Other
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21840501g&link_type=abstract
American Astronomical Society, AAS Meeting #218, #405.01; Bulletin of the American Astronomical Society, Vol. 43, 2011
Other
Scientific paper
Last year's launch of the Solar Dynamics Observatory (SDO) has provided additional data to constrain the temperature of coronal loops, allowing for a more detailed analysis of the nature of the heating. Specifically, the high temperature constraints that have been missing from prior analyses are now available to be considered. Images from a coronal loop on the solar disk on December 10, 2010 from both the Atmospheric Imaging Assembly (AIA) and the X-Ray Telescope (XRT) instruments onboard SDO are analyzed along with data from the same date taken by the Extreme Ultraviolet Imaging Spectrometer (EIS) instrument onboard Hinode. Differential emission measure techniques are used to consider whether the loops are isothermal or multithermal in nature. Conclusions regarding the comparison of this data will be presented.
Solar physics research at the University of Memphis is supported by NSF ATM-0402729 as well as a Hinode subcontract from NASA/SAO.
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