and Abbreviations bps bits per second CCSDS Consultative Committee for Space Data Systems CODMAC Committee on Data Management and Computation CTS Chirp Transform Spectrometer DBMS Database Management System DDS Data Distribution System (Darmstadt, Germany) DVD Digital Video Disk ESA European Space Agency GHz GigaHertz (109 Hz) HSK Housekeeping IFP Intermediate Frequency Processor JPL Jet Propulsion Laboratory (Pasadena, CA) KHz kiloHertz (103 Hz) LO Local Oscillator MHz MegaHertz (106 Hz) MM millimeter MIRO Microwave Instrument for the Rosetta Orbiter NAIF Navigation and Ancillary Information Facility NASA National Aeronautics and Space Agency (USA) OBT On-Board Time PDS Planetary Data System PSA Planetary Science Archive rms root mean square SUBMM submillimeter TDB Barycentric Dynamical Time USO Ultra Stable Oscillator UTC Coordinated Universal Time 1.8 Contact Names and Addresses Last Name First Name Institution Phone Email Backus Charles JPL 818 354-4543 charles.r.backus@jpl.nasa.gov Frerking Margaret JPL 818 354-4902 margaret.a.frerking@jpl.nasa.gov Gulkis Samuel JPL 818 354-5708 samuel.gulkis@jpl.nasa.gov Janssen Michael JPL 818 354-7247 michael.a.janssen@jpl.nasa.gov Kamp Lucas JPL 818 354-4461 lucas.w.kamp@jpl.nasa.gov Nowicki Robert JPL 818 393-5953 robert.m.nowicki@jpl.nasa.gov 2 Overview of Process and Product Generation 2.1 MIRO Overview and Objectives The MIRO investigation addresses the nature of the cometary nucleus, outgassing from the nucleus and development of the coma as strongly interrelated aspects of cometary physics, and searches for outgassing activity on asteroids. MIRO is configured both as a continuum and a very high spectral resolution line receiver. Center-band operating frequencies are near 188 GHz (1.6 mm) and 562 GHz (0.5 mm). Spatial resolution of the instrument at 562 GHz is approximately 5 m at a distance of 2 km from the nucleus; spectral resolution is sufficient to observe individual, thermally broadened, line shapes at all temperatures down to 10 K or less. Four key volatile species - H2O, CO, CH3OH, and NH3-and the isotopes-H217O and H218O-are pre-programmed for observation. The primary retrieved products are abundance, velocity, and temperature of each species, along with their spatial and temporal variability. This information will be used to infer coma structure and processes, including the nature of the nucleus/coma interface. MIRO will sense the subsurface temperature of the nucleus to depths of several centimeters or more using the continuum channels at millimeter and submillimeter wavelengths. Model studies will relate these measurements to electrical and thermal properties of the nucleus and address issues connected to the sublimation of ices, ice and dust mantle thickness, and the formation of gas and dust jets. The global nature of these measurements will allow in situ lander data to be extrapolated globally, while the long duration of the mission will allow us to follow the time variability of surface temperatures and gas production. Models of the thermal emission from comets are very crude at this time since they are only loosely constrained by data. MIRO will offer the first opportunity to gather subsurface temperature data that can be used to test thermal models. MIRO is highly complementary to the IR mapping instrument on the orbiter, having similar spatial resolution but greater depth penetration. 2.2 Instrument Description Summary The MIRO instrument will provide both very sensitive continuum capability for temperature determination and extremely high-resolution spectroscopy for observation of molecular species. The instrument consists of two heterodyne radiometers, one at millimeter wavelengths (1.3 mm) and one at submillimeter wavelengths (0.5 mm). The millimeter and the sub-millmeter radiometers have continuum bandwidths of 0.5 GHz and 1.0 GHz respectively in addition, the submillimeter receiver has a total spectroscopic bandwidth of 180 MHz and a spectral resolution of 44 kHz. In the spectroscopic mode, 4096 channels, each having a bandwidth of 44 kHz, are observed simultaneously. The performance parameters that govern the MIRO instrument design include system sensitivity, spatial resolution, radiometric accuracy (both absolute and relative), beam pattern and pointing accuracy, together with the mass, power, volume envelope, and environmental conditions available within the spacecraft. The MIRO instrument performance characteristics are summarised in Table 2.2. More detailed information can be found in the MIRO User Manual (AD4). Equipment Property Millimeter-Wave Submillimeter-Wave Telescope Primary Diameter Primary F/D Sidelobes Spatial Resolution Footprint size (at 2 km) 30 cm 1 -30 dB 24 arcmin ~15 m 30 cm 1 -30 dB 8 arcmin ~5 m Spectral Performance Frequency Band 1st IF Bandwidth 1st IF Frequenct Range Spectral Resolution Allocated Spectral Range per line Accuracy 188.5-191.5 GHz 550 MHz 1-1.5 GHz n/a n/a n/a 547.5-580.5 Ghz 11 GHz 5.5-16.5 GHz 44 kHz nominally 20 MHz 10 kHz Spectrometer Center Frequency/Bandwidth Number of channels n/a n/a 1350/180 MHz 4096 Radiometric Performance DSB Receiver Noise Temperature SSB Spectroscopic Sensitivity (300 KHz, 2 min) : relative absolute Continuum Sensitivity (1 sec): relative absolute 800 K n/a n/a 1 K rms 3 K rms 3800 K 2 K rms 3 K rms 1 K rms 3 K rms Data Rates Instantaneous Rate Continuum Mode Spectroscopic Mode On-board Storage <1 kbps 2 kbps 0.2 GB (one day's data volume, Mode 3, 100% duty cycle) Table 2.2. MIRO Instrument Performance Characteristics 2.3 Data Products Description 2.3.1 Introduction The MIRO instrument has 6 major modes of operation and data-taking that reflect operational combinations of its two continuum radiometers and the spectrometer, engineering mode, millimeter continuum mode, submillimeter continuum mode, dual continuum mode, CTS/submillimeter continuum mode, and CTS/dual continuum mode. In addition, a special mode has been designed for planetary and asteroid flybys. A number of data compression options are obtained in each mode by varying the data-taking rate (integration time per sample) and/or spectral resolution of the radiometers and spectrometer. The specific parameters for each mode are described in more detail in the MIRO User Manual (AD4), Volume 6.1, and are summarized here. All data files that will be delivered to the PSA are table files, consisting of time sequences of measured data. This applies to engineering (housekeeping), continuum and spectroscopic data, both raw and calibrated. (The detailed structure of these files is defined by the Structure Files listed in Appendix 2.) It is anticipated that, in the future, derived products will be generated in image, cube or map format, but these formats have not yet been defined and there are no plans to archive such products. 2.3.2 Major Data Modes Engineering Mode In engineering mode the MIRO software is collecting engineering data from 56 internal sensors. The sampling of these sensors is at a 5 Hz rate. All engineering measurements are 12-bit A/D converted values. The engineering mode telemetry is sent to the spacecraft in the form of a housekeeping telemetry packet. One engineering telemetry packet is typically generated every 11 seconds. Millimeter Continuum Mode In millimeter continuum mode continuum data are collected from the millimeter radiometer at a 20 Hz. rate. All continuum data consist of 16-bit values. The millimeter continuum data are nominally packetized into science telemetry packets every 10 seconds. A 'summing value' parameter can cause the MIRO software to sum either 1, 2, 5, 10 or 20 separate continuum values prior to putting them into the telemetry packet. This feature can reduce the data rate to as little as one millimeter continuum packet every 200 seconds. Submillimeter Continuum Mode Sub-millimeter continuum mode is identical to the millimeter continuum mode in data collection and packing except that a different set of electronics is powered on. Millimeter and submillimeter continuum data are contained in separate science telemetry packets, identified by a field in the source data header. Dual Continuum Mode In dual continuum mode the millimeter and submillimeter continuum are collected simultaneously. When running in dual continuum mode, the summing value parameter mentioned earlier is applied to both sets of data, causing equal amounts of millimeter and submillimeter data to be generated. CTS / Submillimeter Continuum Mode This mode adds the collection of chirp transform spectrometer (CTS) data. The CTS is programmed by the MIRO software to run for an initial sub-integration period of approximately 5 seconds. An internal LO frequency generator is then switched, which has the effect of introducig a small shift in the frequencies, and another 5 second period is observed. These pairs of observations are repeated with the respective results being summed over time. Selectable integration periods are 30, 60, 90 and 120 seconds. The data from the two LO frequencies are then subtracted from each other to provide a single 4096-element difference spectrum. The 4096 data values can be further reduced by application of a smoothing function whereby data from several channels are combined and weighted to produce fewer final channels. Smoothing window sizes are 1, 5, 7 and 9 channels. A mask is applied to the CTS data and only 12 bits of each resulting measurement are returned. CTS data collection and the LO frequency switching is coordinated with the collection of continuum data. Exactly 100 continuum samples are taken during each CTS scan. Upon receipt of the data on the ground it is known at which LO frequency all of the continuum measurements were made. If the CTS has just been powered on, an internal calibration of the CTS is performed. This consists of loading the 4 CTS sum of square tables with a linear ramping pattern. A 10,000 cycle integration is then performed and the resulting data read out. The data are then averaged to yield the mid-point of the table. The resulting mid-point values for each table are downlinked in telemetry packets for monitoring over time. CTS / Dual Continuum Mode This is the same as the CTS / SMM continuum mode except that the millimeter data are also collected. Asteroid Mode This special data-taking mode has been implemented for the asteroid and planetary encounters to enable MIRO to follow the rapid Doppler shift of spectral lines that may be visible. The primary characteristic of this mode is that LO frequency switching is turned off. The LO is set to either +5 MHz or - 5 MHz from the nominal frequency prior to the encounter. At the specified encounter time, the LO frequency is switched _ 5 Mhz (opposite from the first setting) from the nominal frequency. Continuum data are collected at 20 Hz. Each set of CTS data consists of a single 5-second integration with all 32 bits returned for each 4096 channels. 