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Mixed solar wind originating from coronal regions of different temperatures
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Bochsler, P. |
| Copyright Year | 1983 |
| Description | Ionization states of elements in the solar wind are often used to determine thermal gradients in the lower corona. This method is based on the assumption, that in the beginning, solar wind material has a homogeneous temperature determining the original charge state of elements. Features in M/Q-spectra which might appear if the above assumption is violated are investigated and compared with observational evidence. |
| File Size | 600770 |
| Page Count | 10 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19840005046 |
| Archival Resource Key | ark:/13960/t6159dx0z |
| Language | English |
| Publisher Date | 1983-11-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Ion Charge Solar Corona Ionization Silicon Helium Ions Magnesium Solar Wind Carbon Mass Spectra Metal Ions Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
