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Abstract: Evidence of Mostly Steady Heating of the Cooler Coronal Plasma in a Solar Active Region (AGU25)

Evidence of Mostly Steady Heating of the Cooler Coronal Plasma in a Solar Active Region

Neela Pifer1, Sanjiv K. Tiwari2, Navdeep Panesar2 and Ronald Lee Moore3, (1)Pennsylvania State University University Park, Huntsville, Alabama, UNITED STATES, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, (3)NASA MSFC, Huntsville, United States