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Space Weather Storm Responses at Mars: Lessons from A Weakly Magnetized Terrestrial Planet

Published online by Cambridge University Press:  12 September 2017

J. G. Luhmann ,
C. F. Dong ,
Y. J. Ma ,
S. M. Curry ,
Yan Li ,
C. O. Lee ,
T. Hara ,
R. Lillis ,
J. Halekas  and
J. E. Connerney
...Show all authors
J. G. Luhmann
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA, email: [email protected]
C. F. Dong
Affiliation:
Princeton University, Princeton, NJ, USA
Y. J. Ma
Affiliation:
Princeton University, Princeton, NJ, USA
S. M. Curry
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA, email: [email protected]
Yan Li
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA, email: [email protected]
C. O. Lee
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA, email: [email protected]
T. Hara
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA, email: [email protected]
R. Lillis
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA, email: [email protected]
J. Halekas
Affiliation:
University of Iowa, Iowa City, IA, USA
J. E. Connerney
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD, USA
J. Espley
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD, USA
D. A. Brain
Affiliation:
LASP, University of Colorado, Boulder, CO, USA
Y. Dong
Affiliation:
LASP, University of Colorado, Boulder, CO, USA
B. M. Jakosky
Affiliation:
LASP, University of Colorado, Boulder, CO, USA
E. Thiemann
Affiliation:
LASP, University of Colorado, Boulder, CO, USA
F. Eparvier
Affiliation:
LASP, University of Colorado, Boulder, CO, USA
F. Leblanc
Affiliation:
LATMOS/IPSL, UPMC University Paris, Paris, France
P. Withers
Affiliation:
Boston University, Boston, MA, USA
C. T. Russell
Affiliation:
Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, USA
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Abstract

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Much can be learned from terrestrial planets that appear to have had the potential to be habitable, but failed to realize that potential. Mars shows evidence of a once hospitable surface environment. The reasons for its current state, and in particular its thin atmosphere and dry surface, are of great interest for what they can tell us about habitable zone planet outcomes. A main goal of the MAVEN mission is to observe Mars’ atmosphere responses to solar and space weather influences, and in particular atmosphere escape related to space weather ‘storms’ caused by interplanetary coronal mass ejections (ICMEs). Numerical experiments with a data-validated MHD model suggest how the effects of an observed moderately strong ICME compare to what happens during a more extreme event. The results suggest the kinds of solar and space weather conditions that can have evolutionary importance at a planet like Mars.

Keywords

MarsMagnetosphereMagnetic Storm
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S328: Living Around Active Stars , October 2016 , pp. 211 - 217
Copyright
Copyright © International Astronomical Union 2017 

References

Acuna, M. H. et al., Global distribution of crustal magnetization discovered by the Mars Global Surveyor, 1999, Science, 284, 790–793 CrossRefGoogle ScholarPubMed
Airapetian, V. S. & Usmanov, A. V. Reconstructing the solar wind from its early history to current epoch, 2016, ApJ, 817, L24–L30 Google Scholar
Curry, S.M., et al., Response of Mars O+ pickup ions to the 8 March 2015 ICME: Inferences from MAVEN data-based models, 2015, Geophys. Res. Lett., 42, 9095–9102 Google Scholar
Dong, C. F., et al., 2015, Multifluid MHD study of the solar wind interaction with Mars’ upper atmosphere during the 2015 March 8 th ICME event 2015, Geophys. Res. Lett., 42, 9103–9112 Google Scholar
Edberg, N. J. T., Nilsson, H., Williams, A. O., Lester, M., Milan, S. E., Cowley, S. W. H., Fraenz, M., Barabash, S., & Futaana, Y., Pumping out the atmosphere of Mars through solar wind pressure pulses 2010, Geophys. Res. Lett., 37 Google Scholar
Guedel, et al., this volume Google Scholar
Jakosky, B. & Phillips, R., Mars’ volatile and climate history, 2001, Nature, 412, 237–244 CrossRefGoogle ScholarPubMed
Jakosky, B. M. et al., 2015a, The Mars atmosphere and volatile evolution (MAVEN) mission 2015a, Space Sci. Rev., 195 Google Scholar
Jakosky, B. M. et al., 2015b, MAVEN observations of the response of Mars to an interplanetary coronal mass ejection 2015b, Science, 350 CrossRefGoogle Scholar
Jakosky, B. M., Grebowsky, J. M., Luhmann, J. G., & Brain, D. A., The MAVEN mission to Mars at the end of one Mars year of science observations, 2016, J. Geophys. Res., pressGoogle Scholar
Lillis, R. et al., Characterizing atmospheric escape from Mars today and through time, 2015, Space Sci. Rev., 195, 357–422 CrossRefGoogle Scholar
Luhmann, J. G., Dong, C. F., Ma, Y. J., Curry, S. M., Xu, S., Lee, C. O., Hara, T., Halekas, J., & Li, Yan, Gruesbeck, J. R., Espley, J., Brain, D. A., & Russell, C. T., 2016, Martian magnetic storms 2016, submitted to J. Geophys. Res. Google Scholar
Lundin, R., Barabash, S., Homstrom, M., Nillson, H., Futaana, Y., Ramstad, R., Yamauchi, M., Dubinin, E., & Fraenz, M., Solar cycle effects on the ion escape from Mars, 2013, Geophys. Res. Lett., 40, 6028–6032 CrossRefGoogle Scholar
Ma, Y. J., et al., MHD model results of solar wind interaction with Mars and comparison with MAVEN plasma observations, 2015, Geophys. Res. Lett., 42, 9113–9120 CrossRefGoogle Scholar
Maehara, , H., Shibayama, T., Notsu, S., Notsu, Y., Nagao, T., Kusaba, S., Honda, S., Nogami, D., & Shibata, K., Superflares on solar-type stars, 2012, Nature, 485, 478–481 Google Scholar
Osten, et al., this volume Google Scholar
Ribas, L., Guinan, E. F., Guedel, M., &, Audard, M., Evolution of the Solar Activity over Timeand Effects on Planetary Atmospheres. I. High-Energy Irradiances (1-1700 +), 2005, ApJ, 622, 680–694 Google Scholar
Terada, N., Kulikov, Y. N., Lammer, H., Lichtenegger, H., Tanaka, T., Shinagawa, H., & Zhang, T., Atmosphere and water loss from early Mars under extreme solar windand extreme ultraviolet conditions, 2009, Astrobiology, 9, 55–70 Google Scholar
Thiemann, E. M., et al., Neutral density response to solar flares at Mars, 2015, Geophys. Res. Lett., 42, 8986–8992 CrossRefGoogle Scholar
Tu, L., Johnstone, C. P., Guedel, M., & Lammer, H., The Extreme Ultraviolet and X-Ray Sun in Time: High-Energy Evolutionary Tracks of a Solar-Like Star 2015, Astronomy and Astrophysics, 577 Google Scholar
Wood, B. E., The Solar Wind and the Sun in the Past, 2006, Space Sci. Rev., 126, 3–14 Google Scholar