Loading...
Please wait, while we are loading the content...
Similar Documents
Transport of cosmic rays in the solar corona
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Schatten, K. H. |
| Copyright Year | 1972 |
| Description | A method by which energetic cosmic ray particles in the interplanetary medium can diffuse in solar longitude. The method consists of particle motion occurring along current sheets separating discontinuous field structures in the corona. These sheets can serve as pathways along which energetic particles drift at nearly their propagation speed. A model of the coronal magnetic field and the large scale field behavior are analyzed. A mechanism by which particles can travel across the coronal magnetic field and arrive at the earth is suggested. |
| File Size | 161760 |
| Page Count | 5 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19720026154 |
| Archival Resource Key | ark:/13960/t7tn2076h |
| Language | English |
| Publisher Date | 1972-06-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Interplanetary Medium Solar Corona Current Sheets Particle Motion Diffusion Solar Magnetic Field Cosmic Rays Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |