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This opportunity concerns the modeling of the different aspects of the energy storageand dissipation in the outer solar atmosphere and wind, to be addressed via analyticalmodeling and/or numerical simulations, at either the large, MHD scales, or the smallerkinetic scales involving non-linear wave-particle interactions.
References:Rappazzo, F., Velli, M., Einaudi, G. and Dahlburg, R., (2008) Astrophys. J. 677, 1348,Nonlinear Dynamics of the Parker Scenario for Coronal Heating.Verdini, A. and Velli, M. (2007) Astrophys J. 662, P 669, Alfven Waves and Turbulence in theSolar Atmosphere and Solar Wind
Location:
Jet Propulsion Laboratory
Pasadena, California
Field of Science:Heliophysics Science
Advisors:
Marco Velli
Marco.C.Velli@jpl.nasa.gov
818-354-4369
Applications with citizens from Designated Countries will not be accepted at this time, unless they are Legal Permanent Residents of the United States. A complete list of Designated Countries can be found at: https://www.nasa.gov/oiir/export-control.
Eligibility is currently open to:
Full Time
$52k-65k (estimate)
09/26/2023
07/08/2024
ssc.nasa.gov
Stennis Space Center, MS
100 - 200