2.3.3 Calibration and Test Data 2.3.3.1 Thermal-Vacuum Ground Tests These tests were carried out at JPL from 15 May to 29 June 2001 and were intended to determine characteristics of the MIRO instrument in vacuum conditions and as a function of temperature. The emphasis was on deriving parameters that cannot be obtained under ambient conditions, such as the noise figures of various electronic components, the frequency response of the instrument and the linearity of the response, and the stability of several features. The data obtained from these tests and the accompanying log files are delivered as the first MIRO archive dataset. 2.3.3.2 Radiometric Calibration The MIRO instrument is calibrated on a periodic basis and immediately following every mode change. An automatic calibration will take place every 1895 seconds, if not interrupted by a mode change command, which triggers a calibration immediately. The normal interval of 1895 seconds allows 95 seconds for the calibration and 1800 seconds (30 minutes) for the data collection period. The 1800 seconds allows for complete integration periods of 30, 60, 90, and 120 seconds (60, 30, 20, and 15 integrations respectively). The 95 seconds of calibration data are distributed as follows: Time(seco nds) Activity 5 3 mirror movements/no data collection 30 Warm load position- CTS + continuum + engineering 30 Cold load position - CTS + continuum + engineering 30 Sky position - CTS + continuum + engineering These calibration data are included im the level-2 data files as part of the time sequence. They are flagged by a Calibration field in the header columns (see the Structure files in Appendix 2). Receiver gains (in counts per Kelvin) are computed by measuring the difference in the number of counts from the receiver as the input is switched between loads at two different (known) temperatures. Load temperature differences (in counts) are obtained by switching between 1) warm load and cold load, or 2) warm load and sky. The choice between cold load or sky is indicated by the "Type" field in each record, see Appendix 2. (In the current delivery, this field is missing from the continuum data, which were always calibrated using sky.) Data records are converted to temperature units by dividing by the number of counts per Kelvin. The temperature units reported are Rayleigh-Jeans temperature units, where the product kTB (k = Boltzmann's constant, B = bandwidth and T is the Rayleigh-Jeans temperature) is the received power. A factor of two multiplies the spectroscopic record to convert it to a single sideband. Fluctuations in the gains resulting from LO switching cause small offsets visible in the differenced spectroscopic data, which will be corrected for in future work. These errors are of the order of 5K, about 0.1% of the system temperatures. 2.3.3.3 Frequency calibration The frequency calibration of the CTS is a complex subject, described in AD6, which is included in this delivery as the file MIRO_CTS_FREQUENCY_CALIBRATION_V0 in the Document directory. The Receiver Frequency of the radiation entering the instrument (in the range 547.5 - 580.5 GHz, see Table 2.2) is translated by a series of mixers in the IFP to the frequency range of the CTS, centered at 1350 MHz. The relationship between IFP output frequency and channel number is a function of temperature. In the calibrated data in this delivery, the SPECT_T1 field (see Appendix 2, Section 6.2) gives this temperature, which is always 67.9 C in this dataset, since that is the standard value to which the calibrated data have been rebinned. 2.3.3.4 Geometric Calibration Determination of the position and attitude of the instrument is done using data and software provided by the Navigation and Ancillary Information Facility (NAIF) group at JPL, see AD5. This group, in collaboration with the Flight Dynamics staff of ESA, regularly generates files containing the position and attitude of the Rosetta spacecraft, called "kernels": C (Camera) kernels contain the spacecraft attitude data, SP (Spacecraft and Planet) kernels contain the positions and velocities of the bodies. Other kernels generated by NAIF contain time information (leapseconds, conversion constants to the spacecraft clock), planetary constants (dimensions, rotation rates), and instrument characteristics (beamwidth, orientation relative to the spacecraft frame). The particular kernel files used in the processing for a given delivery are specified in the delivery documentation. The orientation of the MIRO boresight relative to the Rosetta spacecraft frame that is contained in the NAIF Frames kernel for Rosetta was derived by the MIRO team from the Spiral scans of the Earth during the Commissioning phase. The MIRO team has developed software which uses the NAIF kernels to allow appending of geometric information to all science data files, including, at each point in time, instrument boresight attitude and location of the boresight on the target body, if applicable. Such information is not planned to be included in delivered archive products, but will be available for analysis of MIRO data. 2.3.4 Operational Scenarios MIRO is planning to collect scientific and/or calibration data at every planetary and asteroid encounter and at the target comet. In addition, MIRO plans to gather calibration data during system checkout and cruise modes. The data will be limited during the planetary and asteroid flybys, but extensive during the various phases at the comet. Normal mode of operation - In the normal mode of operation, the MIRO instrument will operate in a frequency switching mode. If the instrument is in a continuum only mode, the frequency switching is turned off. Asteroid mode - A special data-taking mode, called the "Asteroid Mode", has been implemented for the asteroid and planetary encounters. The primary characteristic of this mode is that LO frequency switching is turned off. The LO is set _ 5 MHz from the nominal frequency prior to the encounter. At the specified encounter time, the LO frequency is switched _ 5 Mhz (opposite from the first setting) from the nominal frequency. Continuum data are collected at 20 Hz. Each set of CTS data consists of a single 5-second integration with all 32 bits returned for each 4096 channels. Mars and Earth flybys - There are likely to be separate scenarios designed for the Mars and Earth flybys. (Note added in Rev 1.6: MIRO did not participate in the Mars flyby.) 2.3.5 Data Flows The MIRO telemetry packets coming from the spacecraft are retrieved from the ESOC Data Distribution System (DDS) at Darmstadt by PI-controlled workstations located at the Jet Propulsion Laboratory in Pasadena, CA, under the direct responsibility of the PI. The telemetry records will be written in their original SFDU formats for permanent safekeeping in the MIRO archival system at JPL. These telemetry records will be kept in the MIRO project but are not considered part of the formal science archive. The Data Archive has the following characteristics: 1) The MIRO Data Archive system is located at JPL in Pasadena, CA. 2) The Data Archive system has the capability to store and maintain all the data coming from ESA (instrument/science data, housekeeping data, auxiliary data, navigation data, command logs) in their original format (SFDU format where applicable). 3) The Data Archive system is capable of transferring data to the MIRO data base management system (DBMS) for further processing. 4) The Data Archive system has the capability to store and maintain all the data in PDS format that will be delivered to the Small Bodies Node of the PDS. All data (science, housekeeping and auxiliary) in the MIRO Raw Data Archive at JPL are capable of being ingested into the MIRO DBMS. This DBMS is the means of access to the data for team members doing science analysis of these data. Delivery of data to the Rosetta Mission Archive of the PSA of ESA and the Small Bodies Node of the PDS of NASA is done by extracting data from the MIRO DBMS into file formats defined by this document and generating PDS labels for these files. These files are placed in directory trees in the MIRO Data Archive, along with all associated documentation and index tables. Compressed copies of these directories are delivered to the PSA and PDS for external archival and will also remain online in the MIRO Data Archive. The MIRO team will support the peer reviews of MIRO-related data that are conducted by the ESA-PDS archiving team and will correct or otherwise appropriately resolve any liens identified by the peer review(s). The Small Bodies Node of PDS will work jointly with the archiving scientists at ESA to prepare the complete ROSETTA archive within ESA consistent with all PDS standards (see AD2). Ultimately the ROSETTA archive will reside both at ESA and with NASA's PDS. PDS and the ESA archiving scientists will carry out the peer review of all data to ensure that outside users can make good scientific use of the data from the archive. The final archive will be maintained electronically both by the PDS Small Bodies Node and by ESA. ESA will prepare CD ROM (or successor media such as DVD ROM) copies of the archive for distribution both through ESA and through PDS. The raw data at JPL will receive a preliminary radiometric calibration. Further data reduction and data analysis will be carried out to provide calibrated data in standard formats and derived products such as maps of abundances or column densities. Co-Is will also have electronic access to the data from the database in Pasadena. Co-Is will also produce selected calibrated data sets and return them to the Pasadena database. The MIRO science team will also produce, at the home institutions of the team members, derived products as appropriate. These might include spatial maps, rectified to a common coordinate system, of the abundances of specific molecules. The MIRO team expects that the ROSETTA project may wish to combine data from MIRO with data from other instruments, particularly ALICE, OSIRIS or VIRTIS, on a single archive volume. This will considerably enhance the usability of the archive for scientific correlative analysis. Archive preparation of any such combination of data sets from different instruments will be the responsibility either of IDSs carrying out comparative studies or of the ROSETTA project within ESA. 3 Archive Format and Content 3.1 Format This section describes the format of the MIRO Instrument Team Archive volumes. Data in the archive will be formatted in accordance with Planetary Data System specifications (AD2). 