On the origin of the consequent brightening of coronal loops in solar flare arcadesтезисы доклада

Дата последнего поиска статьи во внешних источниках: 22 февраля 2019 г.

Работа с тезисами доклада


[1] Леденцов Л. С., Сомов Б. В. On the origin of the consequent brightening of coronal loops in solar flare arcades // BUKS2018 Waves and instabilities in the solar atmosphere: Confronting the current state-of-the-art. — 2018. — P. 27–27. With the purpose of interpreting modern satellite observations of successively increasing the brightness of individual coronal loops in solar flares, we solved the problem of the stability of small longitudinal perturbations of a homogeneous reconnecting current layer in the MHD approximation. The suppression of the plasma thermal conductivity by the magnetic field inside the current layer provides an instability. The instability increases in a radiative cooling time scale of the plasma in the linear phase. A periodic structure of hot and cold fibers arranged transversely to the direction of the electric current are formed as a result of the instability. The proposed mechanism of the thermal instability can be useful for an explanation of the consistent increase in the brightness of individual coronal loops in solar flares.

Публикация в формате сохранить в файл сохранить в файл сохранить в файл сохранить в файл сохранить в файл сохранить в файл скрыть