HDPWS

Voyager 1 Planetary Radio Astronomy (PRA) Lowband Receiver Jupiter encounter, 6 sec resolution

ResourceID
spase://NASA/NumericalData/Voyager1/PRA/Jupiter/Low/PT6S

Description
(Description based on material from VG1_PRA_JUP_HRES_DS.CAT) Voyager 1 Radio Astronomy (PRA) data from the Jupiter encounter (1979-01-06 to 1979-04-13). The data set provides 6 second high resolution lowband radio mean power data. The data are provided for 70 instrument channels, covering 1.2 to 1326.0 kHz. This data set (VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0) contains data acquired by the Voyager-1 Planetary Radio Astronomy (PRA) instrument during the Jupiter encounter. The bounding time interval set for most Voyager 1 Jupiter PDS data sets is the Voyager project defined 'far encounter' mission phase boundary (1979-02-28 to 1979-03-22). Since, however, the PRA instrument is able to observe planetary phenomenon at much larger ranges than other fields and particles experiments, this boundary is artificial with respect to PRA. Hence, PRA lowband data provided here cover the entire Jupiter Encounter Phase (1979-01-06 to 1979-04-13). Data from beyond the far encounter interval is contained in the cruise data archive which is available from the NSSDC. VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0 contains data at the highest time resolution possible during normal operations. The normal mode of PRA operations during the planetary encounters was to sweep through the two radio receiver bands, high band (40.5 to 1.5 MHz in 128 channels spaced 0.3072 MHz apart) and low band (1326.0 to 1.2 kHz in 70 channels spaced 19.2 kHz apart) in a period of 6 seconds. The receivers measured, on alternate samples, the left hand circular and right hand circular (radio definition) power. Measured Parameters =================== The data here are from the low frequency receiver band and are 'packaged' into spacecraft major frame records. Each major frame is 48 seconds long or eight sweeps through the PRA receiver. The data are calibrated and are given in units of 'millibels' which is 1000 times the log of the received power. Zero millbels corresponds to approximately 1.4 x 10^-21 W m^-2 Hz^-1, however, this value is never seen in practice. The minimum values detected, which includes receiver internal and spacecraft generated noise, are about 2300 to 2400 millibels, or about 3.5 x 10^-19 W m^-2 Hz^-1; even higher values are seen at the very lowest frequencies. The data format is ASCII and consists of a time indicator followed by an array containing the eight low band sweeps. Time is spacecraft event time (SCET) which is basically universal time at the spacecraft. Specifically, time is in the form of YYMMDD and seconds into YYMMDD. Both are written as I6. Example: July 1, 1979 at 12 hours SCET would be 790701, 43200. The seconds correspond, to the nearest second, to the start of the sweep (which occurs in PRA high band). The first value in low band (1326.0 kHz) occurs some 3.9 seconds after this time and samples at successively lower frequencies are spaced 0.03 seconds apart. Only one time is given for the entire major frame, thus the start of each sweep is the time given plus 6 times the sweep number minus 1 (i.e., 0 through 7). The data array is dimensioned as 71 X 8 and written as I4 format (i.e. 568I4). The '8' corresponds to the eight PRA sweeps. The lowest 68 of the 70 low band channels (1287.6 to 1.2 kHz) are in positions 2-69. Positions 70-71 should be ignored. Missing or bad data values are set to zero. In position 1 of each sweep is a status word where the 12 least significant bits have used, although not all 12 have meaning for PRA low band. Numbering those bits 0 for least significant to 11 for most significant, the bits that have meaning are as follows: bit 0: 15 dB attenuator in use when equal to 1 1: 30 dB attenuator in use when equal to 1 2: 45 dB attenuator in use when equal to 1 9,10 (together): polarization of first channel sampled (1326.0 kHz) according to the scheme: +---------------------------+ value bit 10= 0 1 value bit 9= 0 R L 1 L R +---------------------------+ Polarization at successively lower frequencies is opposite to the frequency above it, i.e. either a LRLR or an RLRL pattern. Successive 6-second sweeps start on the opposite polarization as the previous sweep as indicated in the status bits. Note that this