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Please use this identifier to cite or link to this item: http://hdl.handle.net/2014/40912

Title: A Chapman -layers ionspheric model for Mars.
Authors: Pi, Xiaoqing
Edwards, Charles D.
Hajj, George A.
Ao, Chi
Romans, Larry J.
Callas, John L.
Mannucci, Anthony J.
Asmar, Sami W.
Kahan, Daniel S.
Keywords: solar extreme ultraviolet (EUV)
radiation cycles
solar zenith angle
Issue Date: Aug-2008
Publisher: Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2008.
Series/Report no.: JPL Publication
08-24
Abstract: A numerical model (CLIMM) is developed that adopts functions of two Chapman layers to compute Mars ionospheric electron densities at given local solar zenith angle and height. Electron density profiles derived from Mars Global Survey (MGS)-to-Earth radio occultation measurements collected during 1998 through 2005 are used to fit the model. The present model does not include variations with solar extreme ultraviolet (EUV) radiation cycles and seasons, and may have increased errors at lower latitudes. A more sophisticated model taking into account these variations is being developed and will be available in the future.
URI: http://hdl.handle.net/2014/40912
Appears in Collections:JPL TRS 1992+

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