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A discussion of interplanetary post-shock flows with two examples. [with plasma and magnetometer observations
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Burlaga, L. F. Ogilvie, K. W. |
| Copyright Year | 1974 |
| Description | Plasma and magnetometer observations are described for two flare-associated shock flows and the comparison of them with models. One represents a class of flows where the shock is followed by a stream and separated from it by a region in which density temperature and speed decrease monotonically. The other is characterized by a complex region between the shock and the following stream, which has many discontinuities and fluctuations, but in which there is no increase in helium concentration. These two types of flow can be distinguished using ground magnetograms, since the former shows no sudden impulses following the shock, whereas the latter shows many. |
| File Size | 647515 |
| Page Count | 29 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19740011311 |
| Archival Resource Key | ark:/13960/t9f52fd2h |
| Language | English |
| Publisher Date | 1974-01-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Interplanetary Medium Shock Waves Models Magnetometers Plasma Diagnostics Helium Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |