Observation of the solar soft X-ray comp
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Richard G. Teske
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Article
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1969
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Springer
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English
โ 532 KB
Solar X-rays from 8 .12 ~ have been observed with an ion chamber photometer and fluxes derived from the observations after an assumption concerning the spectral distribution. The time variation of the X-ray flux correlates well with the radio flux, plagc index, and sunspot number. Comparisons of X-r