Data Set Information
DATA_SET_NAME VOYAGER 2 SATURN PLASMA DERIVED ELECTRON PARAMETERS 96 SEC
DATA_SET_ID VG2-S-PLS-5-SUMM-ELE-FIT-96SEC-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION Electron fit data from the Plasma experiment (PLS) on Voyager 2 from the Saturn encounter. The data set provides 96 second res. density and temperature measurements for various types of electrons (10-5950 eV).
DATA_SET_DESCRIPTION
Data Set Overview
        =================
          THIS DATA SET CONTAINS ELECTRON PARAMETERS IN THE PLS ENERGY
          RANGE (10-5950 EV) AT SATURN DURING THE VOYAGER 2 ENCOUNTER.
          PARAMETERS ARE CALCULATED IN SEVERAL WAYS.  TOTAL MOMENT
          DENSITY AND TEMPERATURE ARE GIVEN.  EACH ELECTRON SPECTRUM IS
          ALSO FIT WITH A THERMAL COMPONENT AND 1-3 HOT COMPONENTS
          DEPENDING ON HOW MANY MAXWELLIANS ARE NEEDED TO FIT THE ENTIRE
          DISTRIBUTION.  THE MOMENT DENSITY AND TEMPERATURE OF THE HOT
          COMPONENT IS CALCULATED AFTER THE THERMAL COMPONENT IS
          SUBTRACTED FROM THE SPECTRUM.  THE CHI-SQUARE VALUE FOR EACH
          FIT IS GIVEN.  THE SPACECRAFT CHARGE IS NOT CALCULATED
          CONSISTENTLY, AND MAY RESULT IN FACTOR OF 2-3 ERRORS IN THE
          THERMAL ELECTRON DENSITY.  DATA IS UNRELIABLE INSIDE 6 RS AND
          IN THE OCCULTATION REGIONS.  A COMPLETE DESCRIPTION OF THIS
          DATA SET IS IN SITTLERETAL. (1983).

          FITTING PARAMETERS ARE DESCRIBED AS BELOW:

          ===============================================================
          name      type      description
          ---------------------------------------------------------------
          time      A24       time in the format yyyy-mm-ddThh:mm:ss.sssZ
          imax      I2        points in spectrum
          ifly      I1        flag value: 1 = encounter, 0 = cruise
          thbn      1PE9.3    angle between d cup normal and mag. field
                                vector (radians)
          rne       1PE9.3    moment electron density (cnts/cm**3)
          rte       1PE9.3    moment electron temperature (eV)
          phisc     1PE9.3    spacecraft potential (V)
          rnc       1PE9.3    cold electron density (cnts/cm**3)
          sgnc      1PE9.3    std. dev. of cold electron density (rnc)
                                (cnts/cm**3)
          rtc       1PE9.3    cold electron temperature (eV)
          sgtc      1PE9.3    std. dev. of cold electron temperature
                                (rtc) (eV)
          chic      1PE9.3    chi squared of the cold fit
          rnh1      1PE9.3    first hot electron density (cnts/cm**3)
          sgnh1     1PE9.3    std. dev. of first hot electron dens.
                                (rnh1) (cnts/cm**3)
          th1       1PE9.3    first hot electron temperature (eV)
          sgth1     1PE9.3    std. dev. of first hot electron temp.
                                (th1) (eV)
          chih1     1PE9.3    chi squared of the first hot fit
          rnh2      1PE9.3    second hot electron density (cnts/cm**3)
          sgnh2     1PE9.3    std. dev. of second hot electron dens.
                                (rnh2) (cnts/cm**3)
          th2       1PE9.3    second hot electron temperature (eV)
          sgth2     1PE9.3    std. dev. of second hot electron temp.
                                (th2) (eV)
          chih2     1PE9.3    chi squared of second hot fit
          rnh3      1PE9.3    third hot electron density (cnts/cm**3)
          sgnh3     1PE9.3    std. dev. of third hot electron dens.
                                (rnh3) (cnts/cm**3)
          th3       1PE9.3    third hot electron temperature (eV)
          sgth3     1PE9.3    std. dev. of third hot electron temp.
                                (th1) (eV)
          chih3     1PE9.3    chi squared of third hot fit
          chi       1PE9.3    chi squared for total fit
          rnh       1PE9.3    moment of the hot electron density
                                (cnts/cm**3)
          rth       1PE9.3    moment of the hot electron temperature
                                (eV)