3.1.1 Volume Format This document will not be concerned with any particular media formats such as DVD's because data will be delivered electronically. When applicable, media formats will be determined by the PDS. Also, for present purposes, datasets will be regarded as equivalent to volumes. 3.1.2 Data Set Naming The informal Dataset Names used in this document are formed by appending the mission phase descriptor to the instrument name. Examples are: MIRO_THERMALVAC MIRO_COMMISSIONING MIRO_EARTH1 The formal PDS values for DATA_SET_NAME and DATA_SET_ID are formed according to the rules defined in AD1: DATA_SET_NAME = "ROSETTA-ORBITER MIRO ". Examples are: "ROSETTA-ORBITER CAL MIRO 2 GRND THERMAL-VAC V1.0" "ROSETTA-ORBITER EARTH MIRO 2 EAR1 Earth-1 V1.0" DATA_SET_ID = "RO--MIRO---- ". Examples are: "RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0" "RO-E-MIRO-2-EAR1-EARTH1-V1.0" See further AD1 for allowed values for these items. 3.1.3 File Name Formats The following scheme will be used for names of files containing data products: MIRO___begindatetime. The level field is the CODMAC processing level. Valid names for the detector field include: MM SUBMM CTS HSK File extensions can be at least: DAT binary data TXT acsii data, lines of variable length, delimited typically with LBL ascii detached label file DOC text description where necessary Datetime format will be yyyydddhhmmss, where ddd is 1-based Julian day, i.e. Jan 1 is day 1. 3.2 Standards Used in Data Product Generation 3.2.1 PDS Standards The MIRO Data Products comply with the Planetary Data System standards for file formats and labels, as specified in the PDS Standards Reference (AD2). 3.2.2 Time Standards The MIRO Data Products are intended to comply with the CCSDS Time Code Format Standard (CCSDS 301.0-B-2). The On-Board Time (OBT) of the Rosetta spacecraft is used in the PDS keywords SPACECRAFT_CLOCK_START_COUNT and SPACECRAFT_CLOCK_STOP_COUNT. The format of this time (as defined in RO-EST-TN-3165, Rosetta Time Handling) is: "i/mmmmmmmm[.nnnnn]" where: i = integer signifying which zero point is in use. (Currently, all OBTs have i=1, signifying that the zero point is at 2003-01-01T00:00:00 UTC. This integer will change if the clock is ever reset, which is not planned but may happen as a result of unforeseen circumstances.) mmmmmmmm = integer seconds since the zero point. nnnnn = (optional) fractional seconds in units of 1/65536 sec. Therefore, the floating-point time since the zero point represented by a given OBT is: time = mmmmmmmm + nnnnn/65536. The OBT is not used internally in any MIRO data files. Instead, table entries are marked by Sun Modified Julian Time (SMJT) or "unix time", which is elapsed seconds since 1970-01-01T00:00:00 UTC. This takes leapseconds into account and is therefore in the UTC system. The conversion from SMJT to Ephemeris Time (ET2000), which is the standard TDB time system used by NAIF, is given by: ET2000 = SMJT - 946727958.816 + LEAPSECS + O(0.0017) Where the last term represents a sinusoidal correction for the Earth's motion that never exceeds 0.0017 seconds, and LEAPSECS is the number of leapseconds that have been added between 1970 and the relevant date. At the time of writing, LEAPSECS = 24. A Fortran-77 program, named UTCCON, that converts between SMJT and the ISO standard UTC representation, is provided in the DOCUMENT directory. See AD7 for further discussion and conversions to other time systems. 3.2.3 Reference Systems Geometric data such as spacecraft position are reported in the inertial cartesian coordinate frame of epoch J2000, with reference to either the Ecliptic (default) or a specfied Target as center. Target- centered spherical coordinate systems use the standard planetocentric IAU frame. Further details may be found in the Mission Control System Data Delivery Interface Document (DDID), RO-ESC-IF-5003, Appendix H, FD Products. Values for geometric data reported in the labels are given for the time at the midpoint of the observatons in the file. 3.3 Data Validation General data validation procedures are described in the MIRO User Manual (AD4). No data validation has been performed on these products, beyond basic checks on the completeness of Continuum packets and CTS spectra. Validation done on higher-level products will be described in the delivery documentation. 3.4 Content This section describes the directories and contents of the MIRO Data Product volumes, including the file names, file contents, file types, and organization responsible for providing the files. The data described herein appear on each volume of the MIRO Data Product volume series. 3.4.1 Volume Set Since the Rosetta Project plans for electronic delivery and there is no need to bundle several datasets into one volume set, as a general rule, a volume shall be a dataset. 3.4.2 Data Set The following table shows data set name (informal), DATA_SET_ID, delivery date, size, and data types contained, for each volume of the MIRO Data Product volume series through 2008. The naming follows section 3.1.2. For future deliveries (after Oct.2007, as of current writing), the sizes are approximate estimates and the delivery dates nominal. Dataset name Delivery Size Description and DATA_SET_ID Date (Mbytes) MIRO_Thermalvac Nov 2006 728 Science Files, Engineering Files RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0 MIRO_Commissioning (raw) Nov 2006 287 Science Files, Engineering Files, RO-X-MIRO-2-CVP-COMMISSIONING-V1.0 Geometry Files. MIRO_Commissioning (calibrated) Nov 2006 315 Science Files, Geometry Files RO-X-MIRO-3-CVP-COMMISSIONING-V1.0 MIRO_Earth1 (raw) Nov 2006 180 Science Files, Engineering Files, RO-E-MIRO-2-EAR1-EARTH1-V1.0 Geometry Files. MIRO_Earth1 (calibrated) Nov 2006 193 Science Files, Geometry Files, RO-E-MIRO-3-EAR1-EARTH1-V1.0 MIRO_Cruise2 (raw) Dec 2006 629 Science Files, Engineering Files, RO-X-MIRO-2-CR2-CRUISE2-V1.00 Geometry Files. MIRO_Cruise2 (calibrated) Dec 2006 727 Science Files, Geometry Files, RO-X-MIRO-3-CR2-CRUISE2-V1.0 MIRO_Cruise3 (raw) Mar 2008 50 Science Files, Engineering Files, RO-X-MIRO-2-CR3-CRUISE3-V1.00 Geometry Files. MIRO_Cruise3 (calibrated) Mar 2008 70 Science Files, Geometry Files, RO-X-MIRO-3-CR3-CRUISE3-V1.0 MIRO_Earth2 (raw) Jun 2008 150 Science Files, Engineering Files, RO-E-MIRO-2-EAR2-EARTH2-V1.0 Geometry Files. MIRO_Earth2 (calibrated) Jun 2008 170 Science Files, Geometry Files, RO-E-MIRO-3-EAR2-EARTH2-V1.0 MIRO_Cruise4-1 (raw) Jan 2009 100 Science Files, Engineering Files, RO-X-MIRO-2-CR4A-CRUISE4-1-V1.00 Geometry Files. MIRO_Cruise4-1 (calibrated) Jan 2009 140 Science Files, Geometry Files, RO-X-MIRO-3-CR4A-CRUISE4-1-V1.0 MIRO_Steins (raw) May 2009 300 Science Files, Engineering Files, RO-A-MIRO-2-AST1-STEINS-V1.0 Geometry Files. MIRO_Steins (calibrated) May 2009 420 Science Files, Geometry Files, RO-A-MIRO-3-AST1-STEINS-V1.0 MIRO_Cruise4-2 (raw) Mar 2010 70 Science Files, Engineering Files, RO-X-MIRO-2-CR4B-CRUISE4-2-V1.00 Geometry Files. MIRO_Cruise4-2 (calibrated) Mar 2010 90 Science Files, Geometry Files, RO-X-MIRO-3-CR4B-CRUISE4-2-V1.0 MIRO_Earth3 (raw) Jun 2010 150 Science Files, Engineering Files, RO-E-MIRO-2-EAR3-EARTH3-V1.0 Geometry Files. MIRO_Earth3 (calibrated) Jun 2010 170 Science Files, Geometry Files, RO-E-MIRO-3-EAR3-EARTH3-V1.0 MIRO_Cruise5 (raw) Nov 2010 60 Science Files, Engineering Files, RO-X-MIRO-2-CR5-CRUISE5-V1.00 Geometry Files. MIRO_Cruise5 (calibrated) Nov 2010 80 Science Files, Geometry Files, RO-X-MIRO-3-CR5-CRUISE5-V1.0 MIRO_Lutetia (raw) Mar 2011 300 Science Files, Engineering Files, RO-A-MIRO-2-AST2-LUTETIA-V1.0 Geometry Files. MIRO_Lutetia (calibrated) Mar 2011 420 Science Files, Geometry Files, RO-A-MIRO-3-AST2-LUTETIA-V1.0 MIRO_Rendezvous1 (raw) Mar 2008 50 Science Files, Engineering Files, RO-X-MIRO-2-RVM1-RENDEZVOUS1-V1.00 Geometry Files. MIRO_Rendezvous1 (calibrated) Mar 2008 70 Science Files, Geometry Files, RO-X-MIRO-3-RVM1-RENDEZVOUS1-V1.0 3.4.3 Directories This section describes the contents of each directory in a Data Product dataset. 3.4.3.1 Root Directory The following table lists the files located in the root directory. File Name File Contents AAREADME.TXT Introductory information about the contents and format of the volume. CALIBRATION Directory containing MIRO calibration data. CATALOG Directory containing catalog files: mission, instrument, and dataset Descriptions which are duplicated in the PDS higher-level catalog. DATA Root directory for each data type present in this volume: Science (Spectroscopic and Continum) and Engineering. DOCUMENT Directory containing basic documentation. ERRATA.TXT Cumulative listing of comments and corrections. GEOMETRY Directory containing information about spacecraft and target positions and instrument attitude, INDEX Directory containing index tables for the data files in this volume. LABEL Directory containing structure files references by PDS labels. SOFTWARE Directory containing software to manipulate and display MIRO data. VOLDESC.CAT Description of the contents of this volume in a PDS-labelled format. Appendix 1 contains a listing of the VOLDESC.CAT file for the first dataset listed in 3.4.2. 3.4.3.2 Calibration Directory This directory is to contain the calibration files used to convert level 2 products to level 3. Since the MIRO calibration data are part of the normal telemetry stream and are included in the files in the DATA directoriy, at this time no separate calibration files exist. Therefore, this directory is omitted for both level-2 and level-3 archives in the current deliveries. 3.4.3.3 Catalog Directory This directory contains files providing a top-level descirption of the Rosetta mission and spacecraft, the MIRO instrument and its team, and its data products. The following table describes the files in the Catalog Directory. File Name File Contents CATINFO.TXT A description of the contents of this directory. MISSION.CAT PDS mission catalog information about the Rosetta. TARGET.CAT . PDS catalog information about the target bodies observed by Rosetta. INSTHOST.CAT PDS instrument catalog information about the Rosetta Spacecraft. INST.CAT PDS instrument catalog information about the MIRO instrument. PERSONNEL.CAT PDS personnel catalog information about the MIRO Team members responsible for generating the data products. REF.CAT PDS references mentioned in other files. SOFTWARE.CAT PDS catalog information about software included in this archive (currently empty). DATASET.CAT PDS data set catalog information about the MIRO Data Product data sets. 3.4.3.4 Data Directory This directory contains three sub-directories, Spectroscopic, Continuum, and Engineering, which each contain all the data files for the corresponding data type in the data set. 3.4.3.4.1 Continuum Data Directory This directory contains science data files containing Continuum (MM and SMM) data, and their detached labels. 