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Latitudinal properties of the solar wind from studies of ionic comet tails. [statistical analysis of solar wind speed variations
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Brandt, J. C. |
| Copyright Year | 1976 |
| Description | A statistical analysis is presented of the orientations of ionic comet tails in the solar wind. The analysis indicates that the radial solar wind speed is not necessarily higher near the solar poles than near the equator. The results refer to a long-term, global flow pattern and do not refer to short-term variations of solar wind speed. |
| File Size | 211381 |
| Page Count | 13 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19760017038 |
| Archival Resource Key | ark:/13960/t6wx25n43 |
| Language | English |
| Publisher Date | 1976-03-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Comets Root-mean-square Errors Solar Activity Statistical Analysis Polar Coordinates Variations Latitude Sampling Solar Cycles Solar Wind Velocity Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |