Consisting of a plasma that is the last stage of acceleration for outgoing solar wind, for ten points, identify this outer layer of the solar atmposhere.
The imaging and understanding of certain events in this region is the goal of NASA's STEREO mission, whose rotation was measured by the LASCO instrument and by Waldmeier using its namesake green line which arises from a transition in iron. Divided into the K, F, and E components, this region manifests areas of low x-ray emission known as its namesake "holes," which were discovered by SkyLab. The OSO-7 instrument first detected the namesake mass ejections emanating from this region, which extends about 13 million kilometers from the photosphere. Consisting of a plasma that is the last stage of acceleration for outgoing solar wind, for ten points, identify this outer layer of the solar atmposhere.
The imaging and understanding of certain events in this region is the goal of NASA's STEREO mission, whose rotation was measured by the LASCO instrument and by Waldmeier using its namesake green line which arises from a transition in iron.
corona