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Voyager 2 96 second electron spectra data using several isotropic
Maxwelian distribution functions to find electron parameters from
Voyager 2 during the Neptune encounter from 1989-08-24 to 1989-08-25.
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Citation |
Richardson, J.D., VG2-N-PLS-5-RDR-ELEMAGSPHERE-96SEC-V1.0,
VG2 NEP PLS DERIVED RDR ELECTRON MAGNETOSPHERE 96SEC V1.0,
NASA Planetary Data System, 1991. |
Digital Object Identifier (DOI) |
10.17189/1519977
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Data Set Abstract |
The electron spectra are fit using several isotropic Maxwellian
distribution functions to find electron parameters. The spacecraft
charge may seriously affect the density measurements. The temperature
of each component is, however, independent of the spacecraft potential.
To obtain the best estimate of the electron density, the encounter
period is divided into four regions and four different analysis methods
are used. |
Search/Access Data |
Planetary Plasma Interactions Website
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Additional Information |
Mission Information |
VOYAGER
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Data Set Information |
VG2-N-PLS-5-RDR-ELEMAGSPHERE-96SEC-V1.0 |
Instrument Host Information |
VG2
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Instrument Information |
PLS
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Target Information |
NEPTUNE
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