Interactive comment on “Multiscale statistical analysis of coronal solar activity” by D. Gamborino et al
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چکیده
However, the temperature maps as provided by the method of Aschwanden et al. involve several strong assumptions. In particular, these temperature maps are assuming an isothermal plasma, which is a coarse approximation of what the true corona is; it certainly does not hold during flaring activity, and it is likely too to be incorrect too during transients, such as your heat fronts. In addition, flares cause artefacts such as pixel bleeding. Another good reason to be very careful when interpreting synoptic EUV images.
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Interactive comment on “Multiscale statistical analysis of coronal solar activity” by D. Gamborino et al
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Interactive comment on “Multiscale statistical analysis of coronal solar activity” by D. Gamborino et al
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