Webb7 jan. 1998 · A theory for the origin of the slow solar wind is described. Recent papers have demonstrated that magnetic flux moves across coronal holes as a result of the interplay … WebbIt is also found that slow normal CMEs experience the same amount of erosion, regardless of the background wind density. Moreover, as the initial velocity increases, so does the influence of the wind density on the erosion. We found that increasing the CME speed leads to a higher overall erosion due to stronger magnetic reconnection.

On the sources of fast and slow solar wind - Feldman - 2005

WebbThis fast solar wind is relatively slightly variable. In regions closer to the equator, the solar wind is more variable and slower, on average 400 km/s. One speaks of fast and slow … Webb11 maj 2016 · Now, a team at NASA's Goddard Space Flight Center in Greenbelt, Maryland, has explored a detailed case study of the slow solar wind, using newly processed observations close to Earth to determine... irc 6 explanatory

Solar wind speeds, fast and slow - BIRA-IASB

Webb25 maj 2024 · The slow solar wind is typically characterized as having low Alfvénicity. However, Parker Solar Probe (PSP) observed predominately Alfvénic slow solar wind during several of its initial encounters. Webb10 maj 2016 · Now, a team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, has explored a detailed case study of the slow solar wind, using newly processed … WebbRecent SOHO/UVCS observations of the O5+ ion line emission at 1032A in coronal streamers indicate that the emission is stronger by an order of magnitude at the edges … irc 55 pdf download