Data Set Information
|
DATA_SET_NAME |
VOYAGER 2 SAT LOW ENERGY CHARGED PARTICLE CALIB. BR 15MIN
|
DATA_SET_ID |
VG2-S-LECP-4-BR-15MIN
|
NSSDC_DATA_SET_ID |
77-076A-07D
|
DATA_SET_TERSE_DESCRIPTION |
VOYAGER 2 SAT LOW ENERGY CHARGED PARTICLE CALIB. BR 15MIN
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
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 INSTUMENT HAS A ROTATING HEAD FOR OBTAINING ANGULAR
ANISOTROPY MEASUREMENTS OF THE MEDIUM ENERGY CHARGED PARTICLES
THAT IT MEASURES. THE CYCLE TIME FOR THE ROTATION IF 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. KRIMIGIS ET AL., 1979). THE FINAL
PRODUCT OF THESE INSTRUCTIONS WILL BE THE PARTICLE INTENSITY
WITH THE UNITS: COUNTS/(CM**2.STR.SEC.KEV). 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.
Processing Level Id : 4
Software Flag : Y
Processing Start Time : 1982-10-13
Parameters
==========
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
Description
-----------
A measured parameter equaling the number of electrons A
measured parameter equaling the number of ions striking a
hitting a particle detector per specified accumulation
particle detector per specified accumulation interval. The
interval. The counted electrons may or may not be counted
ions may or may not be discriminated as to their energies
(e.g. energy/nucleon or energy/charge between E1
discriminated as to their energies (e.g. greater than E1, or
between E1 and E2). 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_SET_RELEASE_DATE |
1988-09-01T00:00:00.000Z
|
START_TIME |
1981-08-24T12:00:00.000Z
|
STOP_TIME |
1981-09-01T12:00:00.000Z
|
MISSION_NAME |
COMET SL9/JUPITER COLLISION
VOYAGER
|
MISSION_START_DATE |
1993-01-01T12:00:00.000Z
1972-07-01T12:00:00.000Z
|
MISSION_STOP_DATE |
1996-01-01T12:00:00.000Z
N/A (ongoing)
|
TARGET_NAME |
SATURN
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
VG2
|
INSTRUMENT_NAME |
LOW ENERGY CHARGED PARTICLE
|
INSTRUMENT_ID |
LECP
|
INSTRUMENT_TYPE |
ENERGETIC PARTICLE DETECTOR
|
NODE_NAME |
Planetary Plasma Interactions
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
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.
|
CITATION_DESCRIPTION |
Citation TBD
|
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 INSTUMENT HAS A
ROTATING HEAD FOR OBTAINING ANGULAR ANISOTROPY MEASUREMENTS OF
THE MEDIUM ENERGY CHARGED PARTICLES THAT IT MEASURES. THE CYCLE
TIME FOR THE ROTATION IF 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. KRIMIGIS ET AL., 1979). THE FINAL
PRODUCT OF THESE INSTRUCTIONS WILL BE THE PARTICLE INTENSITY WITH
THE UNITS: COUNTS/(CM**2.STR.SEC.KEV). 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.
|
PRODUCER_FULL_NAME |
BARRY H. MAUK
|
SEARCH/ACCESS DATA |
Planetary Plasma Interactions Website
|
|