Anticipating the Geoeffectiveness of Coronal Mass Ejections

Award Information
Agency:
National Aeronautics and Space Administration
Branch
n/a
Amount:
$124,951.00
Award Year:
2012
Program:
SBIR
Phase:
Phase I
Contract:
NNX12CE25P
Award Id:
n/a
Agency Tracking Number:
114896
Solicitation Year:
2011
Solicitation Topic Code:
S1.06
Solicitation Number:
n/a
Small Business Information
9990 Mesa Rim Road, Suite 170, San Diego, CA, 92121-3933
Hubzone Owned:
N
Minority Owned:
N
Woman Owned:
N
Duns:
824866045
Principal Investigator:
Jon Linker
Principal Investigator
(858) 450-6489
linkerj@predsci.com
Business Contact:
Irene Caguinguin
Business Official
(858) 450-6494
irene@predsci.com
Research Institute:
Stub




Abstract
Coronal Mass Ejections (CMEs) are responsible for some of the most severe space weather at Earth. Major geomagnetic storms arise when CMEs carry large amounts of magnetic flux as they propagate in the solar wind. If these magnetic fields have a southward orientation (oppositely directed to the magnetic field at the Earth's magnetopause), they can cause a geomagnetic storm. Predicting in advance whether observed CMEs will carry geoeffective magnetic fields is a long-term priority for the CCMC at NASA GFSC and other groups within NASA as well. We propose to combine the existing CORHEL (Corona-Heliosphere) model of the solar corona and solar wind with a robust technique for generating simulated CMEs. When successfully completed, the new tool, CORHEL-CG, will allow routine simulation of CMEs and represent a leap forward in physics-based space weather prediction models.

* information listed above is at the time of submission.

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