Data Assimilative Optimization of WSA Source Surface and Interface Radii using Particle Filtering

Author:

Meadors Grant David123ORCID,Jones Shaela I.45,Hickmann Kyle S.1,Arge Charles N.4,Godinez‐Vasquez Humberto C.2,Henney Carl J.6ORCID

Affiliation:

1. XCP‐Division, Verification & AnalysisLos Alamos National Laboratory Los Alamos NM USA

2. T‐Division, Applied Mathematics & Plasma PhysicsLos Alamos National Laboratory Los Alamos NM USA

3. A‐Division, Global SecurityLos Alamos National Laboratory Los Alamos NM USA

4. NASA Goddard Space Flight Center Greenbelt MD USA

5. Department of PhysicsCatholic University of America Washington DC USA

6. Air Force Research Laboratory, Space Vehicles Directorate Kirtland AFB NM USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference45 articles.

1. Magnetic fields and the structure of the solar corona

2. A “breathing” source surface for cycles 23 and 24

3. Air Force Data Assimilative Photospheric Flux Transport (ADAPT) model;Arge C. N.;Twelfth International Solar Wind Conference,2010

4. Arge C. N. Henney C. J. Koller J. Toussaint W. A. Harvey J. W. &Young S.(2011).Improving data drivers for coronal and solar wind models. In5th international conference of numerical modeling of space plasma flows (astronum 2010) (N. V.Pogorelov E.Audit &G. P.Zank  Eds.) Astronomical Society of the Pacific Conference Series 444 pp.99.

5. Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME

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