ULY JUP COSPIN KIEL ELE TEL HIRES: Raw Particle Count Rates from NASA Satellite

Raw particle count rates from the COSPIN instrument suite, likely collected by the Ulysses (ULY) or other spacecraft. The data includes single counter rates for a Semiconductor Detector (D1) and an Anticoincidence detector (A), provided by the National Aeronautics and Space Administration. The dataset was last updated on March 13, 2026.

Use Cases

• Modeling cosmic ray modulation in the heliosphere based on particle count rates.
• Studying solar energetic particle events based on detector rate time series.
• Calibrating or validating particle detector simulations based on raw counter data.
• Analyzing long-term trends in galactic cosmic rays based on satellite observations.

Strengths

• Data originates from the National Aeronautics and Space Administration, a highly authoritative source.
• The dataset was last updated on March 13, 2026, indicating recent maintenance.

Limitations

• Description metadata is limited; actual data quality requires manual inspection after download.
• 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

Collection Method

Likely collected by satellite-based particle detectors (e.g., Ulysses spacecraft).

Freshness

Last updated 2026-03-13 03:49:22.445332