Are the brightest coronal loops always rooted in mixed-polarity magnetic flux?

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    W[2019AGUFMSH41F3324E]
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    LI["Linked Institutions (3)"]
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ADS bibcode
2019AGUFMSH41F3324E
year
2019
Listed Authors
Evans, C.
Tiwari, S. K.
Panesar, N. K.
Prasad, A.
Moore, R. L.
Listed Institutions
Organization Not Listed, Washington, DC, United States
Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States
Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
University of Alabama in Huntsville, Huntsville, United States
NASA MSFC, Huntsville, AL, United States

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