作者: A. Egeland , H.C. Carlson , W.F. Denig , K. Fukui , E. Weber
DOI: 10.1109/27.199521
关键词:
摘要: The height distribution of the dayside cusp aurora and relation between optical emissions net downward electron energy flux are discussed. These two important characteristics day-side still unknown. It is instructive to compare particle luminosity because these quantities should be proportional if caused by impact, as has been found for nighttime in oval. Furthermore, there then a direct auroral altitudes energy. Based on coordinated observations at Svalbard Greenland, together with simultaneous, overhead F-9 satellite measurements, have evaluated. >