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Voyager 2 Neptune Cosmic Ray Subsystem (CRS) Electron Telescope D2 Counting Rates, Version 1.0, 96 s Summary Data

ResourceID
spase://NASA/NumericalData/Voyager2/CRS/Neptune/PT96S

Description
  • Data Set Overview
  • =================

Counting Rate from the D2 Detector in the Cosmic Ray Subsystem (CRS) Electron Telescope (TET) on Voyager 2 during the Neptune Encounter. The D2 Detector nominally responds to Electrons with Kinetic Energies above approximately 2.5 MeV (see Detector Description for Details).

  • Parameters
  • ==========

+-----------------------------------------------------------+
| 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 Interval | 96.0 SECONDS |
| Data Set Parameter Name | D2 RATE |
| Noise Level | 0.000 COUNTS/SECOND |
| Data Set Parameter Unit | COUNTS/SECOND |
+-----------------------------------------------------------+

The D2 Detector is located behind the D1 Detector in the TET, so that most of the Electrons observed by D2 have to penetrate D1 first. The D2 Rate therefore applies to Higher Energy Electrons and the Threshold Energy is less distinct than for D1, but is near 2.5 MeV. The Rate can be calculated from the Electron Differential Flux in the same way as the D1 RATE (see D1 RATE Description) with the following Calibration Table.

Table 1. D2 Response Function

+----------------------------------------------------------------+
| Energy | 11 | 23 | 41 | 61 | 80 | 90 | 100 |


| 0.989 | 0.000 | 0.000 | 0.000 | 0.001 | 0.002 | 0.001 | 0.001 |
| 1.179 | 0.000 | 0.000 | 0.000 | 0.013 | 0.023 | 0.021 | 0.018 |
| 1.372 | 0.000 | 0.000 | 0.000 | 0.037 | 0.052 | 0.051 | 0.043 |
| 1.567 | 0.000 | 0.019 | 0.028 | 0.063 | 0.082 | 0.066 | 0.061 |
| 1.763 | 0.041 | 0.034 | 0.045 | 0.090 | 0.111 | 0.098 | 0.080 |
| 1.959 | 0.106 | 0.078 | 0.072 | 0.119 | 0.142 | 0.125 | 0.097 |
| 2.157 | 0.255 | 0.186 | 0.127 | 0.152 | 0.170 | 0.146 | 0.109 |
| 2.355 | 0.488 | 0.381 | 0.228 | 0.206 | 0.212 | 0.176 | 0.126 |
| 2.553 | 0.772 | 0.627 | 0.361 | 0.272 | 0.255 | 0.202 | 0.139 |
| 2.752 | 1.019 | 0.864 | 0.501 | 0.340 | 0.299 | 0.226 | 0.152 |
| 2.951 | 1.220 | 1.053 | 0.634 | 0.400 | 0.335 | 0.250 | 0.165 |
| 3.150 | 1.461 | 1.218 | 0.746 | 0.459 | 0.375 | 0.289 | 0.188 |
| 3.350 | 1.628 | 1.378 | 0.940 | 0.515 | 0.456 | 0.411 | 0.282 |
+----------------------------------------------------------------+

  • Processing
  • ==========

The ENCYCLOPEDIA GENERATOR Program was run by Nand Lal at Goddard Space Flight Center to read the EDR Tape, check for Error Conditions, and reformat the Data to generate a CRS Encyclopedia Tape. The resulting Tape was sent to CalTech for subsequent Data Analysis.

The VCRUSH Program was run at CalTech to select Data of Interest from CRS Encyclopedia Tapes. In the Case of Counting Rate Data, no further Analysis was done to produce the Data in the PDS Data Sets.

Note: Neither the ENCYCLOPEDIA GENERATOR or VCRUSH Software are available for Public Use.

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Details

Version:2.3.0

NumericalData

ResourceID
spase://NASA/NumericalData/Voyager2/CRS/Neptune/PT96S
ResourceHeader
ResourceName
Voyager 2 Neptune Cosmic Ray Subsystem (CRS) Electron Telescope D2 Counting Rates, Version 1.0, 96 s Summary Data
ReleaseDate
2020-07-07 21:15:55Z
Description
  • Data Set Overview
  • =================

Counting Rate from the D2 Detector in the Cosmic Ray Subsystem (CRS) Electron Telescope (TET) on Voyager 2 during the Neptune Encounter. The D2 Detector nominally responds to Electrons with Kinetic Energies above approximately 2.5 MeV (see Detector Description for Details).

