๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Solar flare and neutron telescope

โœ 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.


๐Ÿ“œ SIMILAR VOLUMES


Solar-flare neutrons and gamma rays
โœ R.J. Murphy; R. Ramaty ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 805 KB
A search for solar neutrons during solar
โœ S. O. Ifedili ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 478 KB

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

Comptel measurements of solar flare neut
โœ J. Ryan; K. Bennett; H. Debrunner; D. Forrest; J. Lockwood; M. Loomis; M. McConn ๐Ÿ“‚ Article ๐Ÿ“… 1993 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 397 KB
Solar flare optical, neutron and gamma-r
โœ R. E. Lingenfelter ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 409 KB

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

Gamma-ray lines and neutrons from solar
โœ R. Ramaty; R. J. Murphy; B. Kozlovsky; R. E. Lingenfelter ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 759 KB

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