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To test a technique to be used on the white-light imager onboard the recently launched Parker Solar Probe mission, we performed a numerical differentiation of the brightness profiles along the photometric axis of the F-corona models that are derived from STEREO Ahead Sun Earth Connection Heliospheric Investigation observations recorded with the HI-1 instrument between 2007 December and 2014 March. We found a consistent pattern in the derivatives that can be observed from any S/C longitude between about 18\textdegree and 2 ...
Published by: The Astrophysical Journal Published on: 11/2018
YEAR: 2018   DOI: 10.3847/1538-4357/aae6cb
Published by: \apj Published on: 08/2018
YEAR: 2018   DOI: 10.3847/1538-4357/aacea3