New Views of Active Regions, Flares and CME’s from Space

  • Y. Uchida
Conference paper
Part of the NATO Science Series book series (ASIC, volume 558)


In the present article, we treat (1) the problem of how the active region coronae are heated in extra and supplied mass, and (2) the problems of how the small but high energy loop flares, and the large and dynamic arcade flares, sometimes accompanying massive coronal mass ejections, occur, based on the new observational results derived from the recent satellites, Yohkoh, SOHO, and TRACE, that revolutionized our knowledge about solar, and therefore, stellar activity. We also discuss possible models we propose to interpret those.


Coronal Mass Ejection Solar Phys Solar Flare Flux Tube Separatrix Surface 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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© Springer Science+Business Media Dordrecht 2000

Authors and Affiliations

  • Y. Uchida
    • 1
  1. 1.Physics DepartmentScience University of TokyoTokyoJapan

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