The X ray corona, the coronal hole, and the heliosphere
β Scribed by Parker, E. N.
- Book ID
- 119685935
- Publisher
- American Geophysical Union
- Year
- 1992
- Tongue
- English
- Weight
- 687 KB
- Volume
- 97
- Category
- Article
- ISSN
- 0148-0227
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Radio cool regions observed on strip scans of the Sun made at 2800 MHz with a 1.5 rnin arc fan beam are associated with X-ray coronal holes and are used to derive lower envelopes which are similar to spotless Sun drift curves. Fluxes are evaluated from the Ottawa-ARO solar patrol;.e.g, that of Coron
It is shown that coronal holes may be used as indicators to trace the location of the neutral line on the source surface in the corona. At the same time, coronal holes are shown to concentrate in regions of enhanced magnetic field at the source surface. This provides us with a simple method for pred