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Interpretation of solar wind composition measurements from ulysses
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Esser, Ruth |
| Copyright Year | 1999 |
| Description | Ion charge states measured in situ in interplanetary space carry information on the properties of the solar wind plasma in the inner corona. This information is, however, not easy to extract from the in situ observations. The goal of the proposal was to determine solar wind models and coronal observations that are necessary tools for the interpretation of charge state observations. It has been shown that the interpretation of the in situ ion fractions are heavily dependent on the assumptions about conditions in the inner corona. |
| File Size | 328271 |
| Page Count | 8 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19990014460 |
| Archival Resource Key | ark:/13960/t9576c35t |
| Language | English |
| Publisher Date | 1999-01-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics In Situ Measurement Ion Charge Solar Corona Ulysses Mission Electron Density Concentration Ions Flow Velocity Charged Particles Solar Wind Solar Wind Velocity Interplanetary Space Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
