Return to search results
VG1 SAT PLS DERIVED ION MAGNETOSHEATH 96SEC V1.0
This data set contains Voyager 1 plasma fit data from Saturn's magnetosphere. The fit parameters assume a convected isotropic proton Maxwellian distribution. Use of fit parameters is recommended as these are normally more accurate. Since only the first 72 or last 72 energy/charge channels are telemetered to Earth from each M-mode spectra, derived parameters change significantly only every other set of spectra so the effective time resolution is 96 second.
Complete Metadata
| @type | dcat:Dataset |
|---|---|
| accessLevel | public |
| accrualPeriodicity | irregular |
| bureauCode |
[
"026:00"
]
|
| contactPoint |
{
"fn": "Thomas Morgan",
"@type": "vcard:Contact",
"hasEmail": "mailto:thomas.h.morgan@nasa.gov"
}
|
| description | This data set contains Voyager 1 plasma fit data from Saturn's magnetosphere. The fit parameters assume a convected isotropic proton Maxwellian distribution. Use of fit parameters is recommended as these are normally more accurate. Since only the first 72 or last 72 energy/charge channels are telemetered to Earth from each M-mode spectra, derived parameters change significantly only every other set of spectra so the effective time resolution is 96 second. |
| identifier | urn:nasa:pds:context_pds3:data_set:data_set.vg1-s-pls-5-summ-ion-magsheath-96s-v1.0_n8it-hq5x |
| issued | 2018-06-26 |
| keyword |
[
"voyager"
]
|
| landingPage | https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=VG1-S-PLS-5-SUMM-ION-MAGSHEATH-96S-V1.0 |
| modified | 2025-07-17 |
| programCode |
[
"026:005"
]
|
| publisher |
{
"name": "National Aeronautics and Space Administration",
"@type": "org:Organization"
}
|
| references |
[
"https://pds.nasa.gov"
]
|
| theme |
[
"Earth Science"
]
|
| title | VG1 SAT PLS DERIVED ION MAGNETOSHEATH 96SEC V1.0 |
