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Mars Under Primordial Solar Wind Conditions: Mars Express Observations of the Strongest CME Detected at Mars Under Solar Cycle #24 and its Impact on Atmospheric Ion Escape
Author(s) -
Ramstad Robin,
Barabash Stas,
Futaana Yoshifumi,
Yamauchi Masatoshi,
Nilsson Hans,
Holmström Mats
Publication year - 2017
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2017gl075446
Subject(s) - mars exploration program , coronal mass ejection , solar wind , physics , polar wind , solar cycle , atmospheric sciences , solar maximum , solar cycle 22 , ionosphere , atmospheric escape , flux (metallurgy) , astrobiology , astronomy , plasma , quantum mechanics , materials science , metallurgy
An extremely strong Coronal Mass Ejection (CME) impacted Mars on 12 July 2011, while the Mars Express spacecraft was present inside the nightside ionosphere. Estimated solar wind density and speed during the event are 39 particles cm −3 and 730 km/s, corresponding to nominal solar wind flux at Mars when the solar system was ∼1.1 Ga old. Comparing with expected average atmospheric heavy ion fluxes under similar XUV conditions, the CME impact is found to have no significant effect on the escape rate 3.3 × 10 24 s −1 , with an upper limit at 10 25 s −1 if the observed tail contraction is not taken into account. On the subsequent orbit, 7 h later after magnetosphere response, fluxes were only 2.4% of average. As such, even under primordial solar wind conditions we are unable to find support for a strong solar wind‐driven ion escape, rather the main effect appears to be acceleration of the escaping ions by ×10–×20 typical characteristic energy.