Application of the solar plasma density investigation method based on the solar flare 2.223 MeV gamma-line time profile analysis to the experimental data

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

In the previous works we have shown the possibility of determining solar plasma density altitude profile in the period of solar flare by means of solar flare 2.22 MeV neutron capture gamma-line time profile analysis. The method is a unique possibility to experimentally investigate the deep layers photospheric and subphotospheric, inaxessible to another methods. It have been shown that the most important factors, which impact on the 2.22 MeV gamma-line time profile, are characteristics of initial neutron flux, surrounding medium parameters, neutron decay, neutron and gamma-ray interactions with the medium. Previously we have made allowance for the most part of these factors. In the present work we present the exact calculaions of non-radiative absorption of neutrons by helium-3, as an additional loss of neutrons, which form 2.22 MeV gamma-emission, and investigate the solar flare gamma-line 2.22 MeV time profile dependencies on initial neutron escape geometry. Then we apply the new calculated time profiles to the analysis of the solar gamma-flares experimental data within the framework of the method.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Application of the solar plasma density investigation method based on the solar flare 2.223 MeV gamma-line time profile analysis to the experimental data does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Application of the solar plasma density investigation method based on the solar flare 2.223 MeV gamma-line time profile analysis to the experimental data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Application of the solar plasma density investigation method based on the solar flare 2.223 MeV gamma-line time profile analysis to the experimental data will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-798199

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.