Revisiting the Question: The Cause of the Solar Cycle Variation of Total Solar Irradiance
The Mg II index and sunspot area are usually used to represent the intensification contribution by solar bright structures to total solar irradiance (TSI) and sunspot darkening, respectively. In order to understand the cause of the solar cycle variation of TSI, we use extension of wavelet transform,...
| Published in: | Advances in Astronomy |
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| Main Author: | |
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2019-01-01
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| Online Access: | http://dx.doi.org/10.1155/2019/3641204 |