An X-ray observation in the atmosphere during the August 7, 1972 solar flare
An observation carried out with a balloon-borne detector of an additional flux of secondary X-rays (E ≃ 30 keV) at large depths in the atmosphere is described. This excess is attributed to the emission of very hard X-rays during the solar flare of August 7, 1972. The propagation in the atmosphere of...
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| Autores principales: | Ghielmetti, H.S., Azcárate, I.N., Mugherli, V.J. |
|---|---|
| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004640X_v226_n1_p19_Ghielmetti |
| Aporte de: |
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