Voyager 1 CRS Electron Telescope Counting Rates at Saturn

192-second summary data from the Voyager 1 Cosmic Ray Subsystem Electron Telescope during the Saturn encounter. The D1 detector nominally responds to electrons with kinetic energies above approximately 1 MeV, and the D2 detector above approximately 2.5 MeV. Counting rates can reach up to approximately 50,000 counts per second, requiring deadtime correction near saturation.

Use Cases

• Analyze electron flux variations based on 192-second sampling intervals
• Model Saturn's radiation environment based on electron kinetic energy thresholds
• Correct for instrument deadtime effects based on the provided formula for high counting rates

Strengths

• Data originates from the Voyager 1 spacecraft's Cosmic Ray Subsystem, a primary NASA mission
• Sampling resolution and interval are precisely defined as 192.0 seconds
• Instrument noise level is explicitly stated as 0.000 counts/second

Limitations

• Column-level documentation is absent; field semantics must be inferred after download
• Row count is unknown, which may limit suitability assessment

Provenance

Source

National Aeronautics and Space Administration