Numerical Heliospheric Simulation of Evolving Ambient Solar Wind and Interplanetary Magnetic Field

Details Numerical Heliospheric Simulation of Evolving Ambient Solar Wind and Interplanetary Magnetic Field Numerical Heliospheric Simulation of Evolving Ambient Solar Wind and Interplanetary Magnetic Field

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh13a..07o&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH13A-07

Physics

2134 Interplanetary Magnetic Fields, 2164 Solar Wind Plasma, 7843 Numerical Simulation Studies

Scientific paper

Recent advances in numerical methods and computer systems make it possible to tackle complicated, more realistic ambient and transient solar wind flows. Essential to this effort are the boundary conditions that drive 3-D MHD heliospheric models. We have used the improved source-surface model developed at NOAA/SEC Boulder [Arge et al., 2003, 2004] to derive solar wind parameters at 21.5 Rs. Various approaches and data sources are used and the numerical results obtained are compared with spacecraft observations at the Earth. Particular attention is given to the incorporation of daily updated source surface maps, which can be used to simulate an evolving ambient solar wind and interplanetary magnetic field.

Affiliated with

Also associated with

No associations

Rating

Numerical Heliospheric Simulation of Evolving Ambient Solar Wind and Interplanetary Magnetic Field 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 Heliospheric Simulation of Evolving Ambient Solar Wind and Interplanetary Magnetic Field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical Heliospheric Simulation of Evolving Ambient Solar Wind and Interplanetary Magnetic Field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1692921