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Solar wind disturbances in th outer heliosphere caused by successive solar flares from the same active region
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Hakamada, K. Akasofu, S. I. |
| Copyright Year | 1983 |
| Description | Solar wind disturbances caused by successive flares from the same active region are traced to about 20 AU, using the modeling method developed by Hakamada and Akasofu (1982). It is shown that the flare-generated shock waves coalesce with the co-rotating interaction region of the interplanetary magnetic field, resulting in a large-scale magnetic field structure in the outer heliosphere. Such a structure may have considerable effects on the propagation of galactic cosmic rays. |
| File Size | 809540 |
| Page Count | 10 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19840005036 |
| Archival Resource Key | ark:/13960/t1hj1c10m |
| Language | English |
| Publisher Date | 1983-11-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Heliosphere Magnetohydrodynamics Solar Flares Solar Activity Effects Mathematical Models Solar Wind Cosmic Rays Interplanetary Magnetic Fields Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
