Data Access
Counting Rate from the D2 Detector in the Cosmic Ray Subsystem (CRS) Electron Telescope (TET) on Voyager 2 during the Uranus Encounter. The D2 Detector nominally responds to Electrons with Kinetic Energies above approximately 2.5 MeV (see Detector Description for Details).
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| Parameter Characteristics | Value |
| Sampling Parameter Name | TIME |
| Sampling Parameter Resolution | 6.0 SECONDS |
| Minimum Sampling Parameter | N/A |
| Maximum Sampling Parameter | N/A |
| Sampling Parameter Interval | 96.0 SECONDS |
| Minimum available Sampling Int | 96.0 SECONDS |
| Sampling Parameter Unit | SECOND |
| Data Set Parameter Name | D2 RATE |
| Noise Level | 0.000 COUNTS/SECOND |
| Data Set Parameter Unit | COUNTS/SECOND |
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Version:2.3.0
Counting Rate from the D2 Detector in the Cosmic Ray Subsystem (CRS) Electron Telescope (TET) on Voyager 2 during the Uranus Encounter. The D2 Detector nominally responds to Electrons with Kinetic Energies above approximately 2.5 MeV (see Detector Description for Details).
+------------------------------------------------------+
| Parameter Characteristics | Value |
| Sampling Parameter Name | TIME |
| Sampling Parameter Resolution | 6.0 SECONDS |
| Minimum Sampling Parameter | N/A |
| Maximum Sampling Parameter | N/A |
| Sampling Parameter Interval | 96.0 SECONDS |
| Minimum available Sampling Int | 96.0 SECONDS |
| Sampling Parameter Unit | SECOND |
| Data Set Parameter Name | D2 RATE |
| Noise Level | 0.000 COUNTS/SECOND |
| Data Set Parameter Unit | COUNTS/SECOND |
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| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | MetadataContact | spase://SMWG/Person/Todd.A.King | |||
| 2. | MetadataContact | spase://SMWG/Person/Lee.Frost.Bargatze |
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This Collection is archived with NASA Planetary Data System.