Multipoint observations of coronal mass ejection and solar energetic particle events on Mars and Earth during November 2001

Details Multipoint observations of coronal mass ejection and solar energetic particle events on Mars and Earth during November 2001 Multipoint observations of coronal mass ejection and solar energetic particle events on Mars and Earth during November 2001

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jgra..11606104f&link_type=abstract

Journal of Geophysical Research, Volume 116, Issue A6, CiteID A06104

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Interplanetary Physics: Coronal Mass Ejections (4305, 7513), Computational Geophysics: Model Verification And Validation, Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Energetic Particles (7514), Planetary Sciences: Solar System Objects: Mars

Scientific paper

Multipoint spacecraft observations provide unique opportunities to constrain the propagation and evolution of interplanetary coronal mass ejections (ICMEs) throughout the heliosphere. Using Mars Global Surveyor (MGS) data to study both ICME and solar energetic particle (SEP) events at Mars and OMNI and Geostationary Operational Environmental Satellite (GOES) data to study ICMEs and SEPs at Earth, we present a detailed study of three CMEs and flares in late November 2001. In this period, Mars trailed Earth by 56° solar longitude so that the two planets occupied interplanetary magnetic field lines separated by only ˜25°. We model the interplanetary propagation of CME events using the ENLIL version 2.6 3-D MHD code coupled with the Wang-Sheeley-Arge version 1.6 potential source surface model, using Solar and Heliospheric Observatory (SOHO) Large Angle and Spectrometric Coronagraph (LASCO) images to determine CME input parameters. We find that multipoint observations are essential to constrain the simulations of ICME propagation, as two very different ICMEs may look very similar in only one observational location. The direction and width of the CME as parameters essential to a correct estimation of arrival time and amplitude of the ICME signal. We find that these are problematic to extract from the analysis of SOHO/LASCO images commonly used for input to ICME propagation models. We further confirm that MGS magnetometer and electron reflectometer data can be used to study not only ICME events but also SEP events at Mars, with good results providing a consistent picture of the events when combined with near-Earth data.

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