Data Set Information
|
DATA_SET_NAME |
VOYAGER 1 SATURN PLASMA DERIVED ION MOMENTS 96 SEC
|
DATA_SET_ID |
VG1-S-PLS-5-ION-MOM-96.0SEC
|
NSSDC_DATA_SET_ID |
77-084A-06H
|
DATA_SET_TERSE_DESCRIPTION |
VOYAGER 1 SATURN PLASMA DERIVED ION MOMENTS 96 SEC
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
THIS DATA SET CONTAINS ESTIMATES OF THE ION MOMENT DENSITY IN
THE PLS VOLTAGE RANGE (10-5950 EV/Q) AT SATURN DURING THE
VOYAGER 1 ENCOUNTER. RIGID COROTATION IS ASSUMED, WHICH LEADS
TO AN UNDERESTIMATE OF THE DENSITY IN SOME REGIONS, AS DOES THE
USE OF AN ACCEPTANCE AREA RELEVANT FOR A COLD BEAM FOR PLASMA
WHICH IS TRANSONIC IS SOME REGIONS. DENSITIES MAY BE
UNDERESTIMATED BY A FACTOR OF 2-3 IN THE INNER MAGNETOSPHERE,
SO THIS DATA SET SHOULD BE USED PRIMARILY FOR STUDIES USING
VARIATIONS IN PLASMA DENSITY. THE FIT DENSITIES GIVE A BETTER
ESTIMATE OF THE ABSOLUTE DENSITY. THIS IS THE DATA SHOWN AND
DESCRIBED IN DETAIL IN LAZARUS AND MCNUTT (1983). DATA FORMAT:
COLUMNS 1-5 ARE TIME (YEAR, DAY, HOUR, MIN, SEC) AND COLUMN 6
IS THE MOMENT DENSITY IN CM-3. EACH ROW HAS FORMAT
(I5,I4,2I3,I4,F8.3). VALUES OF 1.E32 INDICATE THAT THE
PARAMETER COULD NOT BE OBTAINED FROM THE DATA USING THE
STANDARD ANALYSIS TECHNIQUE. ADDITIONAL INFORMATION ABOUT THIS
DATASET 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 LAZARUS AND MCNUTT (1983) AND A
COMPLETE INSTRUMENT DESCRIPTION CAN BE FOUND IN BRIDGE (1977).
Processing Level Id : 5
Software Flag : Y
Parameters
==========
Sampling Parameter Name : TIME
Data Set Parameter Name : ION DENSITY
Sampling Parameter Resolution : 96.000000
Sampling Parameter Interval : 96.000000
Minimum Available Sampling Int : 96.000000
Data Set Parameter Unit : CM-3
Sampling Parameter Unit : SECOND
Description
-----------
A derived parameter equaling the number of ions per unit
volume over a specified range of ion energy, energy/charge,
or energy/nucleon. Discrimination with regard to mass and or
charge state is necessary to obtain this quantity, however,
mass and charge state are often assumed due to instrument
limitations.
Many different forms of ion density are derived. Some are
distinguished by their composition (N+, proton, ion, etc.) or
their method of derivation (Maxwellian fit, method of
moments). In some cases, more than one type of density will
be provided in a single dataset. In general, if more than
one ion species is analyzed, either by moment or fit, a total
density will be provided which is the sum of the ion
densities. If a plasma component does not have a Maxwellian
distribution the actual distribution can be represented as
the sum of several Maxwellians, in which case the density of
each Maxwellian is given.
