Published 2009
| Version v1
Miscellaneous
The space weather modeling framework. Progress and challenges
Creators
- 1. Michigan University, Ann Arbor, MI (United States). Center for Space Environment Modeling
Description
Complete text of publication follows. The Space Weather Modeling Framework (SWMF) is a powerful tool for coupling regional models describing the space environment from the solar photosphere to the bottom of the ionosphere. Presently, SWMF contains 13 components: the solar corona (SC), eruptive event generator (EE), inner heliosphere (IE), outer heliosphere (OH), solar energetic particles (SE), global magnetosphere (GM), inner magnetosphere (IM), radiation belts (RB), plasmasphere (PS), ionospheric electrodynamics (IE), polar wind (PW), upper atmosphere (UA) and lower atmosphere (LA). This talk will present an overview of SWMF, new results obtained with improved physics (Hall MHD and multifluid MHD) as well as some validation studies.
Additional details
Identifiers
Publishing Information
- Publisher
- Geodetic and Geophysical Research Institute of the Hungarian Academy of Sciences
- Imprint Place
- Sopron (Hungary)
- Imprint Title
- International Association of Geomagnetism and Aeronomy IAGA 11. Scientific Assembly
- Imprint Pagination
- [1212 p.]
- Journal Page Range
- [1 p.]
- Report number
- INIS-HU--010
Conference
- Title
- International Association of Geomagnetism and Aeronomy IAGA 11. Scientific Assembly
- Dates
- 23-30 Aug 2009
- Place
- Sopron (Hungary)
INIS
- Country of Publication
- Hungary
- Country of Input or Organization
- Hungary
- INIS RN
- 41094801
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Non-conventional Literature
- Descriptors DEI
- EARTH MAGNETOSPHERE; HELIOSPHERE; IONOSPHERE; PHOTOSPHERE; PLASMASPHERE; RADIATION BELTS; SOLAR CORONA
- Descriptors DEC
- ATMOSPHERES; EARTH ATMOSPHERE; EARTH MAGNETOSPHERE; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE