Micro- and meso-scale simulations of magnetospheric processes related to the aurora and substorm morphology. Final technical report, June 1989-November 1991
Abstract
The primary methodology during the grant period has been the use of micro or meso-scale simulations to address specific questions concerning magnetospheric processes related to the aurora and substorm morphology. This approach, while useful in providing some answers, has its limitations. Many of the problems relating to the magnetosphere are inherently global and kinetic. Effort during the last year of the grant period has increasingly focused on development of a global-scale hybrid code to model the entire, coupled magnetosheath - magnetosphere - ionosphere system. In particular, numerical procedures for curvilinear coordinate generation and exactly conservative differencing schemes for hybrid codes in curvilinear coordinates have been developed. The new computer algorithms and the massively parallel computer architectures now make this global code a feasible proposition. Support provided by this project has played an important role in laying the groundwork for the eventual development or a global-scale code to model and forecast magnetospheric weather.
- Authors:
- Publication Date:
- Research Org.:
- Alaska Univ., Fairbanks, AK (United States)
- OSTI Identifier:
- 5288793
- Report Number(s):
- N-94-17527; NASA-CR-193437; NAS-1.26:193437
CNN: NAGW-1787
- Resource Type:
- Technical Report
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; AURORAE; COMPUTERIZED SIMULATION; MAGNETIC STORMS; EARTH MAGNETOSPHERE; IONOSPHERE; MAGNETOSHEATH; PROGRESS REPORT; DOCUMENT TYPES; EARTH ATMOSPHERE; PLANETARY IONOSPHERES; SIMULATION; 661320* - Auroral, Ionospheric, & Magnetospheric Phenomena- (1992-)
Citation Formats
Swift, D W. Micro- and meso-scale simulations of magnetospheric processes related to the aurora and substorm morphology. Final technical report, June 1989-November 1991. United States: N. p., 1991.
Web.
Swift, D W. Micro- and meso-scale simulations of magnetospheric processes related to the aurora and substorm morphology. Final technical report, June 1989-November 1991. United States.
Swift, D W. 1991.
"Micro- and meso-scale simulations of magnetospheric processes related to the aurora and substorm morphology. Final technical report, June 1989-November 1991". United States.
@article{osti_5288793,
title = {Micro- and meso-scale simulations of magnetospheric processes related to the aurora and substorm morphology. Final technical report, June 1989-November 1991},
author = {Swift, D W},
abstractNote = {The primary methodology during the grant period has been the use of micro or meso-scale simulations to address specific questions concerning magnetospheric processes related to the aurora and substorm morphology. This approach, while useful in providing some answers, has its limitations. Many of the problems relating to the magnetosphere are inherently global and kinetic. Effort during the last year of the grant period has increasingly focused on development of a global-scale hybrid code to model the entire, coupled magnetosheath - magnetosphere - ionosphere system. In particular, numerical procedures for curvilinear coordinate generation and exactly conservative differencing schemes for hybrid codes in curvilinear coordinates have been developed. The new computer algorithms and the massively parallel computer architectures now make this global code a feasible proposition. Support provided by this project has played an important role in laying the groundwork for the eventual development or a global-scale code to model and forecast magnetospheric weather.},
doi = {},
url = {https://www.osti.gov/biblio/5288793},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Tue Jan 01 00:00:00 EST 1991},
month = {Tue Jan 01 00:00:00 EST 1991}
}