Relativistic solar protons in the event of January 20, 2005: Model studies
Using the optimization methods, the characteristics of relativistic solar protons (RSPs) have been obtained from the data of ground-based cosmic ray detectors in the event of January 20, 2005, which was the largest event in the last 50 years since the event of February 23, 1956. The RSP dynamics dur...
Gespeichert in:
Veröffentlicht in: | Geomagnetism and Aeronomy 2006-07, Vol.46 (4), p.424-429 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | Using the optimization methods, the characteristics of relativistic solar protons (RSPs) have been obtained from the data of ground-based cosmic ray detectors in the event of January 20, 2005, which was the largest event in the last 50 years since the event of February 23, 1956. The RSP dynamics during the event has been studied. The existence of two populations (components) of particles, fast and delayed (slow) has been shown. The fast component with a hard exponential energy spectrum and strong anisotropy was shown as a giant pulselike enhancement at several southern polar stations. The delayed component had a power-law energy spectrum and a wider pitch-angle distribution, which caused the enhancement effect at the majority of stations at the global network.[PUBLICATION ABSTRACT] |
---|---|
ISSN: | 0016-7932 1555-645X 0016-7940 |
DOI: | 10.1134/S0016793206040037 |