Data Set Information
|
DATA_SET_NAME |
VG2 SAT LECP CALIBRATED RESAMPLED SCAN
AVERAGED 15MIN V1.0
|
DATA_SET_ID |
VG2-S-LECP-4-SUMM-AVERAGE-15MIN-V1.0
|
NSSDC_DATA_SET_ID |
|
DATA_SET_TERSE_DESCRIPTION |
Voyager 2 Energetic Particle (LECP) data from the Saturn encounter.
The data set provides 15 minute scan averaged counting rates.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
Data Set Description
--------------------
This browse data consists of resampled data from the Low
Energy Charged Particle (LECP) experiment on Voyager 2 while
the spacecraft was in the vicinity of Saturn. This instrument
measures the intensities of in-situ charged particles (>26 keV
electrons and >30 keV ions) with various levels of
discrimination based on energy, mass species, and angular
arrival direction. A subset of almost 100 LECP channels are
included with this data set. The LECP data are globally
calibrated to the extent possible (see below) and they are
time averaged to about 15 minute time intervals with the exact
beginning and ending times for those intervals matching the
LECP instrumental cycle periods (the angular scanning
periods). The LECP instrument has a rotating head for
obtaining angular anisotropy measurements of the medium energy
charged particles that it measures. The cycle time for the
rotation is variable, but during encounters it is always
faster than 15 minutes. For this browse data set only scan
average data is given (no angular information). The data is in
the form of 'rate' data which has not been converted to the
usual physical units. The reason is that such a conversion
would depend on uncertain determinations such as the mass
species of the particles and the level of background. Both
mass species and background are generally determined from
context during the study of particular regions. To convert
'rate' to 'intensity' for a particular channel one performs
the following tasks: 1) decide on the level of background
contamination and subtract that off the given rate level.
Background is to be determined from context and from making
use of sector 8 rates (sector 8 has a 2 mm Al shield covering
it). 2) Divide the background corrected rate by the channel
geometric factor and by the energy bandpass of the channel.
The geometric factor is found in entry
'channel_geometric_factor' as associated with each channel
'channel_id'. To determine the energy bandpass, one must judge
the mass species of the of the detected particles (for ions
but not for electrons). The energy band passes are given in
entries 'minimum_instrument_parameter' and
'maximum_instrument_parameter' in table 'FPLECPENERGY', and
are given in the form 'energy/nucleon'. For channels that
begin their names with the designations 'ch' these bandpasses
can be used on mass species that are accepted into that
channel (see entries 'MINIMUM_INSTRUMENT_PARAMETER' and
'MAXIMUM_INSTRUMENT_PARAMETER' in table 'FPLECPCHANZ', which
give the minimum and maximum 'Z' value accepted -- these
entries are blank for electron channels). For other channels
the given bandpass refers only to the lowest 'Z' value
accepted. The bandpasses for other 'Z' values are not all
known, but some are given in the literature (e.g.
[KRIMIGISETAL1979A]). The final product of these instructions
will be the particle intensity with the units:
counts/(cm^2 str sec keV).
Processing Level Id : 4
Software Flag : Y
Processing Start Time : 1988-08-01
Parameters
==========
Electron Rate
-------------
Sampling Parameter Name : TIME
Data Set Parameter Name : ELECTRON RATE
Sampling Parameter Resolution : 15.000000
Sampling Parameter Interval : 15.000000
Data Set Parameter Unit : COUNTS/SECOND
Noise Level : 0.000000
Sampling Parameter Unit : MINUTE
A measured parameter equaling the number of electrons hitting
a particle detector per specified accumulation interval. The
counted electrons may or may not be discriminated as to their
energies (e.g. greater than E1, or between E1 and E2).
Ion Rate
--------
Sampling Parameter Name : TIME
Data Set Parameter Name : ION RATE
Sampling Parameter Resolution : 15.000000
Sampling Parameter Interval : 15.000000
Data Set Parameter Unit : COUNTS/SECOND
Noise Level : 0.000000
Sampling Parameter Unit : MINUTE
A measured parameter equaling the number of ions striking a
particle detector per specified accumulation interval. The
counted ions may or may not be discriminated as to their
energies (e.g. energy/nucleon or energy/charge between E1 and
E2 or greater than E1) and/or as to their ion composition
(atomic number Z or mass number greater than Z1 or M1, or
between Z1 and z2 or M1 and M2).
