Structure of the Long-Living Elements of Solar Granulation
- Авторлар: Baran O.A.1, Stodilka M.I.1, Prysiazhnyi A.I.1
-
Мекемелер:
- Astronomical Observatory
- Шығарылым: Том 34, № 1 (2018)
- Беттер: 13-18
- Бөлім: Solar Physics
- URL: https://journals.rcsi.science/0884-5913/article/view/178022
- DOI: https://doi.org/10.3103/S0884591318010026
- ID: 178022
Дәйексөз келтіру
Аннотация
Spatial and temporal variations in thermodynamic and kinematic parameters of structural elements of solar granulation are investigated by solving the inverse nonequilibrium radiative transfer problem using the observational data from the Vacuum Tower Telescope (duration of observations 2.6 h). In the lower photosphere, we have detected long-living (with lifetime up to 1.5 h) structures—trees of fragmenting granules. They occur as a result of the division of an ascending granular flow into several fragments, which can be repeated multiple times. We have found that approximately 67% of the regions with the highest positive variations of pressure correspond to the time and place of fragmentation of granular flows; approximately 12% of the regions correspond to the approach of adjacent structures.
Негізгі сөздер
Авторлар туралы
O. Baran
Astronomical Observatory
Хат алмасуға жауапты Автор.
Email: lesiaab@gmail.com
Украина, Lviv, 79005
M. Stodilka
Astronomical Observatory
Email: lesiaab@gmail.com
Украина, Lviv, 79005
A. Prysiazhnyi
Astronomical Observatory
Email: lesiaab@gmail.com
Украина, Lviv, 79005
Қосымша файлдар
