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The relative abundance of 3he(++) in the solar wind
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Geiss, J. Coplan, M. A. Bochsler, P. Ogilvie, K. W. |
| Copyright Year | 1983 |
| Description | Continuous measurements of solar wind 3He(++) and 4He(++) were made covering a full range of solar wind conditions. The average flux ratio derived from these data is 2310 + or - 50, in excellent agreement with the Apollo foil measurements. A probable correlation between average flux ratio and solar activity was found; however, an examination of the data during periods of 3He(++)-rich solar flares shows no detectable increase in 3He(++) in the solar wind. |
| File Size | 289966 |
| Page Count | 6 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19840005043 |
| Archival Resource Key | ark:/13960/t9x10xq7z |
| Language | English |
| Publisher Date | 1983-11-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Ion Concentration Solar Flares Transit Time Flux Density Helium Isotopes Solar Activity Effects Helium Ions Solar Wind Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