Source Instrument Parameters
============================
Instrument Host ID : VG2
Data Set Parameter Name : ION RATE
Instrument Parameter Name : ION RATE
Important Instrument Parameters : 1
Instrument Host ID : VG2
Data Set Parameter Name : ELECTRON RATE
Instrument Parameter Name : ELECTRON RATE
Important Instrument Parameters : 1
Processing
==========
Processing History
------------------
Source Data Set ID : VG2-S-LECP-2-
Software : PFAT:VGER
Product Data Set ID : VG2-S-LECP-4-BR-15MIN
Software 'PFAT:VGER'
--------------------
Software Name : PFAT:VGER
Software Type : PIN
Software Release Date : N/A
Node ID : N/A
Cognizant Engineer : N/A
Software Access Description : N/A
Data Coverage
=============
Filename Records Start Stop
----------------------------------------------------------------------
Volume ID: VG_1601
AVERAGE.TAB 668 1981-08-24T00:07:29.560 1981-08-30T23:52:30.430
Missing Data Flag
=================
Any data column whose value is -9.9e+10 is a missing data
value.
|
DATA_SET_RELEASE_DATE |
2002-08-21T00:00:00.000Z
|
START_TIME |
1981-08-24T12:07:29.560Z
|
STOP_TIME |
1981-08-30T11:52:30.430Z
|
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 |
VG2
|
INSTRUMENT_NAME |
LOW ENERGY CHARGED PARTICLE
|
INSTRUMENT_ID |
LECP
|
INSTRUMENT_TYPE |
CHARGED PARTICLE ANALYZER
|
NODE_NAME |
Planetary Plasma Interactions
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview
=========================
At all times during this planetary encounter there exist data
in this data set that can be rated with the highest confidence
level. However, some of the channels of data are contaminated
by various kinds and various levels of contaminations. It is
therefore imperative, in using this data set, that the
contamination tables within the catalog be examined. Also, not
all kinds of contamination have been fully documented. When in
doubt the data supplier must be contacted.
Some channels are subject to serious contaminations, and many
of these contaminations cannot be removed except with a region-
by-region analysis, which has not been done for this data.
Thus, to use this data it is absolutely vital that the
contamination types ('CONTAMINATION_ID' , 'CONTAMINATION_DESC')
and the levels of contamination ('DATA_QUALITY_ID'
corresponding to the definitions 'DATA_QUALITY_DESC') be
carefully examined for all regions of study. A dead time
correction procedure has been applied in an attempt to correct
the linear effects of detector overdrive (pulse-pileup). This
procedure does not fix severely overdriven detectors. A
procedure is available for correcting Voyager 2 LECP electron
contamination of low energy ion channels, but its
effectiveness has been evaluated only for the Uranus data set.
Thus, corrections have been applied only to the Uranus data
set.
|
CITATION_DESCRIPTION |
Krimigis, S. M., Mauk, B. H., Armstrong, T. P.,
VG2-S-LECP-4-SUMM-AVERAGE-15MIN-V1.0, VG2 SAT LECP
CALIBRATED RESAMPLED SCAN AVERAGED 15MIN V1.0,
NASA Planetary Data System, 2002.
|
ABSTRACT_TEXT |
This browse data consists of resampled data from the Low
Energy Charged Particle (LECP) experiment on Voyager 2 while
the spacecraft was in the vicinity of Saturn. This instrument
measures the intensities of in-situ charged particles (>26 keV
electrons and >30 keV ions) with various levels of
discrimination based on energy, mass species, and angular
arrival direction. A subset of almost 100 LECP channels are
included with this data set. The LECP data are globally
calibrated to the extent possible (see below) and they are
time averaged to about 15 minute time intervals with the exact
beginning and ending times for those intervals matching the
LECP instrumental cycle periods (the angular scanning
periods). The LECP instrument has a rotating head for
obtaining angular anisotropy measurements of the medium energy
charged particles that it measures. The cycle time for the
rotation is variable, but during encounters it is always
faster than 15 minutes. For this browse data set only scan
average data is given (no angular information). The data is in
the form of 'rate' data which has not been converted to the
usual physical units.
|
PRODUCER_FULL_NAME |
BARRY H. MAUK
|
SEARCH/ACCESS DATA |
Planetary Plasma Interactions Website
|
|