polarization is the received polarization, not necessarily the emitted polarization. Correct interpretation of the received polarization depends on the antenna plane orientation relative to the radio source. A good description of this concept can be found in Leblanc Y., Aubier M. G., Ortega-Molina A., Lecacheux A., 1987, J.Geophys. Res. 92, 15125 and in Wang, L. and Carr, T.D., Recalibration of the Voyager PRA antenna for polarization sense measurement, Astron. Astrophys., 281, 945-954, 1994. and references therein. Missing or bad data values are set to zero. If the status word is zero, any data in that receiver sweep should be discarded. Data Coverage ============= The data are stored as 4 ASCII tables (.TAB), each accompanied with a PDS label file (.LBL) which describes properties of the data file. Data cover the following time intervals: Volume ID: VGPR_1201 +------------------------------------------------------------------------+ Filename Records Start Stop ------------------------------------------------------------------------ PRA_I.TAB 35569 1979-01-06T00:00:34.000Z 1979-01-30T23:59:47.000Z PRA_II.TAB 39493 1979-01-31T00:00:35.000Z 1979-02-25T23:59:47.000Z PRA_III.TAB 41371 1979-02-26T00:00:35.000Z 1979-03-22T23:59:56.000Z PRA_IV.TAB 24587 1979-03-23T00:00:44.000Z 1979-04-13T23:59:08.000Z +------------------------------------------------------------------------+ Confidence Level Overview ========================= The accuracy of calibration in the PRA low band is approximately 2 dB, except at frequencies below 100 kHz where it is somewhat worse. Interference from the Voyager power subsystem is a major problem to the PRA instrument, affecting many of the 70 low band channels. This interference manifests itself by abrupt changes in background levels. Some channels, notably 136 and 193 kHz, are almost always affected, whereas, others are only affected for short intervals. Usually, this interference is only a problem when the natural signals are weak. Additional information associated with this data set is available in the following files: +-----------------------------------------------------------------------------------------------------------------------------------+ file contents http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/VG1_PRA1_INST.CAT VG1 PRA instrument description http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/VG1_PRA_JUP_HRES_DS.CAT data set description http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/PERSON.CAT personnel information http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/REF.CAT key reference description http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/DOCUMENT/INSTRUMENT ASCII and HTML versions of the PRA investigation description paper +-----------------------------------------------------------------------------------------------------------------------------------+

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NumericalData

ResourceID
spase://NASA/NumericalData/Voyager1/PRA/Jupiter/Low/PT6S
ResourceHeader
ResourceName
Voyager 1 Planetary Radio Astronomy (PRA) Lowband Receiver Jupiter encounter, 6 sec resolution
AlternateName
VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0
ReleaseDate
2020-07-07 21:15:54Z
Description
(Description based on material from VG1_PRA_JUP_HRES_DS.CAT) Voyager 1 Radio Astronomy (PRA) data from the Jupiter encounter (1979-01-06 to 1979-04-13). The data set provides 6 second high resolution lowband radio mean power data. The data are provided for 70 instrument channels, covering 1.2 to 1326.0 kHz. This data set (VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0) contains data acquired by the Voyager-1 Planetary Radio Astronomy (PRA) instrument during the Jupiter encounter. The bounding time interval set for most Voyager 1 Jupiter PDS data sets is the Voyager project defined 'far encounter' mission phase boundary (1979-02-28 to 1979-03-22). Since, however, the PRA instrument is able to observe planetary phenomenon at much larger ranges than other fields and particles experiments, this boundary is artificial with respect to PRA. Hence, PRA lowband data provided here cover the entire Jupiter Encounter Phase (1979-01-06 to 1979-04-13). Data from beyond the far encounter interval is contained in the cruise data archive which is available from the NSSDC. VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0 