YOHKOH Results in the Context of the High-Latitude Heliosphere

Details YOHKOH Results in the Context of the High-Latitude Heliosphere YOHKOH Results in the Context of the High-Latitude Heliosphere

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...72...17c&link_type=abstract

Space Science Reviews, Volume 72, Issue 1-2, pp. 17-28

Computer Science

Scientific paper

Designed primarily to study solar activity, Yohkoh includes an X-ray telescope that obtains full-sun coronal images which show a range of features. Coronal X-ray emission-exclusive of flares, is notable for its variability even in the largest structures. A mass ejection event is related to magnetic field reconnection. Such events exhibit both accelerated and decelerated behaviour. Coronal hole temperatures are estimated from the filter ratio method. A plasma component at around 2.106 K is identified. X-ray emission is detected from the South polar coronal hole. A preliminary comparison of Spartan coronagraph images with Yohkoh data suggests that polar plumes or rays are not connected to bright points.

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