๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

THE RELATIONSHIP BETWEEN SOLAR FLARE GAMMA-RAY EMISSION AND NEUTRON PRODUCTION

โœ Scribed by J. A. Lockwood; H. Debrunner; J. M. Ryan


Book ID
110217199
Publisher
Springer
Year
1997
Tongue
English
Weight
879 KB
Volume
173
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


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

Solar flare neutrons and their capture g
โœ X M. Hua; R. E. Lingenfelter ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 412 KB

We briefly describe our recent Monte Carlo calculations of the energy and angular distributions of neutrons escaping from the solar atmosphere. Comparing the calculation results with measurements of the neutron flux from the flares, we determined the angular distribution and energy spectrum of the a

Solar-flare neutrons and gamma rays
โœ R.J. Murphy; R. Ramaty ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 805 KB
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

On the relation between solar-flare gamm
โœ V. V. Zaitsev; A. V. Stepanov ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 559 KB

It is shown that escaping of solar flare energetic protons into interplanetary space as well as their relation to the flare gamma-ray emission depend on the parameter/~ = 8np/B~, where p is the pressure of hot plasma and energetic particles and Bo is the magnetic field in a flaring loop. If/3 ~ 1, t