3.4.3.4.2 Engineering Data Directory This directory contains files containing Engineering data, and their detached labels. 3.4.3.4.3 Spectroscopic Data Directory This directory contains science data files containing Spectroscopic (CTS) data, and their detached labels. 3.4.3.5 Index Directory This directory contains index files providing summary information for all the data products in this data set. The following table describes the files in the Index Directory. File Name File Contents INDEX.LBL A volume index file. INDEXINFO.TXT A description of the contents of this directory. SPECINDX.TAB Index table file for all Spectroscopic data products. SPECINDX.LBL Detached label file describing the contents of specindx.tab. CONTINDX.TAB Index table file for all Continuum data products. CONTINDX.LBL Detached label file describing the contents of contindx.tab. ENGINDX.TAB Index table file for all Engineering data products. ENGINDX.LBL Detached label file describing the contents of engindx.tab. GEOMINDX.TAB Index table file for all Geometry files (not present if data set includes no Geometry files). GEOMINDX.LBL Detached label file describing the contents of geomindx.tab files (not present if data set includes no Geometry files). 3.4.3.6 Label Directory This directory includes files referenced by data files on this volume, e.g. FMT files containing header descriptions. Sample structure files used in MIRO PDS labels are given in Appendix 2. 3.4.3.7 Document Directory This directory contains various files documenting the contents of this data set. The following table describes the files in the Document Directory. File Name File Contents DOCINFO.TXT A description of the contents of this directory. MIRO_READ_DATA.ASC A Fortran-77 program to list selected parts of MIRO data files, intended primarily as additional documentation for the structure files in Appendix 2. UTCCON.ASC A Fortran-77 program that converts between the time system used in the data files and standard UTC notation. Other documents, as appropriate. E.g., in the Groundtesting delivery, log files of the tests are included. 3.4.3.8 Geometry Directory This directory contains files pertaining to the geometry and attitude information required to interpret or process any of the MIRO data in the delivery. It will be omitted if not necessary, e.g., for the Groundtesting dataset. 3.4.3.9 Software Directory It is intended that the software used to calibrate the data will be included in this directory for level-3 products. Currently, this software is in an early stage of development and is tied to the local database used by the processing, hence is not suitable for delivery to the archive at this time. The description of the algorithms in section 2.3.3.2 fulfills this function, for now. Therefore, this directory was omitted in the current deliveries. 3.4.4 Data and Label Files Science and Engineering data files are placed in the appropriate subdirectories of the data directory (3.4.3.4), together with their detached labels. Other data files shall be placed in their appropriate directories, all with detached PDS label. 4. Detailed Interface Specifications In this chapter, detailed information about the archive design at instrument and detector level is given. 4.1 Data Product Identification The basic MIRO data product is a binary file containing scientific or ancillary data in table format, and an associated detached label file in PDS format describing the data. The filenaming convention for these files is given in 3.1.3. A data file contains a continuous stream of data for one of the MIRO instruments (CTS, MM radiometer, or SUBMM radiometer) or for Engineering, see section 2.3. Note that the Data Mode in which the data were taken (section 2.3.2) is not relevant to the type of the data product, although the mode information for each row of the table is stored in the file. The length of a data file is arbitrary, being defined by the process of obtaining the data from the database, but it shall not exceed an observing time of one week 4.2 PDS Label Structure, Definition and Format The following keywords are used in the PDS labels for MIRO data products (with the values given when these will be invariant): PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE RECORD_TYPE = FIXED_LENGTH RECORD_BYTES FILE_RECORDS ^TABLE DATA_SET_NAME DATA_SET_ID MISSION_NAME = "INTERNATIONAL ROSETTA MISSION" MISSION_ID = ROSETTA INSTRUMENT_HOST_NAME = "ROSETTA ORBITER" INSTRUMENT_HOST_ID = RO INSTRUMENT_NAME = "MICROWAVE INSTRUMENT FOR THE ROSETTA ORBITER" INSTRUMENT_ID = MIRO INSTRUMENT_TYPE = {"RADIOMETER","SPECTROMETER"} ^INSTRUMENT_DESCRIPTION = "RO-MIR-IF-0001_16.TXT" INSTRUMENT_MODE_ID INSTRUMENT_MODE_DESC TARGET_NAME TARGET_TYPE MISSION_PHASE_NAME ORBIT_NUMBER SPACECRAFT_CLOCK_START_COUNT SPACECRAFT_CLOCK_STOP_COUNT START_TIME STOP_TIME SC_SUN_POSITION_VECTOR SC_TARGET_POSITION_VECTOR SC_TARGET_VELOCITY_VECTOR SUB_SPACECRAFT_LATITUDE SUB_SPACECRAFT_LONGITUDE SPACECRAFT_ALTITUDE NOTE = " The values of the keywords SC_SUN_POSITION_VECTOR, SC_TARGET_POSITION_VECTOR and SC_TARGET_VELOCITY_VECTOR are related to the ECLIPJ2000 reference frame. The values of SUB_SPACECRAFT_LATITUDE and SUB_SPACECRAFT_LONGITUDE are northren latitude and eastern longitude in the standard planetocentric IAU frame. All values are computed for the time 20xx-xx-xxTxx:xx:xx.xxx, the midpoint of the observations. Distances are given in , velocities in , angles in ." PRODUCT_CREATION_TIME PRODUCT_ID PRODUCT_TYPE PROCESSING_LEVEL_ID PRODUCER_FULL_NAME = "Dr. Samuel Gulkis" PRODUCER_INSTITUTION_NAME = "JET PROPULSION LABORATORY" PRODUCER_ID = JPL DATA_QUALITY_ID DATA_QUALITY_DESC = "1 = nominal, 2 = problematical" OBJECT = TABLE INTERCHANGE_FORMAT = BINARY COLUMNS ROWS ROW_BYTES ^STRUCTURE = "xxxx.FMT" END_ OBJECT = TABLE END The FMT file pointed to by the ^STRUCTURE keyword will be one of the five files in Appendix 2 (see 3.4.3.6). These contain the detailed specification of the contents of the data. The file pointed to by the ^INSTRUMENT_DESCRIPTION resides in the Document directory (3.4.3.7). No mission-specific keywords will be used. All keywords are defined in the PDS data dictionary (AD3 or online at http://pds.nasa.gov/tools/data_dictionary_lookup.cfm). The coordinate system used for the geometric items in the label (SC...VECTOR) ia the J2000 system, which is an inertial cartesian frame based on the Earth mean equator of Epoch J2000. 4.3 Overview of Detectors 4.3.1 Spectrometer data The contents of the spectrometer (CTS) level-2 and level-3 data products are fully defined by the structure files CTS_LEVEL_2_FORMAT.FMT, listed in Appendix 6.1, and CTS_LEVEL_3_FORMAT.FMT, listed in Appendix 6.2. Sample record printouts generated by the program MIRO_READ_DATA found in the DOCUMENT directory are also shown in those appendices. For further details, see MIRO User Manual (AD4) 6.2.3. 4.3.2 Radiometer (continuum) data The contents of the mm and submm radiometer level-2 and level-3 data products are fully defined by the structure files CONT_LEVEL_2_FORMAT.FMT, listed in Appendix 6.3 and CONT_LEVEL_3_FORMAT.FMT, listed in Appendix 6.4. Sample record printouts generated by the program MIRO_READ_DATA found in the DOCUMENT directory are also shown in those appendices. For further details, see MIRO User Manual (AD4) 6.2.4 and 6.2.5. 4.3.3 Engineering data The contents of the Engineering data products are fully defined by the structure file ENG_LEVEL_2_FORMAT.FMT, listed in Appendix 6.5. A sample record printout generated by the program MIRO_READ_DATA found in the DOCUMENT directory is also shown in that appendix. For further details, see MIRO User Manual (AD4) 6.2.2. 4.4 Data Format Description The contents of the MIRO data files are fully defined by the *.FMT files in the LABEL directories of the archives. Here, a brief explanation is provided of the science-data portion of CTS and Continuum files. (The Engineering files are not discussed further as they are not likely to be of interest to the general user.) It is important to understand that the Data colum of the MIRO science files contains a large data array in each row. In the CTS files, this contains a complete spectrum, whereas in the Continuum files this is a packet of data in time order. The name of the Data column is SPECTRAL_DATA in the CTS files, but simply D in the Continuum files. The layout of a MIRO science file can be viewed as a 2-D array with N rows (where N is the value of the FILE_RECORDS keyword in the label), each row containing M entries, with a "header" on the left- hand side, consisting of the columns preceding the Data column of the table). For Level-3 CTS files: M = 4250 spectral items and the header contains 18 items; for Level-2 CTS files: M = 4096 spectral items and the header contains 10 items, one of which is itself an array of 24 items; for all Continuum files: M = 200 data items and the header contains 12 items; additionally, Level-3 Continuum files contain a timestamp (UTC) at the end of each row, forming a "footer". When program MIRO_READ_DATA (see Section 3.4.3.7) is used in the "formatted output" mode, it prints, for each row, one entry each for the header columns and then four entries for the Data column, starting with the "starting data item #" that the program prompts for. (Four was picked for the number of entries arbitrarily, just to give a representative sample.) When the program is run in "average spectrum" mode, then it prints all entries of the Data column to a file, averaged over the rows specified. This allows the user to save these data for purposes of plotting or analyisis. (The averaging feature is most useful for the CTS data, while for Continuum data single packets are more meaningful.) A very important item is the Cal/No-cal flag in Column 6. When this flag is 0, then the spectrum is for a calibration sequence, and the data are brightness temperatures; furthermore, the targets are either sky, cold load or warm load, depending on the value of the Mirror position flag in column 2. However, when the Cal/No-cal flag is 1, then the data are difference spectra between the two LO states, so will be close to zero on average. Only the Cal=1 data (and the Sky data for Cal=0) are the observational data for the target body. (It is unfortunate that Cal=0 means calibration, but this is a historical accident and cannot now be changed.) See Appendix 3 (Section 7) for a description of an IDL-based tool to read MIRO data that is provided by PDS, called READPDS. Frequency calibration: the total bandwidth of MIRO is 180 MHz, with the frequency going inversely with the bin (channel) number of the CTS spectra, in an approximately linear fashion. The exact dependence is dependent on the temperature, which is why the number of bins are increased from 4096 for the raw data to 4250 for the calibrated data. This is described in the document CTS_FREQUENCY_CALIBRATION.PDF in the DOCUMENT directories of the Level-3 archives. This also describes how the true frequencies of the lines observed (which span 33 GHz, far more than the nominal bandwidth) are mapped into the CTS spectrum. Discontinuities between the eight regions of the different mappings appear as smooth transitions, because of the design of the CTS. Data in the transition regions between these bands are not usable. 