Source Instrument Parameters
============================
Instrument Host ID : VG1
Data Set Parameter Name : ION DENSITY
Instrument Parameter Name : ION RATE
Important Instrument Parameters : 1
Instrument Host ID : VG1
Data Set Parameter Name : ION DENSITY
Instrument Parameter Name : ION CURRENT
Important Instrument Parameters : 1
Instrument Host ID : VG1
Data Set Parameter Name : ION DENSITY
Instrument Parameter Name : PARTICLE MULTIPLE PARAMETERS
Important Instrument Parameters : 1
Processing
==========
Processing History
------------------
Source Data Set ID : VG1-PLS
Software : MOMANAL
Product Data Set ID : VG1-S-PLS-5-ION-MOM-96.0SEC
Software 'MOMANAL'
------------------
Software Name : MOMANAL
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 |
1988-08-01T00:00:00.000Z
|
START_TIME |
1980-11-12T03:00:11.000Z
|
STOP_TIME |
1980-11-13T08:58:35.000Z
|
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 SCIENCE EXPERIMENT
|
INSTRUMENT_ID |
PLS
|
INSTRUMENT_TYPE |
PLASMA ANALYZER
|
NODE_NAME |
Planetary Plasma Interactions
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Overview
========
THIS DATA SET PROVIDES AN ESTIMATE OF THE POSITIVE ION CHARGE
DENSITY. SEVERAL ASSUMPTION/SIMPLIFICATIONS ARE MADE TO
SIMPLIFY THE ANALYSIS WHICH MAY AFFECT THE ACCURACY OF THE
RESULTS. HIGH MACH NUMBER FLOW IS ASSUMED; MACH NUMBERS OF 1,
WHICH ARE OBSERVED IN THE INNER MAGNETOSPHERE, CAN RESULT IN
50% UNDERESTIMATES OF THE CHARGE DENSITY. THE ANALYSIS ASSUMES
A UNIT RESPONSE (IE., ALL PARTICLES IN A COLD BEAM INCIDENT ON
THE APERTURE OF THE EXPERIMENT WOULD BE MEASURED AT THE
COLLECTOR). THE ACTUAL RESPONSE IS AS LOW AS 70%. A VELOCITY
INTO THE DETECTOR MUST ALSO BE ASSUMED; THE VELOCITY USED IS
THE COROTATION VELOCITY. OBSERVATIONS INDICATE THAT IN SOME
REGIONS THE ACTUAL VELOCITY IS AS LITTLE AS HALF OF THE
COROTATION VELOCITY, GIVING FACTOR OF 2 ERRORS IN THE DENSITY.
FINALLY, ONLY IONS IN THE PLS ENERGY RANGE (10-5950 EV/Q) ARE
COUNTED. THE CUMULATIVE ERROR FROM ALL THESE EFFECTS IS LESS
THAN 10% IN THE SOLAR WIND, LESS THAN A FACTOR OF 2 IN THE
OUTER MAGNETOSPHERE (R>10 RS), AND UP TO A FACTOR OF 3 INSIDE
THIS. SINCE THE AMPLITUDE OF EACH OF THESE EFFECTS VARIES
SLOWLY IN TIME (DISTANCE), THE RELATIVE CHANGES IN DENSITY ARE
GOOD TO 10 PERCENT IN MOST CASES. THIS DATA SET IS MOST USEFUL
FOR LOOKING AT DENSITY VARIATIONS; ION FIT DENSITIES ARE MUCH
BETTER INDICATORS OF THE ABSOLUTE PLASMA DENSITY
|
CITATION_DESCRIPTION |
Citation TBD
|
ABSTRACT_TEXT |
THIS DATA SET CONTAINS ESTIMATES OF THE ION MOMENT DENSITY IN THE
PLS VOLTAGE RANGE (10-5950 EV/Q) AT SATURN DURING THE VOYAGER 1
ENCOUNTER. RIGID COROTATION IS ASSUMED, WHICH LEADS TO AN
UNDERESTIMATE OF THE DENSITY IN SOME REGIONS, AS DOES THE USE OF
AN ACCEPTANCE AREA RELEVANT FOR A COLD BEAM FOR PLASMA WHICH IS
TRANSONIC IS SOME REGIONS. DENSITIES MAY BE UNDERESTIMATED BY A
FACTOR OF 2-3 IN THE INNER MAGNETOSPHERE, SO THIS DATA SET SHOULD
BE USED PRIMARILY FOR STUDIES USING VARIATIONS IN PLASMA DENSITY.
THE FIT DENSITIES GIVE A BETTER ESTIMATE OF THE ABSOLUTE DENSITY.
THIS IS THE DATA SHOWN AND DESCRIBED IN DETAIL IN LAZARUS AND
MCNUTT (1983). DATA FORMAT: COLUMNS 1-5 ARE TIME (YEAR, DAY,
HOUR, MIN, SEC) AND COLUMN 6 IS THE MOMENT DENSITY IN CM-3. EACH
ROW HAS FORMAT (I5,I4,2I3,I4,F8.3). VALUES OF 1.E32 INDICATE THAT
THE PARAMETER COULD NOT BE OBTAINED FROM THE DATA USING THE
STANDARD ANALYSIS TECHNIQUE. ADDITIONAL INFORMATION ABOUT THIS
DATASET 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 LAZARUS AND MCNUTT (1983) AND A COMPLETE
INSTRUMENT DESCRIPTION CAN BE FOUND IN BRIDGE (1977).
|
PRODUCER_FULL_NAME |
JOHN D. RICHARDSON
|
SEARCH/ACCESS DATA |
Planetary Plasma Interactions Website
|
|