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The recovery of the cosmic ray flux from maximum solar modulation at imp-8 (1 au) and at pioneer (r 30 au)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Pyle, K. R. Simpson, J. A. McKibben, R. B. |
| Copyright Year | 1985 |
| Description | In the period 1980-84, observations of relativistic and low energy (30 E 70 MeV/n) cosmic ray nuclei from Pioneer 10 in the outer heliosphere and from IMP-8 at AU show that increases as well as decreases in intensity propagate outward at velocities equal to or greater than the average solar wind velocity. |
| File Size | 253345 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850026739 |
| Archival Resource Key | ark:/13960/t5jb11r45 |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Protons Heliosphere Solar Activity Explorer 50 Satellite Voyager 1 Spacecraft Propagation Velocity Energy Spectra Helium Voyager 2 Spacecraft Cosmic Rays Solar Wind Velocity Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
