Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh51b2017o&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SH51B-2017
Physics
[2101] Interplanetary Physics / Coronal Mass Ejections, [2114] Interplanetary Physics / Energetic Particles, [2139] Interplanetary Physics / Interplanetary Shocks, [7959] Space Weather / Models
Scientific paper
At least 11 coronal mass ejections (CMEs) were observed by coronagraphs onboard SOHO and STEREO spacecraft in August 2010. These events generated a complex scenario of mutually interacting heliospheric disturbances and caused large geomagnetic storms and solar energetic particle (SEP) events. We use the WSA-ENLIL-CONE-SEPMOD modeling system to show the global solution in the inner heliosphere as it evolves during the whole month. Further we trace individual CMEs and compare their basic parameters with multi-spacecraft in-situ solar wind measurements and with remote white-light observations. Finally we detect interplanetary shock parameters, extract solar wind parameters along interplanetary magnetic field lines connecting the observer with the interplanetary shock, and simulate energy spectra of SEP. This example provides an update on one modeling capability with potential applications to both future event studies and space weather forecasting.
Luhmann Janet G.
MacNeice Peter J.
Odstrcil Dusan
Pulkkinen Aappo
Taktakishvili A.
No associations
LandOfFree
Numerical simulation of CMEs and SEPs in the inner heliosphere in August 2010 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Numerical simulation of CMEs and SEPs in the inner heliosphere in August 2010, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical simulation of CMEs and SEPs in the inner heliosphere in August 2010 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-881009