The absence of flares in λ3835 and the heating of the chromosphere |
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Authors: | Harold Zirin |
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Institution: | (1) Big Bear Solar Observatory, Hale Observatories, California Institute of Technology, Carnegie Institution of Washington, U.S.A. |
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Abstract: | Simultaneous observations of flares in H and a band 15 Å wide centered on 3835 Å show no change whatever in 3835 Å at the time of several flares, although the chromospheric network is easily visible. Flares are therefore transparent in this wavelength.Since the flare represents a test heat input from above, and no brightening of the network appears, we conclude it is impossible for the corona to produce the bright network by downward convection. |
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