Studying subsecond X-ray and radio bursts (spikes) in solar flares provides insights into the temporal characteristics of magnetic reconnection and particle acceleration in the solar atmosphere. These rapid flux variations reveal the characteristic timescales of energy release processes in flares. Here, we analyzed an M2.8 flare that occurred on January 12, 2000, during which both X-ray and radio bursts were recorded. We detected bursts using an improved empirical mode decomposition technique that offers high sensitivity and a low false-positive rate. Analysis of the flare's temporal structure revealed delays between bursts in different energy bands and allowed us to estimate the plasma parameters in the emission region. Keywords: solar flares, hard X-ray (HXR) emission, radio emission, sub-second bursts, particle acceleration, magnetic reconnection.

Подсчитывается количество просмотров абстрактов ("html" на диаграммах) и полных версий статей ("pdf"). Просмотры с одинаковых IP-адресов засчитываются, если происходят с интервалом не менее 2-х часов.

Дата начала обработки статистических данных - 27 января 2016 г.