Solar terrestrial coupling through space plasma processes
Description
This is the final report of a three-year, Laboratory-Directed Research and Development (LDRD) project at the Los Alamos National Laboratory (LANL). The project investigates plasma processes that govern the interaction between the solar wind, charged particles ejected from the sun, and the earth's magnetosphere, the region above the ionosphere governed by the terrestrial magnetic field. Primary regions of interest are the regions where different plasma populations interact with each other. These are regions of particularly dynamic plasma behavior, associated with magnetic flux and energy transfer and dynamic energy release. The investigations concerned charged particle transport and energization, and microscopic and macroscopic instabilities in the magnetosphere and adjacent regions. The approaches combined space data analysis with theory and computer simulations
Availability note (English)
Available from INIS in electronic form; Also available from OSTI as DE00768901; PURL: https://www.osti.gov/servlets/purl/768901-IoAUvk/webviewable/
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Additional details
Identifiers
Publishing Information
- Imprint Pagination
- 31 p.
- Report number
- LA-UR--00-5748
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 32026383
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S58: GEOSCIENCES;
- Descriptors DEI
- CHARGED PARTICLES; CHARGED-PARTICLE TRANSPORT; DATA ANALYSIS; EARTH MAGNETOSPHERE; ENERGY TRANSFER; IONOSPHERE; MAGNETIC FIELDS; MAGNETIC FLUX; PLASMA; SOLAR WIND; SUN
- Descriptors DEC
- EARTH ATMOSPHERE; MAIN SEQUENCE STARS; RADIATION TRANSPORT; SOLAR ACTIVITY; STARS; STELLAR ACTIVITY; STELLAR WINDS
Optional Information
- Contract/Grant/Project number
- W-7405-ENG-36
- Funding organization
- US Department of Energy (United States)