Ensemble Modeling of the Inner Heliosphere Using WSA-ENLIL and SWMF Models

Details Ensemble Modeling of the Inner Heliosphere Using WSA-ENLIL and SWMF Models Ensemble Modeling of the Inner Heliosphere Using WSA-ENLIL and SWMF Models

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh13b1533t&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH13B-1533

Astronomy and Astrophysics

Astrophysics

[7500] Solar Physics, Astrophysics, And Astronomy

Scientific paper

At the Community Coordinated Modeling Center we are developing the infrastructure to perform ensemble modeling of the background solar wind conditions at the L1 point using two models: 1) Wang-Sheeley-Arge solar corona + ENLIL inner heliosphere model combination, and 2) Space Weather Modeling Center solar corona and inner heliosphere model. As a solar input for both models we used the GONG observatory magnetograms for Carrington Rotations 2047-2074. We compared the models’ output for the solar wind parameters, such as speed, density, temperature and magnetic field magnitude at L1 point, with ACE observations. We also performed the "ensemble" modeling, by taking the average of the two models' output for each of the solar wind parameter.

Affiliated with

Also associated with

No associations

Rating

Ensemble Modeling of the Inner Heliosphere Using WSA-ENLIL and SWMF Models 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 Ensemble Modeling of the Inner Heliosphere Using WSA-ENLIL and SWMF Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ensemble Modeling of the Inner Heliosphere Using WSA-ENLIL and SWMF Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1781939