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
We thank the referee for the comments and we attach a PDF file with our detailed answers. The document gives a sequence of the referee’s original comments, followed by our answer and the corresponding modification of the text. We hope the answers and the changes can be convincing. The paper has been greatly improved as a result of this revision. The new version will be uploaded as soon as the s...
متن کاملInteractive comment on “Multiscale statistical analysis of coronal solar activity” by D. Gamborino et al
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, ...
متن کاملInteractive comment on “Multiscale statistical analysis of coronal solar activity” by D. Gamborino et al
The authors present an interesting spatio-temporal analysis of 4-dim solar data, for a flaring event, the preflare phase, and a Quiet Sun region. They use a Singular Value Decomposition method and investigate the multi-scale behavior of the physical parameter of the temperature T, and attempt to extract information on the heat flow dT/dx in a flare. The description of the method is clear, and t...
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