          IN COMPUTING RNH1 AND TH1 WE USED THE 3RD TO 7TH CHANNELS ABOVE
          THE BREAKPOINT ENERGY EB1 AND SUBTRACTED THE COLD COMPONENT FC
          FROM FE (OBSERVED) BEFORE DOING THE FIT.  IN REALITY THIS FIT
          WAS DONE ITERATIVELY BETWEEN THE COLD AND HOT COMPONENT FITS
          (FC=FE-FH AND FH=FE-FC ETC.).  A SIMILAR APPROACH WAS USED IN
          COMPUTING RNH3,TH3 FOR WHICH A MAXWELLIAN FIT WAS DONE TO THOSE
          CHANNELS ABOVE EB2.  THE PARAMETERS RNH2,TH2 WERE FIT TO THE
          UPPER 5 (3 MIN) CHANNELS (GENERALLY ABOVE EB2).  THIS FIT WAS
          PRIMARILY DONE TO ALLOW PROPER ESTIMATION OF FE TO THE HIGH
          ENERGY PORTION OF THE SPECTRUM.  IN MANY CASES THERE ARE NOT
          SUFFICIENT POINTS TO COMPUTE RNH3,TH3 AND RNH2,TH2 DO PROVIDE
          A FAIR REPRESENTATION OF THE SPECTRUM.  IF RNH1=RNH2=RNH3 THEN
          YOU SHOULD NOT USE THE 2ND AND 3RD FIT PARAMETERS.  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              : VG2
          Data Set Parameter Name         : ELECTRON DENSITY
          Instrument Parameter Name       : ELECTRON RATE
          Important Instrument Parameters : 1

          Instrument Host ID              : VG2
          Data Set Parameter Name         : ELECTRON DENSITY
          Instrument Parameter Name       : ELECTRON CURRENT
          Important Instrument Parameters : 1

          Instrument Host ID              : VG2
          Data Set Parameter Name         : ELECTRON TEMPERATURE
          Instrument Parameter Name       : ELECTRON RATE
          Important Instrument Parameters : 1

          Instrument Host ID              : VG2
          Data Set Parameter Name         : ELECTRON TEMPERATURE
          Instrument Parameter Name       : ELECTRON CURRENT
          Important Instrument Parameters : 1


        Processing
        ==========

          Processing History
          ------------------
            Source Data Set ID          : VG2-PLS
            Software                    : UNK
            Product Data Set ID         : VG2-S-PLS-5-ELE-PAR-96.0SEC
DATA_SET_RELEASE_DATE 2002-10-14T00:00:00.000Z
START_TIME 1981-08-25T12:00:42.991Z
STOP_TIME 1981-08-27T12:29:30.816Z
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 PLASMA SCIENCE EXPERIMENT
INSTRUMENT_ID PLS
INSTRUMENT_TYPE PLASMA INSTRUMENT
NODE_NAME Planetary Plasma Interactions
ARCHIVE_STATUS ARCHIVED
CONFIDENCE_LEVEL_NOTE
Confidence Level
    =================

          THIS DATA SET PROVIDES AN ESTIMATE OF THE ELECTRON PARAMETERS
          IN THE PLS ENERGY RANGE (10-5950 EV).  THE THERMAL ELECTRON
          DENSITY MAY BE UNDERESTIMATED BY FACTORS OF 2 IN SOME REGIONS
          DUE TO NEGATIVE SPACECRAFT CHARGING.  THERMAL ELECTRON
          PARAMETERS ARE ALSO UNRELIABLE INSIDE SIX KRONIAN RADII WHERE
          ELECTRON TEMPERATURES ARE COLD AND IN THE OCCULTATION REGIONS.
          HOT ELECTRONS ARE RELATIVELY UNDISTURBED BY CHARGING AND THESE
          PARAMETERS HAVE UNCERTAINTIES OF LESS THAN 20%.


    Data Coverage
    ==================
    Filename Records Start                     Stop
    ---------------------------------------------------------------------
    Volume ID: VG_1601
    ELE_FIT.TAB  1658  1981-08-25T00:00:42.991Z  1981-08-27T00:29:30.816Z


    Missing Data Flag
    ==================
    Any data column whose value is  9.999e+10 is a missing data value.
CITATION_DESCRIPTION Richardson, J.D., VG2-S-PLS-5-SUMM-ELE-FIT-96SEC-V1.0, VOYAGER 2 SATURN PLASMA DERIVED ELECTRON PARAMETERS 96 SEC, NASA Planetary Data System, 2002.
ABSTRACT_TEXT THIS DATA SET CONTAINS ELECTRON PARAMETERS IN THE PLS ENERGY RANGE (10-5950 EV) AT SATURN DURING THE VOYAGER 2 ENCOUNTER. PARAMETERS ARE CALCULATED IN SEVERAL WAYS. TOTAL MOMENT DENSITY AND TEMPERATURE ARE GIVEN. EACH ELECTRON SPECTRUM IS ALSO FIT WITH A THERMAL COMPONENT AND 1-3 HOT COMPONENTS DEPENDING ON HOW MANY MAXWELLIANS ARE NEEDED TO FIT THE ENTIRE DISTRIBUTION. THE MOMENT DENSITY AND TEMPERATURE OF THE HOT COMPONENT IS CALCULATED AFTER THE THERMAL COMPONENT IS SUBTRACTED FROM THE SPECTRUM. THE CHI-SQUARE VALUE FOR EACH FIT IS GIVEN. THE SPACECRAFT CHARGE IS NOT CALCULATED CONSISTENTLY, AND MAY RESULT IN FACTOR OF 2-3 ERRORS IN THE THERMAL ELECTRON DENSITY. DATA IS UNRELIABLE INSIDE 6 RS AND IN THE OCCULTATION REGIONS.
PRODUCER_FULL_NAME JOHN D. RICHARDSON
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