Sectorial anisotropy of solar cosmic rays
β Scribed by S. P. Duggal; M. A. Pomerantz
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 701 KB
- Volume
- 27
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
A hitherto unobserved sectorial pattern of anisotropy that was limited to a narrow and stable region was displayed by the ground level event (GLE) of January 24, 1971. For the entire 1 89 h interval following onset before isotropy set in, the anisotropy was limited to a 10 ~ cone centered about 60 ~ from the spiral magnetic field line. It is also the first solar particle event for which it is possible, by analytical procedures based upon a theoretical propagation model, to distinguish between two rival candidates for the parent flare.
π SIMILAR VOLUMES
We briefly summarize our study on anisotropy of Ultra-High Energy Cosmic-Rays (UHECRs), in which we define a statistics that measures the correlation between UHECRs and Large Scale Structure (LSS). We also comment here on recently published paper by Koers and Tinyakov that compared our statistics to