Statistical analysis of long-duration low-density solar wind events

• Main Authors: S. Watari, T. Watanabe, K. Marubashi
• Format: Article
• Language: English
• Published: Copernicus Publications 2001-01-01
• Series: Annales Geophysicae
• Online Access: https://www.ann-geophys.net/19/17/2001/angeo-19-17-2001.pdf

Low solar wind density with long duration was measured by in situ observation between 11 and 12 May 1999. As a result of this low-density solar wind condition, the magnetosphere of the Earth expanded considerably. We used a database of one-hour-averaged solar wind (1963–1999) near 1 AU to determine whether or not the observed low-density event was extremely abnormal. As a result it was found that this event has the longest duration in approximately 36 years of solar wind observations. There are three events with density 0.5 cm^-3 or less and duration ten hours or longer. They were observed on 4 and 31 July 1979, and 11–12 May 1999. The 4 July 1979 event recurred on 31 July 1979. The events were characterized by low-beta, low Alfven Mach number (<i>M_A</i> ), and low dynamic pressure. The occurrence rate of low-density solar wind with density 0.5 cm^-3 or less shows several peaks near solar maxima. However, it is difficult to find a clear relationship between the sunspot number and the occurrence rate.<br><br><b>Key words. </b>Interplanetary physics (flare and stream dynamics; solar wind plasma; sources of the solar wind)