  • Parameters
  • ==========

+-----------------------------------------------------------+
| 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 Interval | 96.0 SECONDS |
| Data Set Parameter Name | D2 RATE |
| Noise Level | 0.000 COUNTS/SECOND |
| Data Set Parameter Unit | COUNTS/SECOND |
+-----------------------------------------------------------+

The D2 Detector is located behind the D1 Detector in the TET, so that most of the Electrons observed by D2 have to penetrate D1 first. The D2 Rate therefore applies to Higher Energy Electrons and the Threshold Energy is less distinct than for D1, but is near 2.5 MeV. The Rate can be calculated from the Electron Differential Flux in the same way as the D1 RATE (see D1 RATE Description) with the following Calibration Table.

Table 1. D2 Response Function

+----------------------------------------------------------------+
| Energy | 11 | 23 | 41 | 61 | 80 | 90 | 100 |


| 0.989 | 0.000 | 0.000 | 0.000 | 0.001 | 0.002 | 0.001 | 0.001 |
| 1.179 | 0.000 | 0.000 | 0.000 | 0.013 | 0.023 | 0.021 | 0.018 |
| 1.372 | 0.000 | 0.000 | 0.000 | 0.037 | 0.052 | 0.051 | 0.043 |
| 1.567 | 0.000 | 0.019 | 0.028 | 0.063 | 0.082 | 0.066 | 0.061 |
| 1.763 | 0.041 | 0.034 | 0.045 | 0.090 | 0.111 | 0.098 | 0.080 |
| 1.959 | 0.106 | 0.078 | 0.072 | 0.119 | 0.142 | 0.125 | 0.097 |
| 2.157 | 0.255 | 0.186 | 0.127 | 0.152 | 0.170 | 0.146 | 0.109 |
| 2.355 | 0.488 | 0.381 | 0.228 | 0.206 | 0.212 | 0.176 | 0.126 |
| 2.553 | 0.772 | 0.627 | 0.361 | 0.272 | 0.255 | 0.202 | 0.139 |
| 2.752 | 1.019 | 0.864 | 0.501 | 0.340 | 0.299 | 0.226 | 0.152 |
| 2.951 | 1.220 | 1.053 | 0.634 | 0.400 | 0.335 | 0.250 | 0.165 |
| 3.150 | 1.461 | 1.218 | 0.746 | 0.459 | 0.375 | 0.289 | 0.188 |
| 3.350 | 1.628 | 1.378 | 0.940 | 0.515 | 0.456 | 0.411 | 0.282 |
+----------------------------------------------------------------+

  • Processing
  • ==========

The ENCYCLOPEDIA GENERATOR Program was run by Nand Lal at Goddard Space Flight Center to read the EDR Tape, check for Error Conditions, and reformat the Data to generate a CRS Encyclopedia Tape. The resulting Tape was sent to CalTech for subsequent Data Analysis.

The VCRUSH Program was run at CalTech to select Data of Interest from CRS Encyclopedia Tapes. In the Case of Counting Rate Data, no further Analysis was done to produce the Data in the PDS Data Sets.

Note: Neither the ENCYCLOPEDIA GENERATOR or VCRUSH Software are available for Public Use.

Contacts
RolePersonStartDateStopDateNote
1.MetadataContactspase://SMWG/Person/Todd.A.King
2.MetadataContactspase://SMWG/Person/Lee.Frost.Bargatze
InformationURL
Name
VG2-N-CRS-4-SUMM-D2-96SEC-V1.0
URL
Description

The Document describing the Contents of the Collection.

Language
En
PriorIDs
spase://VMO/NumericalData/Voyager2/CRS/Neptune/PT96S
spase://VSPO/NumericalData/Voyager2/CRS/Neptune/PT96S
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
PDS/PPI
URL
ProductKey
VG2-N-CRS-4-SUMM-D2-96SEC-V1.0
Description

This Collection is archived with NASA Planetary Data System.

Language
En
Format
Text.ASCII
Acknowledgement
NASA Planetary Plasma Interactions (PPI) Node of the Planetary Data System (PDS) and the Principal Investigator for the Data.
InstrumentIDs
MeasurementType
EnergeticParticles
TemporalDescription
TimeSpan
StartDate
1989-08-24 22:00:00.00
StopDate
1989-08-25 10:00:00.00
Cadence
PT96S
ObservedRegion
Neptune