Solar flare and neutron telescope
โ Scribed by Y. Muraki; Y. Matsubara; I. Imaida; T. Koi; T. Murata; A. Okada; S. Sakakibara; T. Sako; H. Tsuchiya; Y. Munakata; S. Shibata; R. Tatsuoka; H. Sakai; T. Nonaka; T. Ohnishi; T. Wakasa; K. Hatanaka; Y. Ishida
- Book ID
- 114290383
- Publisher
- Elsevier Science
- Year
- 1998
- Tongue
- English
- Weight
- 603 KB
- Volume
- 60
- Category
- Article
- ISSN
- 0920-5632
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The upperlirnit on the solar neutron flux from 1-20 MeV has been measured, by a neutron detector on the OGO-6 satel!ite, to be less than 5 :-< 10 -z n cm -2 s -1 at the 95% confidence level for several flares including two flares of importance 3B and a solar proton event of importance 3B. The measur
It has previously been suggested that the energy for the optical emission of solar flares was provided by ionization losses of accelerated particles in the flares. We show that nuclear interaction of these particles would also produce fluxes of secondary neutrons and gamma rays detectable at the ear
We have derived the energy spectrum of accelerated protons and nuclei at the site of the June 21, 1980 limb flare by a new technique, using observations of the time-dependent flux of highenergy neutrons at the Earth. We find that this energy spectrum is very similar to the energy spectra of 7 disk f