5. Appendix 1: VOLDESC.CAT PDS_VERSION_ID = PDS3 RECORD_TYPE = "STREAM" RECORD_BYTES = "UNK" OBJECT = VOLUME VOLUME_SERIES_NAME = " ROSETTA SCIENCE ARCHIVE" VOLUME_SET_NAME = " ROSETTA: MIRO DATA" VOLUME_SET_ID = " USA_NASA_JPL_ROMIR_1000" VOLUMES = 1 VOLUME_NAME = " RAW MIRO DATA FOR THE GROUND PHASE" VOLUME_ID = " ROMIR_1001" VOLUME_VERSION_ID = " VERSION 1" VOLUME_FORMAT = " ISO-9660" DATA_SET_ID = "RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0" MEDIUM_TYPE = "ELECTRONIC" PUBLICATION_DATE = 2006-11-06 DESCRIPTION = "This volume is the first containing Microwave Instrument for the Rosetta Orbiter (MIRO) data. It contains data obtained during ground testing at NASA/JPL." OBJECT = DATA_PRODUCER INSTITUTION_NAME = "JET PROPULSION LABORATORY" FACILITY_NAME = "MIRO DATA PROCESSING TEAM" FULL_NAME = "SAMUEL GULKIS" ADDRESS_TEXT = "JET PROPULSION LABORATORY \N 4800 OAK GROVE DRIVE \n MAILSTOP 183-301 \n PASADENA, CA 91109 \n USA" END_OBJECT = DATA_PRODUCER OBJECT = CATALOG ^MISSION_CATALOG = "MISSION.CAT" ^INSTRUMENT_HOST_CATALOG = "INSTHOST.CAT" ^INSTRUMENT_CATALOG = "INST.CAT" ^DATA_SET_CATALOG = "DATASET.CAT" ^REFERENCE_CATALOG = "REF.CAT" ^PERSONNEL_CATALOG = "PERSONNEL.CAT" ^SOFTWARE_CATALOG = "SOFTWARE.CAT" ^TARGET_CATALOG = "TARGET.CAT" END_OBJECT = CATALOG END_OBJECT = VOLUME END 6. Appendix 2: Structure Files 6.1 Spectrometer Level 2 Data (see section 4.3.1) Filename: CTS_LEVEL_2_FORMAT.FMT Rosetta/miro cts raw data structure This structure label gives the data structure for the data decommutated from the telemetry for the uncalibrated (raw) data from the MIRO Chirp Transform Spectrometer (CTS). OBJECT = COLUMN NAME = TIME COLUMN_NUMBER = 1 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 1 BYTES = 8 DESCRIPTION = "Time of acquisition of the spectrum in elapsed UTC seconds after 1-Jan-1970 (see EAICD Section 3.2.2)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MIRPOS COLUMN_NUMBER = 2 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 9 BYTES = 1 DESCRIPTION = "Mirror position: 1: sky, 2: cold target, 3: warm target" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POWERMODE COLUMN_NUMBER = 3 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 10 BYTES = 1 DESCRIPTION = "Values 1-6 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = INTEGRATION COLUMN_NUMBER = 4 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 11 BYTES = 1 DESCRIPTION = "Values 0-3 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMOOTHING COLUMN_NUMBER = 5 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 12 BYTES = 1 DESCRIPTION = "Values 0-3 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = CAL COLUMN_NUMBER = 6 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 13 BYTES = 1 DESCRIPTION = "0: Calibration in progress, 1: No calibration in progress"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = LO COLUMN_NUMBER = 7 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 14 BYTES = 1 DESCRIPTION = "LO designation, 0 or 1" END_OBJECT = COLUMN OBJECT = COLUMN NAME = NUMPLL COLUMN_NUMBER = 8 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I2 START_BYTE = 15 BYTES = 1 DESCRIPTION = "Number of used pll (phased-lock-loop) bytes" END_OBJECT = COLUMN OBJECT = COLUMN NAME = PLL_DATA COLUMN_NUMBER = 9 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = 24I1 START_BYTE = 16 BYTES = 24 ITEMS = 24 ITEM_BYTES = 1 DESCRIPTION = "pll (phased-lock-loop) status bytes as described in MIRO User Manual 6.2.3." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ASTEROID COLUMN_NUMBER = 10 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 40 BYTES = 1 DESCRIPTION = "Asteroid mode: 0: in asteroid mode, 1: not in asteroid mode, 4 as described In MIRO User Manual 6.1.2.2." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECTRAL_DATA COLUMN_NUMBER = 11 DATA_TYPE = MSB_INTEGER FORMAT = 4096I9 START_BYTE = 41 BYTES = 16384 ITEMS = 4096 ITEM_BYTES = 4 DESCRIPTION = "Uncalibrated brightness temperature as signed integer" END_OBJECT = COLUMN The following is an example of the first record of a Level-2 Spectroscopic file, with just 4 of the 4250 data fields shown, in both hex and formatted representations: Listing of rows 1 to 1 for file RO-E-MIRO-2-EAR1-EARTH1- V1.0/DATA/SPECTROSCOPIC/MIRO_2_CTS_20050630809.DAT COL.#: 1 2 3 4 5 6 7 8 9 10 11 ITEMS: 41D08A0D4F32378B 02 01 00 00 00 00 06 80 80 80 80 80 80 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00974000 009A8000 0097C000 009B4000 COL.#: 1 2 3 4 5 6 7 8 9 10 11 ITEMS: 1.109931325E+09 2 1 0 0 0 0 6 128 128 128 128 128 128 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 9912320 10125312 9945088 10174464 6.2 Spectrometer Level 3 Data (see section 4.3.1) Filename: CTS_LEVEL_3_FORMAT.FMT Rosetta/miro cts calibrated data structure This structure label gives the data structure for the calibrated data from the MIRO Chirp Transform Spectrometer (CTS). OBJECT = COLUMN NAME = TIME COLUMN_NUMBER = 1 DATA_TYPE = IEEE_REAL START_BYTE = 1 BYTES = 8 DESCRIPTION = "Time of acquisition of the spectrum in elapsed UTC seconds after 1-Jan-1970 (see EAICD Section 3.2.2)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MIRPOS COLUMN_NUMBER = 2 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 9 BYTES = 1 DESCRIPTION = "Mirror position: 1: sky, 2: cold target, 3: warm target" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POWERMODE COLUMN_NUMBER = 3 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 10 BYTES = 1 DESCRIPTION = "Values 1-6 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = INTEGRATION COLUMN_NUMBER = 4 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 11 BYTES = 1 DESCRIPTION = "Values 0-3 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMOOTHING COLUMN_NUMBER = 5 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 12 BYTES = 1 DESCRIPTION = "Values 0-3 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = CAL COLUMN_NUMBER = 6 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 13 BYTES = 1 DESCRIPTION = "0: Calibration in progress, 1: No calibration in progress"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = LO COLUMN_NUMBER = 7 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 14 BYTES = 1 DESCRIPTION = "LO designation, 0 or 1" END_OBJECT = COLUMN OBJECT = COLUMN NAME = ASTEROID COLUMN_NUMBER = 8 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 15 BYTES = 1 DESCRIPTION = "Asteroid mode: 0: in asteroid mode, 1: not in asteroid mode, 4 as described in MIRO User Manual 6.1.2.2." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T1 COLUMN_NUMBER = 9 DATA_TYPE = IEEE_REAL FORMAT = F6.2 START_BYTE = 16 BYTES = 4 DESCRIPTION = "Engineering temperature of CTS (degrees C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = TYPE COLUMN_NUMBER = 10 DATA_TYPE = CHARACTER FORMAT = A1 START_BYTE = 20 BYTES = 1 DESCRIPTION = "Type of calibration data used: C = cold, S = sky" END_OBJECT = COLUMN OBJECT = COLUMN NAME = STATUS COLUMN_NUMBER = 11 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 21 BYTES = 1 DESCRIPTION = "Status flag: 0 = nominal, <0 = problematical, >0 = TBD" END_OBJECT = COLUMN OBJECT = COLUMN NAME = METHOD COLUMN_NUMBER = 12 DATA_TYPE = CHARACTER FORMAT = A1 START_BYTE = 22 BYTES = 1 DESCRIPTION = "Method of calibration: A = average, I = interpolate, N = nearest neighbor" END_OBJECT = COLUMN OBJECT = COLUMN NAME = PLL COLUMN_NUMBER = 13 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I4 START_BYTE = 23 BYTES = 1 DESCRIPTION = "Logical OR of the PLL bytes in the raw record, indicating phased-lock loop status" END_OBJECT = COLUMN OBJECT = COLUMN NAME = RA COLUMN_NUMBER = 14 DATA_TYPE = IEEE_REAL FORMAT = F7.3 UNIT = DEGREE START_BYTE = 24 BYTES = 4 DESCRIPTION = "Right Ascension of the MIRO boresight" END_OBJECT = COLUMN OBJECT = COLUMN NAME = DEC COLUMN_NUMBER = 15 DATA_TYPE = IEEE_REAL FORMAT = F7.3 UNIT = DEGREE START_BYTE = 28 BYTES = 4 DESCRIPTION = "Declination of the MIRO boresight" END_OBJECT = COLUMN OBJECT = COLUMN NAME = VEL COLUMN_NUMBER = 16 DATA_TYPE = IEEE_REAL FORMAT = E11.3 UNIT = KILOMETER_PER_SECOND START_BYTE = 32 BYTES = 4 DESCRIPTION = "Relative velocity" END_OBJECT = COLUMN OBJECT = COLUMN NAME = S0 COLUMN_NUMBER = 17 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 36 BYTES = 4 DESCRIPTION = "Spare" END_OBJECT = COLUMN OBJECT = COLUMN NAME = S1 COLUMN_NUMBER = 18 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 40 BYTES = 4 DESCRIPTION = "Spare" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECTRAL_DATA COLUMN_NUMBER = 19 DATA_TYPE = IEEE_REAL FORMAT = 4250F6.0 UNIT = KELVIN START_BYTE = 44 BYTES = 17000 ITEMS = 4250 ITEM_BYTES = "Antenna temperatures" END_OBJECT = COLUMN The following is an example of the first record of a Level-3 Spectroscopic file, with just 4 of the 4250 data fields shown, in both hex and formatted representations: Listing of rows 1 to 1 for file RO-E-MIRO-3-EAR1-EARTH1- V1.0/DATA/SPECTROSCOPIC/MIRO_3_CTS_20050631015.DAT COL.#: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 ITEMS: 41D08A0D4F32378B 02 01 00 00 00 00 00 4287CCCD 53 00 4E 80 00000000 00000000 00000000 00000000 00000000 467FDAAA 467EF66D 4685B9FD 46889DD2 COL.