Scattering of fast flare electrons in solar atmosphere and their X-ray spectrum
The evolution of the energy distributions of fast flare electrons injected toward the chromosphere are computed by the Monte Carlo method for different depths. By using these distributions, power law bremsstrahlung spectra having spectral indices increasing with photon energies are obtained.
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| Published in | Solar physics Vol. 57; no. 2; pp. 409 - 413 |
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| Main Authors | , |
| Format | Journal Article |
| Language | English |
| Published |
01.04.1978
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| Online Access | Get full text |
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| Summary: | The evolution of the energy distributions of fast flare electrons injected toward the chromosphere are computed by the Monte Carlo method for different depths. By using these distributions, power law bremsstrahlung spectra having spectral indices increasing with photon energies are obtained. |
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| Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
| ISSN: | 0038-0938 1573-093X |
| DOI: | 10.1007/BF00160113 |