contains data at the highest time resolution possible during normal operations. The normal mode of PRA operations during the planetary encounters was to sweep through the two radio receiver bands, high band (40.5 to 1.5 MHz in 128 channels spaced 0.3072 MHz apart) and low band (1326.0 to 1.2 kHz in 70 channels spaced 19.2 kHz apart) in a period of 6 seconds. The receivers measured, on alternate samples, the left hand circular and right hand circular (radio definition) power. Measured Parameters =================== The data here are from the low frequency receiver band and are 'packaged' into spacecraft major frame records. Each major frame is 48 seconds long or eight sweeps through the PRA receiver. The data are calibrated and are given in units of 'millibels' which is 1000 times the log of the received power. Zero millbels corresponds to approximately 1.4 x 10^-21 W m^-2 Hz^-1, however, this value is never seen in practice. The minimum values detected, which includes receiver internal and spacecraft generated noise, are about 2300 to 2400 millibels, or about 3.5 x 10^-19 W m^-2 Hz^-1; even higher values are seen at the very lowest frequencies. The data format is ASCII and consists of a time indicator followed by an array containing the eight low band sweeps. Time is spacecraft event time (SCET) which is basically universal time at the spacecraft. Specifically, time is in the form of YYMMDD and seconds into YYMMDD. Both are written as I6. Example: July 1, 1979 at 12 hours SCET would be 790701, 43200. The seconds correspond, to the nearest second, to the start of the sweep (which occurs in PRA high band). The first value in low band (1326.0 kHz) occurs some 3.9 seconds after this time and samples at successively lower frequencies are spaced 0.03 seconds apart. Only one time is given for the entire major frame, thus the start of each sweep is the time given plus 6 times the sweep number minus 1 (i.e., 0 through 7). The data array is dimensioned as 71 X 8 and written as I4 format (i.e. 568I4). The '8' corresponds to the eight PRA sweeps. The lowest 68 of the 70 low band channels (1287.6 to 1.2 kHz) are in positions 2-69. Positions 70-71 should be ignored. Missing or bad data values are set to zero. In position 1 of each sweep is a status word where the 12 least significant bits have used, although not all 12 have meaning for PRA low band. Numbering those bits 0 for least significant to 11 for most significant, the bits that have meaning are as follows: bit 0: 15 dB attenuator in use when equal to 1 1: 30 dB attenuator in use when equal to 1 2: 45 dB attenuator in use when equal to 1 9,10 (together): polarization of first channel sampled (1326.0 kHz) according to the scheme: +---------------------------+ value bit 10= 0 1 value bit 9= 0 R L 1 L R +---------------------------+ Polarization at successively lower frequencies is opposite to the frequency above it, i.e. either a LRLR or an RLRL pattern. Successive 6-second sweeps start on the opposite polarization as the previous sweep as indicated in the status bits. Note that this polarization is the received polarization, not necessarily the emitted polarization. Correct interpretation of the received polarization depends on the antenna plane orientation relative to the radio source. A good description of this concept can be found in Leblanc Y., Aubier M. G., Ortega-Molina A., Lecacheux A., 1987, J.Geophys. Res. 92, 15125 and in Wang, L. and Carr, T.D., Recalibration of the Voyager PRA antenna for polarization sense measurement, Astron. Astrophys., 281, 945-954, 1994. and references therein. Missing or bad data values are set to zero. If the status word is zero, any data in that receiver sweep should be discarded. Data Coverage ============= The data are stored as 4 ASCII tables (.TAB), each accompanied with a PDS label file (.LBL) which describes properties of the data file. Data cover the following time intervals: Volume ID: VGPR_1201 +------------------------------------------------------------------------+ Filename Records Start Stop ------------------------------------------------------------------------ PRA_I.TAB 35569 1979-01-06T00:00:34.000Z 1979-01-30T23:59:47.000Z PRA_II.TAB 39493 1979-01-31T00:00:35.000Z 1979-02-25T23:59:47.000Z PRA_III.TAB 41371 1979-02-26T00:00:35.000Z 1979-03-22T23:59:56.000Z PRA_IV.TAB 24587 1979-03-23T00:00:44.000Z 1979-04-13T23:59:08.000Z +------------------------------------------------------------------------+ Confidence Level Overview ========================= The accuracy of calibration in the PRA low band is approximately 2 dB, except at frequencies below 100 kHz where it is somewhat worse. Interference from the Voyager power subsystem is a major problem to the PRA instrument, affecting many of the 70 low band channels. This interference manifests itself by abrupt changes in background levels. Some channels, notably 136 and 193 kHz, are almost always affected, whereas, others are only affected for short intervals. Usually, this interference is only a problem when the natural signals are weak. Additional information associated with this data set is available in the following files: +-----------------------------------------------------------------------------------------------------------------------------------+ file contents http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/VG1_PRA1_INST.CAT VG1 PRA instrument description http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/VG1_PRA_JUP_HRES_DS.CAT data set description http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/PERSON.CAT personnel information http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/CATALOG/REF.CAT key reference description http://ppi.pds.nasa.gov/ditdos/download?id=pds://PPI/VGPR_1201/DOCUMENT/INSTRUMENT ASCII and HTML versions of the PRA investigation description paper +-----------------------------------------------------------------------------------------------------------------------------------+
Acknowledgement
When using delivered data please acknowledge the data provider and PDS in accordance with the PDS citation policy. Full details can be found at: http://ppi.pds.nasa.gov/citations_policy.jsp
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://SMWG/Person/James.W.Warwick
2. MetadataContact spase://SMWG/Person/Todd.A.King

InformationURL
Name
PPI/PDS PRA Instrument catalog file PRAINST.CAT
URL
Description
Information about the PRA instrument on the Voyager mission including operational mode descriptions.
InformationURL
Name
VG1_PRA_JUP_HRES_DS.CAT
URL
Description
VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0 dataset description file
PriorIDs
spase://VWO/NumericalData/Voyager1/PRA/VG1_PRA_Low_Jupiter_PT6S
spase://VWO/NumericalData/Voyager1/PRA/Jupiter/Low.PT6S
spase://VSPO/NumericalData/Voyager1/PRA/Jupiter/Low/PT6S
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
Access to dataset ID VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0
URL
Description
Below this directory level are the 4 ASCII files (TAB) and the accompanying PDS label (LBL) files.
Language
en
Format
Text.ASCII
Encoding
None
Acknowledgement
When using delivered data please acknowledge the data provider and PDS in accordance with the PDS citation policy. Full details can be found at: http://ppi.pds.nasa.gov/citations_policy.jsp
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
PDS/PPI
URL
ProductKey
VG1-J-PRA-3-RDR-LOWBAND-6SEC-V1.0
Description
This collection is archived with NASA's Planetary Data System.
Language
En
Format
Text.ASCII
Acknowledgement
NASA's Planetary Plasma Interactions (PPI) Node of the Planetary Data System (PDS) and the P.I. for the data.
InstrumentIDs
MeasurementType
Waves.Passive
MeasurementType
Spectrum
MeasurementType
ElectricField
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
1979-01-06 00:00:34Z
StopDate
1979-04-13 23:59:08Z
Cadence
PT6S
SpectralRange
RadioFrequency
ObservedRegion
Jupiter
ObservedRegion
Heliosphere.Outer
Keywords
Dynamic Spectrogram
Spectrogram
Jupiter
Kilometric Radio Emission
KOM
Parameter #1
Name
Date
Description
Year, month, and day of start of first sweep in (SCET) in the format YYMMDD (Format=I6)
Support
SupportQuantity
Temporal
Parameter #2
Name
Second
Description
Seconds of day (SCET) of start of first sweep (Format=I6)
Units
s
Support
SupportQuantity
Temporal
Parameter #3
Name
Spectral Power
Description
Electric field power spectral density, 8 sweeps of the PRA lowband receiver of 70 frequency channels each.
Units
millibels
Wave
WaveType
PlasmaWaves
WaveQuantity
ACElectricField
FrequencyRange
SpectralRange
RadioFrequency
Low
1.2
High
1326
Units
kHz
Parameter #4
Name
Status Word
Description
indicates attenuators used to record the data and the polarization
Support
SupportQuantity
Other