Data Set Information
|
DATA_SET_NAME |
VG1 SAT PWS RESAMPLED SPECTRAL ANALYZER
48SEC V1.0
|
DATA_SET_ID |
VG1-S-PWS-4-SUMM-SA-48SEC-V1.0
|
NSSDC_DATA_SET_ID |
|
DATA_SET_TERSE_DESCRIPTION |
Voyager 1 Plasma Wave (PWS) spectrum analyzer data from the Saturn
encounter. The data set provides 48 second averages of the wave electric
field intensities.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
Instrument P.I. : Donald A. Gurnett
Data Supplier : William S. Kurth
Data sampling rate : 48 seconds
Data Set Start Time : 1981-08-24T00:00:00.000Z
Data Set Stop Time : 1981-08-31T23:59:12.000Z
Data Set Description
--------------------
This data set consists of 48-second calibrated, averaged wave
electric field intensities from the Voyager 1 Plasma Wave
Receiver spectrum analyzer obtained in the vicinity of the
Jovian magnetosphere. For each 48-second interval, a geometric
average field strength is determined for each of the 16
spectrum analyzer channels whose center frequencies range from
10 Hertz to 56.2 kiloHertz and which are logarithmically
spaced in frequency, four channels per decade. The time
associated with each set of averages is the beginning of the
averaging interval. Averages are stored in units of
volt/meter. During data gaps where complete 48-second
intervals are missing, no entries exist in the file, that is,
the gaps are not zero-filled or tagged in any other way.
Additional information about this data set and the instrument
which produced it can be found elsewhere in this catalog. An
overview of the data in this data set can be found in
[GURNETTETAL1979] and a complete instrument description can be
found in [SCARF&GURNETT1977].
Processing Level Id : 4
Software Flag : Y
Processing Start Time : 1988-02-01
Parameters
==========
Sampling Parameter Name : TIME
Data Set Parameter Name : PLASMA WAVE SPECTRUM
Sampling Parameter Resolution : 48.000000
Minimum Sampling Parameter : 197708201553.000000
Sampling Parameter Interval : 48.000000
Minimum Available Sampling Int : 4.000000
Data Set Parameter Unit : VOLT/METER
Noise Level : 0.000005
Sampling Parameter Unit : SECOND
A set of derived parameters consisting of wave electric field
intensities or electric field spectral densities at various
contiguous frequencies over a range of frequencies. The MKS
units are: Volts/Meter or Volts**2/(Hertz Meter**2),
respectively.
Source Instrument Parameters
============================
Instrument Host ID : VG1
Data Set Parameter Name : PLASMA WAVE SPECTRUM
Instrument Parameter Names : ELECTRIC FIELD WAVEFORM
ELECTRIC FIELD COMPONENT
MAGNETIC FIELD COMPONENT
WAVE ELECTRIC FIELD INTENSITY
WAVE MAGNETIC FIELD INTENSITY
Important Instrument Parameters : 1 (for all parameters)
|
DATA_SET_RELEASE_DATE |
2002-10-02T00:00:00.000Z
|
START_TIME |
1980-11-11T12:00:00.000Z
|
STOP_TIME |
1980-11-17T11:59:12.000Z
|
MISSION_NAME |
VOYAGER
|
MISSION_START_DATE |
1972-07-01T12:00:00.000Z
|
MISSION_STOP_DATE |
N/A (ongoing)
|
TARGET_NAME |
SATURN
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
VG1
|
INSTRUMENT_NAME |
PLASMA WAVE RECEIVER
|
INSTRUMENT_ID |
PWS
|
INSTRUMENT_TYPE |
PLASMA WAVE SPECTROMETER
|
NODE_NAME |
Planetary Plasma Interactions
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview
=========================
This data set includes all available spectrum analyzer data
within the interval of time covered. The data set has been
cleaned as well as possible for periodic noise spikes due to a
stepper motor operating on the LECP and a modulated grid
within the PLS. The averages do not include these noise
spikes. Other possible sources of noise which have not been
eliminated include a nearly continuous tone at about 311 Hz
after closest approach due to interference from the gyros and
random intense spikes of noise below 1 kiloHertz due to the
operation of attitude control thrusters. The data between 0040
and 0155 spacecraft event time on July 10 1979 is heavily
contaminated by thruster activity associated with a trajectory
correction maneuver. Other randomly occurring spikes or time
periods of intense spikes over the entire frequency range are
indicative of telemetry errors. No attempt has been made to
remove spikes since some could be valid data, i.e. real bursts
of wave activity. The 17.8-Hz channel is sometimes
contaminated by interference from the PRA instrument,
depending on that instrument's mode. This interference is at a
relatively constant level.
Data Coverage
=============
Filename Records Start Stop
-----------------------------------------------------------------------
Volume ID: VG_1601
SA_48S.TAB 14235 1981-08-24T00:00:00.000Z 1981-08-31T23:59:12.000Z
Missing Data Flag
=================
Any columns containing the value -9.99e+10 (depending upon column
format) is a missing data value.
|
CITATION_DESCRIPTION |
Kurth, W.S., VG1-S-PWS-4-SUMM-SA-48SEC-V1.0,
VG1 SAT PWS RESAMPLED SPECTRAL ANALYZER 48SEC V1.0,
NASA Planetary Data System, 2002.
|
ABSTRACT_TEXT |
This data set consists of 48-second
calibrated, averaged wave electric field intensities from the Voyager 1
Plasma Wave Receiver spectrum analyzer obtained in the vicinity of the
Jovian magnetosphere. For each 48-second interval, a geometric average
field strength is determined for each of the 16 spectrum analyzer channels
whose center frequencies range from 10 Hertz to 56.2 kiloHertz and which
are logarithmically spaced in frequency, four channels per decade. The
time associated with each set of averages is the beginning of the
averaging interval. Averages are stored in units of volt/meter. During
data gaps where complete 48-second intervals are missing, no entries exist
in the file, that is, the gaps are not zero-filled or tagged in any other
way. Additional information about this data set and the instrument which
produced it can be found elsewhere in this catalog.
|
PRODUCER_FULL_NAME |
WILLIAM S. KURTH
|
SEARCH/ACCESS DATA |
Planetary Plasma Interactions Website
|