Invisibility of Solar Active Region Umbra-to-Umbra Coronal Loops: New Evidence that Magnetoconvection Drives Solar-Stellar Coronal Heating

    flowchart
    W[2017AGUFMSH43A2789T]
    LA["Linked Authors (0)"]
    LI["Linked Institutions (3)"]
    W== author ==>LA
    W== affil ==>LI
    click LA "#linked-authors"
    click LI "#linked-institutions"
Graph neighborhood for 'Invisibility of Solar Active Region Umbra-to-Umbra Coronal Loops: New Evidence that Magnetoconvection Drives Solar-Stellar Coronal Heating'. Click aggregate nodes to navigate.
ADS bibcode
2017AGUFMSH43A2789T
year
2017
Listed Authors
Tiwari, S. K.
Thalmann, J. K.
Panesar, N. K.
Moore, R. L.
Winebarger, A. R.
Listed Institutions
Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States
Institute for Physics/IGAM, University of Graz, Graz, Austria
NASA Marshall Space Flight Center, Huntsville, AL, United States
NASA Marshall Space Flight Center, Huntsville, AL, United States; Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States
NASA Marshall Space Flight Center, Huntsville, AL, United States

Linked Authors [?]

Linked Institutions