Computer Science
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679...75j&link_type=abstract
SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 75-78
Computer Science
13
Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
We have developed a Computer Assisted Tomography (CAT) program that modifies a time-dependent three-dimensional kinematic heliospheric model to fit interplanetary scintillation (IPS) observations. The tomography program iteratively changes this global model to least-squares fit IPS data. The short time intervals of the kinematic modeling (~1 day) force the heliospheric reconstructions to depend on outward solar wind motion to give perspective views of each point in space accessible to the observations, allowing reconstruction of interplanetary Coronal Mass Ejections (CMEs) as well as corotating structures. We show these models as velocity or density Carrington maps and remote views. We have studied several events, including the July 14, 2000 Bastille-day halo CME. We check our results by comparison with additional remote-sensing observations, and observations from near-Earth spacecraft.
Buffington Andrew
Fujiki Ken'ichi
Hick Pierre P.
Jackson Bernard V.
Kojima Masamichi
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