Coronal loop: Difference between revisions

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1991–present day: The Sun's surface itself (photosphere) is only 5500 Cº.
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===1991–present day===
[[Image:Tracemosaic.jpg|thumb|Full-disk mosaic of the million-degree [[Sun]]corona by [[TRACE]]]]
 
In August 1991, the solar observatory spacecraft [[Yohkoh]] launched from the [[Kagoshima Space Centre|Kagoshima Space Center]]. During its 10 years of operation, it revolutionized X-ray observations. Yohkoh carried four instruments; of particular interest is the SXT instrument, which observed X-ray-emitting coronal loops. This instrument observed X-rays in the 0.25–4.0&nbsp;[[SI units|keV]] range, resolving solar features to 2.5 arc seconds with a temporal resolution of 0.5–2 seconds. SXT was sensitive to plasma in the 2–4&nbsp;MK temperature range, making its data ideal for comparison with data later collected by TRACE of coronal loops radiating in the extra ultraviolet (EUV) wavelengths.<ref>{{cite journal