Heliospheric Streamers: Comparison Between Model Calculations and SECCHI Observations

Details Heliospheric Streamers: Comparison Between Model Calculations and SECCHI Observations Heliospheric Streamers: Comparison Between Model Calculations and SECCHI Observations

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh42a..04h&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH42A-04

Physics

2102 Corotating Streams, 7833 Mathematical And Numerical Techniques (0500, 3200)

Scientific paper

We have generated a time dependent 3-dimensional description of the electron density distribution out to 1 AU using the ENLIL model at the Community Coordinated Modeling Center (CCMC). Using this electron density description we have computed the brightness measurements that would be observed by coronagraphic instruments such as SECCHI using the Raytrace package. We compare the computed images with the actual SECCHI observations of streamers/heliospheric current sheet.

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