Electron and Proton Peak Intensities Observed by a Five-Spacecraft Fleet

A table of parameters for a study of solar energetic particle events. The dataset likely contains event dates, flare characteristics, and particle onset and peak measurements from five spacecraft. It was published in Astronomy & Astrophysics in 2025 and is hosted by CERN and the European Commission.

Use Cases

• Correlate solar flare characteristics with proton and electron peak intensities based on flare class and location data.
• Analyze the timing and intensity of particle events across different spacecraft positions based on onset and peak time fields.
• Study the spatial distribution of solar energetic particles using spacecraft latitude, longitude, and radial distance fields.

Strengths

• Data is directly linked to a peer-reviewed publication in Astronomy & Astrophysics (A&A, 693 (2025) A198).
• Includes measurements from five distinct spacecraft (BepiColombo, L1, Parker Solar Probe, STEREO A, Solar Orbiter).
• Covers multiple particle types and energies (25 MeV protons and 100 keV electrons).

Limitations

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

Provenance

Source

CERN - European Organization for Nuclear Research and European Commission

Collection Method

Observational data from spacecraft instruments, compiled for a specific research publication.

Time Range

Solar Cycle 25 (likely covering events from approximately 2019 onward).

Freshness

Last updated 2025-06-09 00:00:00; freshness should be verified.