| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8139309 | Journal of Atmospheric and Solar-Terrestrial Physics | 2018 | 7 Pages |
Abstract
We suggest that we observed the photoionization-recombination process caused by UV radiation from the transition region and corona during the coronal flare. With this, we point out the difficulties in interpreting the time lag between the emission maximum in the SDO UV channels and the second absorption maximum in the He i 10830â¯Ã
line.
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Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Nikolai Kobanov, Andrei Chelpanov, Vasiliy Pulyaev,