Using the 17 and 34 GHz Nobeyama Redioheliograph observations the July 13, 2000 transequatorial eruptive prominence was studied. It was found that the eruption started near the bright equatorial feature which reappeared th the post-eruption phase.
Using the 17 and 34 GHz Nobeyama Redioheliograph observations the July 13, 2000 transequatorial eruptive prominence was studied. It was found that the eruption started near the bright equatorial feature which reappeared th the post-eruption phase. (en)