Anomalous Heating of the Solar Atmosphere in the Epoch of the Solar Activity Minimum
- 作者: Romanov K.1
-
隶属关系:
- Astafiev Krasnoyarsk State Pedagogical University
- 期: 卷 59, 编号 8 (2019)
- 页面: 1121-1127
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/158014
- DOI: https://doi.org/10.1134/S0016793219080164
- ID: 158014
如何引用文章
详细
The article studies the physical mechanism of the generation of a steady stream of weak shock waves at the photospheric level during the epoch of the solar-activity cycle minimum. The distribution of altitude thermodynamic parameters within the solar chromosphere are calculated with the relaxation method. A nonlinear increase in wave-flow power in the lower layers of the solar atmosphere has been determined in the epoch of increased cycle activity. The physical mechanism of radiative heating of the solar atmosphere is studied at the stage of increased cycle activity.
作者简介
K. Romanov
Astafiev Krasnoyarsk State Pedagogical University
编辑信件的主要联系方式.
Email: k-v-romanov@yandex.ru
俄罗斯联邦, Krasnoyarsk