Место издания:Пулковская обсерватория Санкт-Петербург
Первая страница:325
Последняя страница:328
Аннотация:An overview of the velocities of coronal matter in the picture plane using the results ofLASCO SOHO observations is presented. General characteristics of moving coronal formations and their velocities are systematized. On the distances (2–6) Rʘ, events were detectedwith the movement of corona plasma both to the Sun and from its surface at speeds from tensto hundreds of km/s. The possible physical nature of the events is discussed.