#: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 ITEMS: 1.109931325E+09 2 1 0 0 0 0 0 6.790E+01 S 0 N 128 0.000E+00 0.000E+00 0.000E+00 0.000E+00 0.000E+00 1.637E+04 1.632E+04 1.712E+04 1.749E+04 6.3 Continuum Level 2 Data (see section 4.3.2) Filename: CONT_LEVEL_2_FORMAT.FMT Rosetta/MIRO continuum files raw data structure This structure label gives the data structure for the data decommutated from the telemetry for the uncalibrated (raw) data from the MIRO Millimeter and Submillimeter Continuum Radiometers. OBJECT = COLUMN NAME = TIME COLUMN_NUMBER = 1 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 1 BYTES = 8 DESCRIPTION = "Time of start of acquisition of the data in elapsed UTC seconds after 1-Jan-1970 (see EAICD Section 3.2.2)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME1 COLUMN_NUMBER = 2 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 9 BYTES = 8 DESCRIPTION = "Time of acquisition of the 100th element of the raw data array, if summation=1, or of the 50th element if summation=2 or greater; this is zero if summation=0." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME2 COLUMN_NUMBER = 3 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 17 BYTES = 8 DESCRIPTION = "Time of acquisition of the 100th element of the raw data array, if summation=2 or greater; otherwise zero." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME3 COLUMN_NUMBER = 4 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 25 BYTES = 8 DESCRIPTION = "Time of acquisition of the 150th element of the raw data array, if summation=2 or greater; otherwise zero." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MIRPOS COLUMN_NUMBER = 5 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 33 BYTES = 1 DESCRIPTION = "Mirror position: 1: sky, 2: cold target, 3: warm target" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POWERMODE COLUMN_NUMBER = 6 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 34 BYTES = 1 DESCRIPTION = "Values 1-6 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SUMMATION COLUMN_NUMBER = 7 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 35 BYTES = 1 DESCRIPTION = "Values 0-4 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = ND COLUMN_NUMBER = 8 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I3 START_BYTE = 36 BYTES = 1 DESCRIPTION = "Number of elements in raw data array; should always be 200." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MMSUBTRACTION COLUMN_NUMBER = 9 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I5 START_BYTE = 37 BYTES = 2 DESCRIPTION = "Offset in millimeter continuum data, as described in MIRO User Manual 6.2.5." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMMSUBTRACTION COLUMN_NUMBER = 10 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I5 START_BYTE = 39 BYTES = 2 DESCRIPTION = "Offset in submillimeter continuum data, as described in MIRO User Manual 6.2.4." END_OBJECT = COLUMN OBJECT = COLUMN NAME = CALMODE COLUMN_NUMBER = 11 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 41 BYTES = 2 DESCRIPTION = "0: Calibration in progress, 1: No calibration in progress" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SP COLUMN_NUMBER = 12 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 43 BYTES = 2 DESCRIPTION = "Spare, not used" END_OBJECT = COLUMN OBJECT = COLUMN NAME = D COLUMN_NUMBER = 13 DATA_TYPE = MSB_INTEGER FORMAT = 200I6 START_BYTE = 45 BYTES = 400 ITEMS = 200 ITEM_BYTES = 2 DESCRIPTION = "Uncalibrated brightness temperature as signed integer" END_OBJECT = COLUMN The following is an example of the first record of a Level-2 Continuum file, with just the first 4 of the 200 data fields shown, in both hex and formatted representations: Listing of rows 1 to 1 for file RO-E-MIRO-2-EAR1-EARTH1- V1.0/DATA/CONTINUUM/MIRO_2_MM_20050630809.DAT COL.#: 1 2 3 4 5 6 7 8 9 10 11 12 13 ITEMS: 41D08A0D4F339485 41D08A0D508AF41F 0000000000000000 0000000000000000 02 01 00 C8 0000 0000 0000 0000 1CA9 1CAB 1CAB 1CAA COL.#: 1 2 3 4 5 6 7 8 9 10 11 12 13 ITEMS: 1.109931325E+09 1.109931330E+09 0.000000000E+00 0.000000000E+00 2 1 0 200 0 0 0 0 7337 7339 7339 7338 6.4 Continuum Level 3 Data (see section 4.3.2) Filename: CONT_LEVEL_3_FORMAT.FMT Rosetta/MIRO continuum files raw data structure This structure label gives the data structure for the calibrated data from the MIRO Millimeter and Submillimeter Continuum Radiometers. OBJECT = COLUMN NAME = TIME COLUMN_NUMBER = 1 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 1 BYTES = 8 DESCRIPTION = "Time of start of acquisition of the data in elapsed UTC seconds after 1-Jan-1970 (see EAICD Section 3.2.2)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME1 COLUMN_NUMBER = 2 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 9 BYTES = 8 DESCRIPTION = "Time of acquisition of the 100th element of the raw data array, if summation=1, or of the 50th element if summation=2 or greater; this is zero if summation=0." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME2 COLUMN_NUMBER = 3 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 17 BYTES = 8 DESCRIPTION = "Time of acquisition of the 100th element of the raw data array, if summation=2 or greater; otherwise zero." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME3 COLUMN_NUMBER = 4 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 25 BYTES = 8 DESCRIPTION = "Time of acquisition of the 150th element of the raw data array, if summation=2 or greater; otherwise zero." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MIRPOS COLUMN_NUMBER = 5 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 33 BYTES = 1 DESCRIPTION = "Mirror position: 1: sky, 2: cold target, 3: warm target" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POWERMODE COLUMN_NUMBER = 6 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 34 BYTES = 1 DESCRIPTION = "Values 1-6 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SUMMATION COLUMN_NUMBER = 7 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 35 BYTES = 1 DESCRIPTION = "Values 0-4 as described in MIRO User Manual 6.1.2.1"" END_OBJECT = COLUMN OBJECT = COLUMN NAME = ND COLUMN_NUMBER = 8 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I3 START_BYTE = 36 BYTES = 1 DESCRIPTION = "Number of elements in raw data array; should always be 200." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MMSUBTRACTION COLUMN_NUMBER = 9 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I5 START_BYTE = 37 BYTES = 2 DESCRIPTION = "Offset in millimeter continuum data, as described in MIRO User Manual 6.2.5." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMMSUBTRACTION COLUMN_NUMBER = 10 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 39 BYTES = 2 DESCRIPTION = "Offset in submillimeter continuum data, as described in MIRO User Manual 6.2.4." END_OBJECT = COLUMN OBJECT = COLUMN NAME = CALMODE COLUMN_NUMBER = 11 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 41 BYTES = 2 DESCRIPTION = "0: Calibration in progress, 1: No calibration in progress" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SP COLUMN_NUMBER = 12 DATA_TYPE = UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 43 BYTES = 2 DESCRIPTION = "Spare, not used" END_OBJECT = COLUMN OBJECT = COLUMN NAME = D COLUMN_NUMBER = 13 DATA_TYPE = IEEE_REAL FORMAT = 200F6.0 UNIT = KELVIN START_BYTE = 45 BYTES = 800 ITEMS = 200 ITEM_BYTES = 4 DESCRIPTION = "Antenna temperatures" END_OBJECT = COLUMN The following is an example of the first record of a Level-3 Continuum file, with just the first 4 of the 200 data fields shown, in both hex and formatted representations: Listing of rows 1 to 1 for file RO-E-MIRO-3-EAR1-EARTH1- V1.0/DATA/CONTINUUM/MIRO_3_MM_20050631017.DAT COL.#: 1 2 3 4 5 6 7 8 9 10 11 12 13 ITEMS: 41D08A0D6A110EAA 41D08A0D6B6223E2 0000000000000000 0000000000000000 01 01 00 C8 0000 0000 0001 0000 412CBA5D 4135BD7F 4135BD7F 413BBF95 COL.#: 1 2 3 4 5 6 7 8 9 10 11 12 13 ITEMS: 1.109931432E+09 1.109931438E+09 0.000000000E+00 0.000000000E+00 1 1 0 200 0 0 1 0 1.080E+01 1.136E+01 1.136E+01 1.173E+01 6.5 Housekeeping Data (see section 4.3.3) Filename: ENG_LEVEL_2_FORMAT.FMT Rosetta/MIRO engineering raw data structure This structure label gives the data structure for the data decommutated from the telemetry for the engineering (housekeeping) data from the MIRO instrument. */ OBJECT = COLUMN NAME = TIME COLUMN_NUMBER = 1 DATA_TYPE = IEEE_REAL FORMAT = F16.5 START_BYTE = 1 BYTES = 8 DESCRIPTION = "Time of acquisition of the data packet in elapsed UTC seconds after 1-Jan-1970 (see EAICD Section 3.2.2)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T1 COLUMN_NUMBER = 2 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 9 BYTES = 4 DESCRIPTION = "CTS Temperature sensor #1 Branch A (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T2 COLUMN_NUMBER = 3 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 13 BYTES = 4 DESCRIPTION = "CTS Temperature sensor #2 Branch A (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T3 COLUMN_NUMBER = 4 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 17 BYTES = 4 DESCRIPTION = "CTS Temperature sensor #1 Branch B (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T4 COLUMN_NUMBER = 5 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 21 BYTES = 4 DESCRIPTION = "CTS Temperature sensor #2 Branch B (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T5 COLUMN_NUMBER = 6 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 25 BYTES = 4 DESCRIPTION = "CTS Temperature sensor #1 analog tray (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPECT_T6 COLUMN_NUMBER = 7 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 29 BYTES = 4 DESCRIPTION = "CTS Temperature sensor #2 analog tray (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = EU_TEMP COLUMN_NUMBER = 8 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 33 BYTES = 4 DESCRIPTION = "Electronics Unit (EU) temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = ECAL_TEMP COLUMN_NUMBER = 9 DATA_TYPE = IEEE_REAL FORMAT = F5.0 START_BYTE = 37 BYTES = 4 DESCRIPTION = "Reference temperature (634 Ohms) (Digital Units)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_5V_EU COLUMN_NUMBER = 10 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 41 BYTES = 4 DESCRIPTION = "EU +5V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_12V_EU COLUMN_NUMBER = 11 DATA_TYPE = IEEE_REAL FORMAT = F6.3 START_BYTE = 45 BYTES = 4 DESCRIPTION = "EU +12V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = NEG_12V_EU COLUMN_NUMBER = 12 DATA_TYPE = IEEE_REAL FORMAT = F7.3 START_BYTE = 49 BYTES = 4 DESCRIPTION = "EU -12V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = 3V_EU COLUMN_NUMBER = 13 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 53 BYTES = 4 DESCRIPTION = "EU +3.3V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_24V_EU COLUMN_NUMBER = 14 DATA_TYPE = IEEE_REAL FORMAT = F6.3 START_BYTE = 57 BYTES = 4 DESCRIPTION = "EU +24V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_5V_ANA_EU COLUMN_NUMBER = 15 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 61 BYTES = 4 DESCRIPTION = "EU +5V analog voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_5V_CURR_EU COLUMN_NUMBER = 16 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 65 BYTES = 4 DESCRIPTION = "EU +5V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_12V_CURR_EU COLUMN_NUMBER = 17 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 69 BYTES = 4 DESCRIPTION = "EU +12V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = NEG_12V_CURR_EU COLUMN_NUMBER = 18 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 73 BYTES = 4 DESCRIPTION = "EU -12V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_24V_ANA_CURR_EU FORMAT = E11.3 COLUMN_NUMBER = 19 DATA_TYPE = IEEE_REAL START_BYTE = 77 BYTES = 4 DESCRIPTION = "EU +24V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = 3V_CURR_EU COLUMN_NUMBER = 20 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 81 BYTES = 4 DESCRIPTION = "EU +3V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_5V_ANA_CURR_EU COLUMN_NUMBER = 21 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 85 BYTES = 4 DESCRIPTION = "EU +5V analog current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = TLM_Heating COLUMN_NUMBER = 22 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 89 BYTES = 4 DESCRIPTION = "this item has been removed, see MIRO User Manual 6.2.2.5. END_OBJECT = COLUMN OBJECT = COLUMN NAME = TLM_RF COLUMN_NUMBER = 23 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 93 BYTES = 4 DESCRIPTION = "this item has been removed, see MIRO User Manual 6.2.2.5. END_OBJECT = COLUMN OBJECT = COLUMN NAME = CTS_V_ANA_1 COLUMN_NUMBER = 24 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 97 BYTES = 4 DESCRIPTION = "CTS PG1 Voltage (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = CTS_V_ANA_2 FORMAT = F5.3 COLUMN_NUMBER = 25 DATA_TYPE = IEEE_REAL START_BYTE = 101 BYTES = 4 DESCRIPTION = "CTS PG1 Voltage (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = COLD_LOAD1_TEMP COLUMN_NUMBER = 26 DATA_TYPE = IEEE_REAL FORMAT = F6.1 START_BYTE = 105 BYTES = 4 DESCRIPTION = "Cold load temperature #1 (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = COLD_LOAD2_TEMP COLUMN_NUMBER = 27 DATA_TYPE = IEEE_REAL FORMAT = F6.1 START_BYTE = 109 BYTES = 4 DESCRIPTION = "Cold load temperature #2 (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = WARM_LOAD1_TEMP COLUMN_NUMBER = 28 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 113 BYTES = 4 DESCRIPTION = "Warm load temperature #1 (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = OB_TEMP COLUMN_NUMBER = 29 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 117 BYTES = 4 DESCRIPTION = "Optical Bench temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = TELESCOPE1_TEMP COLUMN_NUMBER = 30 DATA_TYPE = IEEE_REAL FORMAT = F6.1 START_BYTE = 121 BYTES = 4 DESCRIPTION = "Telescope #1 temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = TELESCOPE2_TEMP COLUMN_NUMBER = 31 DATA_TYPE = IEEE_REAL FORMAT = F6.1 START_BYTE = 125 BYTES = 4 DESCRIPTION = "Telescope #2 temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = PLL_TEMP COLUMN_NUMBER = 32 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 129 BYTES = 4 DESCRIPTION = "Phase lock loop temerature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = IFP_DET_TEMP COLUMN_NUMBER = 33 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 133 BYTES = 4 DESCRIPTION = "smm IF processor detector temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = IFP_AMP_TEMP FORMAT = F5.1 COLUMN_NUMBER = 34 DATA_TYPE = IEEE_REAL START_BYTE = 137 BYTES = 4 DESCRIPTION = "smm IF processor amplifier temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMM_LO_GUNN COLUMN_NUMBER = 35 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 141 BYTES = 4 DESCRIPTION = "smm LO Gunn temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = MM_LO_GUNN COLUMN_NUMBER = 36 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 145 BYTES = 4 DESCRIPTION = "mm LO Gunn temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = MOTOR_TEMP COLUMN_NUMBER = 37 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 149 BYTES = 4 DESCRIPTION = "Mirror motor temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SEN_EL COLUMN_NUMBER = 38 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 153 BYTES = 4 DESCRIPTION = "Sensor Electronics Unit (SBEU) temperature (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = WARM_LOAD2_TEMP COLUMN_NUMBER = 39 DATA_TYPE = IEEE_REAL FORMAT = F5.1 START_BYTE = 157 BYTES = 4 DESCRIPTION = "Warm load temperature #2 (deg C)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = CAL_TEMP_LOW COLUMN_NUMBER = 40 DATA_TYPE = IEEE_REAL FORMAT = F3.0 START_BYTE = 161 BYTES = 4 DESCRIPTION = "Reference temperature 191 Ohms (digital units)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = CAL_TEMP_HIGH COLUMN_NUMBER = 41 DATA_TYPE = IEEE_REAL FORMAT = F4.0 START_BYTE = 165 BYTES = 4 DESCRIPTION = "Reference temperature 681 Ohms (digital units)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_5V_SBEU COLUMN_NUMBER = 42 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 169 BYTES = 4 DESCRIPTION = "SBEU +5V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_12V_1_SBEU COLUMN_NUMBER = 43 DATA_TYPE = IEEE_REAL FORMAT = F6.3 START_BYTE = 173 BYTES = 4 DESCRIPTION = "SBEU +12V voltage monitor #1 (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_12V_2_SBEU COLUMN_NUMBER = 44 DATA_TYPE = IEEE_REAL FORMAT = F6.3 START_BYTE = 177 BYTES = 4 DESCRIPTION = "SBEU +12V voltage monitor #2 (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = NEG_12V_SBEU COLUMN_NUMBER = 45 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 181 BYTES = 4 DESCRIPTION = "SBEU -12V voltage monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_5V_CURR_SBEU COLUMN_NUMBER = 46 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 185 BYTES = 4 DESCRIPTION = "SBEU +5V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_12V_CURR_1_SBEU COLUMN_NUMBER = 47 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 189 BYTES = 4 DESCRIPTION = "SBEU +12V current monitor #1 (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POS_12V_CURR_2_SBEU COLUMN_NUMBER = 48 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 193 BYTES = 4 DESCRIPTION = "SBEU +12V current monitor #2 (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = NEG_12V_CURR_SBEU COLUMN_NUMBER = 49 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 197 BYTES = 4 DESCRIPTION = "SBEU -12V current monitor (A)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = MM_GUNN_CURR COLUMN_NUMBER = 50 DATA_TYPE = IEEE_REAL FORMAT = F6.2 START_BYTE = 201 BYTES = 4 DESCRIPTION = "mm LO Gunn current (mA)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMM_Mult_CURR COLUMN_NUMBER = 51 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 205 BYTES = 4 DESCRIPTION = "smm multiplier current (mA)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMM_PLL_ERR COLUMN_NUMBER = 52 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 209 BYTES = 4 DESCRIPTION = "static phase error for smm PLL (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = FS1_ERR COLUMN_NUMBER = 53 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 213 BYTES = 4 DESCRIPTION = "Phase error for frequency synthesizer #1 (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = FS2_ERR COLUMN_NUMBER = 54 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 217 BYTES = 4 DESCRIPTION = "Phase error for frequency synthesizer #2 (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = FS3_ERR COLUMN_NUMBER = 55 DATA_TYPE = IEEE_REAL FORMAT = F5.3 START_BYTE = 221 BYTES = 4 DESCRIPTION = "Phase error for frequency synthesizer #3 (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMM_PLL_GUNN_CURR COLUMN_NUMBER = 56 DATA_TYPE = IEEE_REAL FORMAT = F6.2 START_BYTE = 225 BYTES = 4 DESCRIPTION = "smm Gunn oscillator current (via PLL) (mA)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMM_PLL_IF_PWR COLUMN_NUMBER = 57 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 229 BYTES = 4 DESCRIPTION = "smm PLL IF power monitor (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SMM_GDO_VOLTAGE COLUMN_NUMBER = 58 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 233 BYTES = 4 DESCRIPTION = "smm GDO bias voltage (V)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPAREF COLUMN_NUMBER = 59 DATA_TYPE = IEEE_REAL FORMAT = E11.3 START_BYTE = 237 BYTES = 4 DESCRIPTION = "spare" END_OBJECT = COLUMN OBJECT = COLUMN NAME = MIRPOS COLUMN_NUMBER = 60 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 241 BYTES = 1 DESCRIPTION = "Mirror position: 1: sky, 2: cold load, 3: warm load" END_OBJECT = COLUMN OBJECT = COLUMN NAME = POWERMODE COLUMN_NUMBER = 61 DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = I1 START_BYTE = 242 BYTES = 1 DESCRIPTION = "Values 1-6 as described in MIRO User Manual 6.1.2.1.5" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SUCR0 COLUMN_NUMBER = 62 DATA_TYPE = CHARACTER FORMAT = A2 START_BYTE = 243 BYTES = 2 DESCRIPTION = "Low order bits 0-15 of Sensor Unit Control Register" OBJECT = BIT_COLUMN NAME = HSKMUX START_BIT = 1 BITS = 5 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z5 DESCRIPTION = "Selects housekeeping channel" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NON5VSMM START_BIT = 6 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Commands +5V, +/-12V on after -5V is commanded using smm cont mode" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = IFPCTL0 START_BIT = 7 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Bit 0 of 4 bit ifp power control setting" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = IFPCTL1 START_BIT = 8 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Bit 1 of 4 bit ifp power control setting" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = MMLNAON START_BIT = 9 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Powers on mm LNA bias 0 = on, 1 = off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = SMMLNAON START_BIT = 10 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Powers on smm LNA bias 0 = on, 1 = off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NON5VMM