Abstract
Nearly 1000 solar events with fluxes measured in 0.5-3A/sup 0/, 1-8A/sup 0/ and 8-20A/sup 0/ bands by Explorer 37 (US NRL Solrad) satellite are statistically analyzed. The differential distribution of peak fluxes can be represented by power laws with exponents -1.4, -2.2, -2.9 respectively, which are compared to 2-12A/sup 0/ results. For the 0.5-3A/sup 0/ band there is a suggested peak in the distribution. Autocorrelation analyses of the distribution have shown that in the harder band (0.5-3A/sup 0/) there is a concentration of events at preferred values multiplied of about 10x10/sup -5/erg cm/sup -2/S/sup -1/ of unknown origin.
Kaufmann, P;
Piazza, L R;
Schaal, R E
[1]
- Universidade Mackenzie, Sao Paulo (Brazil). Centro de Radio-Astronomia e Astrofisica
Citation Formats
Kaufmann, P, Piazza, L R, and Schaal, R E.
Statistical distribution of solar soft X-ray bursts.
Brazil: N. p.,
1979.
Web.
Kaufmann, P, Piazza, L R, & Schaal, R E.
Statistical distribution of solar soft X-ray bursts.
Brazil.
Kaufmann, P, Piazza, L R, and Schaal, R E.
1979.
"Statistical distribution of solar soft X-ray bursts."
Brazil.
@misc{etde_5790401,
title = {Statistical distribution of solar soft X-ray bursts}
author = {Kaufmann, P, Piazza, L R, and Schaal, R E}
abstractNote = {Nearly 1000 solar events with fluxes measured in 0.5-3A/sup 0/, 1-8A/sup 0/ and 8-20A/sup 0/ bands by Explorer 37 (US NRL Solrad) satellite are statistically analyzed. The differential distribution of peak fluxes can be represented by power laws with exponents -1.4, -2.2, -2.9 respectively, which are compared to 2-12A/sup 0/ results. For the 0.5-3A/sup 0/ band there is a suggested peak in the distribution. Autocorrelation analyses of the distribution have shown that in the harder band (0.5-3A/sup 0/) there is a concentration of events at preferred values multiplied of about 10x10/sup -5/erg cm/sup -2/S/sup -1/ of unknown origin.}
journal = []
volume = {9:1}
journal type = {AC}
place = {Brazil}
year = {1979}
month = {Mar}
}
title = {Statistical distribution of solar soft X-ray bursts}
author = {Kaufmann, P, Piazza, L R, and Schaal, R E}
abstractNote = {Nearly 1000 solar events with fluxes measured in 0.5-3A/sup 0/, 1-8A/sup 0/ and 8-20A/sup 0/ bands by Explorer 37 (US NRL Solrad) satellite are statistically analyzed. The differential distribution of peak fluxes can be represented by power laws with exponents -1.4, -2.2, -2.9 respectively, which are compared to 2-12A/sup 0/ results. For the 0.5-3A/sup 0/ band there is a suggested peak in the distribution. Autocorrelation analyses of the distribution have shown that in the harder band (0.5-3A/sup 0/) there is a concentration of events at preferred values multiplied of about 10x10/sup -5/erg cm/sup -2/S/sup -1/ of unknown origin.}
journal = []
volume = {9:1}
journal type = {AC}
place = {Brazil}
year = {1979}
month = {Mar}
}