On the inability of magnetically constricted transition regions to account for the 105 to 106 K plasma in the quiet solar atmosphere
- 1 September 1987
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 112 (2) , 255-279
- https://doi.org/10.1007/bf00148781
Abstract
No abstract availableKeywords
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