DATA_SET_DESCRIPTION |
Data Set Overview
=================
THIS DATA SET CONTAINS THE THERMAL ELECTRON DENSITY AND
TEMPERATURE IN THE PLS ENERGY RANGE (10-5950 EV) FROM VOYAGER 1
AT SATURN DERIVED BY FITTING THE LOW ENERGY ELECTRON COMPONENT
WITH A MAXWELLIAN DISTRIBUTION, AND THE MOMENT DENSITY AND
TEMPERATURE OF THE HOT ELECTRONS CALCULATED AFTER THE SIGNAL
FROM THE THERMAL COMPONENT IS SUBTRACTED FROM THE ELECTRON
SPECTRA. IT IS A SUBSET OF THE DATA SET
VG1-S-PLS-5-ELE-FIT-96.0SEC WHICH SHOULD BE OBTAINED BEFORE
THIS DATA IS USED. SPACECRAFT CHARGING MAY RESULT IN FACTOR OF
2-3 ERRORS IN THE THERMAL ELECTRON DENSITY. THE FIRST SIX
COLUMNS ARE THE TIME TAG (YEAR, DAY, HOUR, MIN, SEC, MSEC),
COLUMN 7 AND 8 ARE THE FIT DENSITY AND TEMPERATURE OF THE
THERMAL ELECTRON COMPONENT, AND 9 AND 10 ARE THE MOMENT DENSITY
AND TEMPERATURE OF THE SUPRATHERMAL ELECTRONS. EACH ROW HAS
THE FORMAT (6I5,4E12.4). 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 SITTLER ET AL. (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 : ELECTRON 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 giving an indication of the mean A
derived parameter equaling the number of electrons per unit
volume over a specified range of electron energy.
energy/electron, assuming the shape of the electron energy
Different forms of electron density are derived spectrum to
be Maxwellian (i.e.highest entropy shape). Given
distinguished by method of derivation (Maxwellian fit, that
the electron energy spectrum is not exactly Maxwellian,
method of moments) or by the some selection criteria (ie.,
the electron temperature can be defined integrally (whereby
the mean energy obtained by integrating under the actual hot
electron and cold electron density). In general, if more
electron energy spectrum is set equal to the integral under
than one electron component is analyzed, either by moment or
fit, a total density will be provided which is the sum of a
Maxwellian, where the temperature is a free parameter for the
electron densities. If the electron do not have a which to
solve), or differentially (whereby the slopes of Maxwellian
distribution the actual distribution can be the actually
electron energy spectrum at various energies are matched to
the slopes of a corresponding Maxwellian). represented as
the sum of several Maxwellians, in which case the density of
each Maxwellian is given. The temperature parameter is often
qualified with a range of applicable energies. temperatures
can be angularly anisotropic. If the electrons do not have a
Maxwellian distribution the actual distribution can be
represented as the sum of several Maxwellians, each with a
separate temperature.
Source Instrument Parameters
============================
Instrument Host ID : VG1
Data Set Parameter Name : ELECTRON DENSITY
Instrument Parameter Name : ELECTRON RATE
Important Instrument Parameters : 1
Instrument Host ID : VG1
Data Set Parameter Name : ELECTRON DENSITY
Instrument Parameter Name : ELECTRON CURRENT
Important Instrument Parameters : 1
Instrument Host ID : VG1
Data Set Parameter Name : ELECTRON TEMPERATURE
Instrument Parameter Name : ELECTRON RATE
Important Instrument Parameters : 1
Instrument Host ID : VG1
Data Set Parameter Name : ELECTRON TEMPERATURE
Instrument Parameter Name : ELECTRON CURRENT
Important Instrument Parameters : 1
Processing
==========
Processing History
------------------
Source Data Set ID : VG1-PLS
Software : UNK
Product Data Set ID : VG1-S-PLS-5-ELE-BR-96.0SEC
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ABSTRACT_TEXT |
THIS DATA SET CONTAINS THE THERMAL ELECTRON DENSITY AND
TEMPERATURE IN THE PLS ENERGY RANGE (10-5950 EV) FROM VOYAGER 1
AT SATURN DERIVED BY FITTING THE LOW ENERGY ELECTRON COMPONENT
WITH A MAXWELLIAN DISTRIBUTION, AND THE MOMENT DENSITY AND
TEMPERATURE OF THE HOT ELECTRONS CALCULATED AFTER THE SIGNAL FROM
THE THERMAL COMPONENT IS SUBTRACTED FROM THE ELECTRON SPECTRA. IT
IS A SUBSET OF THE DATA SET VG1-S-PLS-5-ELE-FIT-96.0SEC WHICH
SHOULD BE OBTAINED BEFORE THIS DATA IS USED. SPACECRAFT CHARGING
MAY RESULT IN FACTOR OF 2-3 ERRORS IN THE THERMAL ELECTRON
DENSITY. THE FIRST SIX COLUMNS ARE THE TIME TAG (YEAR, DAY, HOUR,
MIN, SEC, MSEC), COLUMN 7 AND 8 ARE THE FIT DENSITY AND
TEMPERATURE OF THE THERMAL ELECTRON COMPONENT, AND 9 AND 10 ARE
THE MOMENT DENSITY AND TEMPERATURE OF THE SUPRATHERMAL ELECTRONS.
EACH ROW HAS THE FORMAT (6I5,4E12.4). 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 SITTLER ET AL. (1983) AND A COMPLETE
INSTRUMENT DESCRIPTION CAN BE FOUND IN BRIDGE (1977).
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