START_BIT = 11 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Commands +5V, +/-12V on after -5V is commanded using mm cont mode" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NON5VSPC START_BIT = 12 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Commands +5V, +/-12V on after -5V is commanded using cts mode" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = PLLRESET START_BIT = 13 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Phase-lock reset (0 locks, 1 unlocks) CF User Manual V6.2-7" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = IFPCTL2 START_BIT = 14 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Bit 2 of 4 bit ifp power control setting" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = IFPCTL3 START_BIT = 15 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Bit 3 of 4 bit ifp power control setting (MSB)" END_OBJECT = BIT_COLUMN END_OBJECT = COLUMN OBJECT = COLUMN NAME = SUCR16 COLUMN_NUMBER = 63 DATA_TYPE = CHARACTER FORMAT = A2 START_BYTE = 244 BYTES = 2 DESCRIPTION = "High order bits 16-31 of Sensor Unit Control Register" END_OBJECT = COLUMN OBJECT = BIT_COLUMN NAME = SMMGUNNOSCV START_BIT = 1 BITS = 4 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z4 DESCRIPTION = "Setting for voltage to smm Gunn oscillator" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = MMGUNNOSCV START_BIT = 5 BITS = 4 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z4 DESCRIPTION = "Setting for voltage to mm Gunn oscillator" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NEG5VSMM START_BIT = 9 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Set -5V for smm continuum mode" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NEG5VMM START_BIT = 10 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Set -5V for mm continuum mode" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NEG5VCTS START_BIT = 11 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Set -5V for cts mode" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = LDFRQ START_BIT = 12 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Set and cleared to load the 3 fequency synthsizer chips"" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = MIRROROFF START_BIT = 13 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "0: Mirror power on, 1: Mirror power off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = MIRRORBACK START_BIT = 14 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "1: backward mirror motion, 0: forward mirror motion" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = SMMFRQSW START_BIT = 15 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Set LO = 0 or 1 when frequency swtiching is on" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = PINPULLER START_BIT = 16 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Set and cleared to activate mirror pin puller" END_OBJECT = BIT_COLUMN END_OBJECT = COLUMN OBJECT = COLUMN NAME = ADDR100 COLUMN_NUMBER = 64 DATA_TYPE = CHARACTER FORMAT = A2 START_BYTE = 246 BYTES = 2 DESCRIPTION = "Bits from address 100" OBJECT = BIT_COLUMN NAME = EMUX START_BIT = 1 BITS = 5 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z5 DESCRIPTION = "Bits 0-5 set corresponding EMUX, 0-5" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = SND2SU START_BIT = 6 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Send command register data to Sensor Unit" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = MOTSTEP START_BIT = 7 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Enable motor stepping" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = LDENABLE START_BIT = 8 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "1: Enable load, 0: Disable load"" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = POS12VSPEC START_BIT = 9 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "+12V Spectrometer on, 1: On, 0: Off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = POS5VSPEC START_BIT = 10 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "+5V Spectrometer on, 1: On, 0: Off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = POS5VANA START_BIT = 11 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "+5V Analog spectrometer on, 1: On, 0: Off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = POS3VSPEC START_BIT = 12 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "+3V Spectrometer on, 1: On, 0: Off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = NEG12VSPEC START_BIT = 13 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "-12V Spectrometer on, 1: On, 0: Off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = USO24V START_BIT = 14 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "+24V USO on, 1: On, 0: Off" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = CALHTRON START_BIT = 15 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "Calibration Heater On, 0: Off, 1: On" END_OBJECT = BIT_COLUMN OBJECT = BIT_COLUMN NAME = CTSTRISTORE START_BIT = 16 BITS = 1 BIT_DATA_TYPE = MSB_UNSIGNED_INTEGER FORMAT = Z1 DESCRIPTION = "CTS Tri-state, 1: disable, 0: enable" END_OBJECT = BIT_COLUMN END_OBJECT = COLUMN The following is an example of the first record of an Engineering file, with just the first 4 of the 58 engineering data fields shown, in both hex and formatted representations: Listing of rows 1 to 2 for file RO-CAL-MIRO-2-GRND-THERMALVAC- V1.0/DATA/ENGINEERING/MIRO_2_HSK_20011410000.DAT COL.#: 1 2 3 4 5 60 61 62 63 64 ITEMS: 41CD8476E0294984 C19DCEA5 41C03E77 41BF872B 41C042C4 01 06 0000 1004 0000 ITEMS: 41CD8476E5C2F683 41C00553 41C08312 41BFCC30 41C042C4 01 06 001F 1004 0000 Listing of rows 1 to 2 for file RO-CAL-MIRO-2-GRND-THERMALVAC- V1.0/DATA/ENGINEERING/MIRO_2_HSK_20011410000.DAT COL.#: 1 2 3 4 5 60 61 62 63 64 ITEMS: 9.904408963E+08 -1.973E+01 2.403E+01 2.394E+01 2.403E+01 1 6 0 4100 0 7. Appendix 3: Available Software to read PDS files The MIRO data files can be read by PDS-supported software such as NASAVIEW. Currently, the software used by the MIRO team to process the data files is code written by individual team members in IDL. PDS discourages the archiving of software, since it is generally difficult to maintain and port as available hardware evolves. Furthermore, IDL is a proprietary product. A simple Fortran-77 program to read and print out selected parts of the MIRO data files is included in the DOCUMENT directory, named MIRO_READ_DATA (see Section 3.4.3.7). It is described in Section 4.4. It should be emphasised that program MIRO_READ_DATA is intended only as supplementary documentation and an example for understanding the structure of MIRO data. A more useful tool for processing MIRO data is an IDL package provided by PDS, named READPDS; for this, see: http://pdssbn.astro.umd.edu/nodehtml/software.shtml Here is an example of the use of READPDS to ingest a CTS file such as MIRO_3_CTS_20051792320.DAT in the Level-3 Deep-Impact archive. To start, the following command should be issued: IDL> data = readpds('MIRO_3_CTS_20051792320.LBL') which will read the entire file into an object named "data.table". The structure of this object can then be viewed with the command: IDL> help, /STRUCTURE, data.table which shows that it contains 19 columns, named ".column1" through ".column19", with properties as defined in the .FMT files in this archive. In particular, the spectroscopic data themselves are accessible in the 2-dimensional object data.table.column19[4250,17112]. These can then be processed or plotted using standard IDL commands. 8. Appendix 4: Directory Listing of Data Set MIRO_Thermalvac % ls -R RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0 RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0: AAREADME.TXT INDEX CATALOG LABEL DATA RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0.tar.gz DOCUMENT VOLDESC.CAT ERRATA.TXT RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/CATALOG: CATINFO.TXT INST.CAT MISSION.CAT REF.CAT TARGET.CAT DATASET.CAT INSTHOST.CAT PERSONNEL.CAT SOFTWARE.CAT RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/DATA: CONTINUUM ENGINEERING SPECTROSCOPIC RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/DATA/CONTINUUM: MIRO_MM_20011410000.DAT MIRO_MM_20011690000.DAT MIRO_SUBMM_20011550000.DAT MIRO_MM_20011410000.LBL MIRO_MM_20011690000.LBL MIRO_SUBMM_20011550000.LBL MIRO_MM_20011480000.DAT MIRO_MM_20011760000.DAT MIRO_SUBMM_20011620000.DAT MIRO_MM_20011480000.LBL MIRO_MM_20011760000.LBL MIRO_SUBMM_20011620000.LBL MIRO_MM_20011550000.DAT MIRO_SUBMM_20011410000.DAT MIRO_SUBMM_20011690000.DAT MIRO_MM_20011550000.LBL MIRO_SUBMM_20011410000.LBL MIRO_SUBMM_20011690000.LBL MIRO_MM_20011620000.DAT MIRO_SUBMM_20011480000.DAT MIRO_SUBMM_20011760000.DAT MIRO_MM_20011620000.LBL MIRO_SUBMM_20011480000.LBL MIRO_SUBMM_20011760000.LBL RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/DATA/ENGINEERING: MIRO_HSK_20011410000.DAT MIRO_HSK_20011480000.LBL MIRO_HSK_20011620000.DAT MIRO_HSK_20011690000.LBL MIRO_HSK_20011410000.LBL MIRO_HSK_20011550000.DAT MIRO_HSK_20011620000.LBL MIRO_HSK_20011760000.DAT MIRO_HSK_20011480000.DAT MIRO_HSK_20011550000.LBL MIRO_HSK_20011690000.DAT MIRO_HSK_20011760000.LBL RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/DATA/SPECTROSCOPIC: MIRO_CTS_20011410000.DAT MIRO_CTS_20011480000.LBL MIRO_CTS_20011620000.DAT MIRO_CTS_20011690000.LBL MIRO_CTS_20011410000.LBL MIRO_CTS_20011550000.DAT MIRO_CTS_20011620000.LBL MIRO_CTS_20011760000.DAT MIRO_CTS_20011480000.DAT MIRO_CTS_20011550000.LBL MIRO_CTS_20011690000.DAT MIRO_CTS_20011760000.LBL RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/DOCUMENT: CALIBRATION_PROC.LBL MIRO_LOGBOOK_18.XLS MIRO_TVDATA_07.LBL THERMAL_VAC_PROC.LBL CALIBRATION_PROC.PDF MIRO_LOGBOOK_19.LBL MIRO_TVDATA_07.ASC THERMAL_VAC_PROC.PDF CALIBRATION_PROC.ASC MIRO_LOGBOOK_19.ASC MIRO_TVDATA_07.XLS THERMAL_VAC_PROC.ASC DOCINFO.TXT MIRO_LOGBOOK_19.XLS RO-MIR-IF-0001_15.LBL USER_MANUAL.LBL MIRO_LOGBOOK_17.LBL MIRO_READ_DATA.LBL RO-MIR-IF-0001_15.PDF USER_MANUAL.PDF MIRO_LOGBOOK_17.ASC MIRO_READ_DATA.ASC RO-MIR-IF-0001_15.ASC USER_MANUAL.ASC MIRO_LOGBOOK_17.XLS MIRO_TVDATA_06.LBL THERMAL_VAC_PLAN.LBL UTCCON.LBL MIRO_LOGBOOK_18.LBL MIRO_TVDATA_06.ASC THERMAL_VAC_PLAN.PDF UTCCON.ASC MIRO_LOGBOOK_18.ASC MIRO_TVDATA_06.XLS THERMAL_VAC_PLAN.ASC RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/INDEX: INDEX.LBL INDEX.TAB INDXINFO.TXT RO-CAL-MIRO-2-GRND-THERMALVAC-V1.0/LABEL: CONT_LEVEL_2_FORMAT.FMT CTS_LEVEL_2_FORMAT.FMT ENG_LEVEL_2_FORMAT.FMT LABINFO.TXT 8 - 65 - ROSETTA To Planetary Science Archive Interface Control Document Document No. Issue/Rev. No. Date Page : RO-MIR-IF-0001 : 1.8 : 2009-05-15 : 65