Loading...
Please wait, while we are loading the content...
Similar Documents
Solar large-scale positive polarity magnetic fields and geomagnetic disturbances
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Bumba, V. |
| Copyright Year | 1972 |
| Description | Unlike the negative polarity solar magnetic field large-scale regular features that correlate with enhanced solar activity regions, the positive polarity regular formations formed in the weak and old background magnetic fields seem to correlate well with geomagnetically enhanced periods of time (shifted for 4 days), which means that they seem to be the source of the quiet solar wind. This behavior of the large intervals of heliographic longitude with prevailing positive polarity fields may be followed to the end of the 18th cycle, during the declining part of the 19th cycle, and during the first half of the present 20th cycle of solar activity. |
| File Size | 731714 |
| Page Count | 7 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19730002045 |
| Archival Resource Key | ark:/13960/t4nk84601 |
| Language | English |
| Publisher Date | 1972-01-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Magnetic Disturbances Magnetic Flux Polarity Solar Cycles Solar Magnetic Field Magnetic Properties Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
