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Minor constituents in the solar wind originating from plasma-dust interactions
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Ripken, H. W. |
| Copyright Year | 1983 |
| Description | Atoms, molecules, and atomic and molecular ions generated by solar wind interactions with dust grains of the zodiacal cloud are discussed. The main processes leading to the generation of these particles are described and relevant methods of observation are examined. |
| File Size | 160558 |
| Page Count | 3 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19840005048 |
| Archival Resource Key | ark:/13960/t3dz53150 |
| Language | English |
| Publisher Date | 1983-11-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Zodiacal Dust Hydrogen Atoms Ions Mass Spectroscopy Plasma Interactions Helium Carbon Molecules Ion Charge Ionization Silicon Solar Wind Interplanetary Dust Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
