Long-lived coronal structures and recurrent geomagnetic patterns in 1974

Planetary and Space Science

Volumn 24, Issue 4, 1976, Pages 381-388

  Hansen, Richard T ^a   Hansen, Shirley F ^a   Sawyer, Constance ^b  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^b NOAA Fisheries   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000152255     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/0032-0633(76)90051-9     Document Type: Article

References (28)

1. Relation between magnetic storms and solar activity
2. M-regions
3. Coronal holes
4. Terrestrial magnetic activity and its relations to solar phenomena
5. Intensity of the Fe XV emission line corona, the level of geomagnetic activity, and the velocity of the solar wind
6. The origin of M-region geomagnetic storms
7. Solar coronal streamers. I. Observed locations, general evolution and classification
8. Solar coronal streamers. II. Evolution of discrete features from the sun to 1 A. U
9. Coronal disturbances. I. Fast transient events observed in the green coronal emission line during the last solar cycle
10. Coronal events observed in 5303 Å
11. Mass ejections from the sun A view from Skylab
12. Interplanetary disturbances: A classification
13. Coronal λ5303 intensity, geomagnetic activity and solar sources of high speed plasma streams
14. K-coronal enhancements and chromospheric plages
15. Abrupt depletions of the inner corona
16. Evolution of coronal helmets during the ascending phase of solar cycle 20
17. Observation of sectored structure in the outer solar corona: Correlation with interplanetary magnetic field
18. A coronal hole and its identification as the source of a high velocity solar wind stream
19. X-ray observations of coronal holes and their relation to high velocity solar wind streams
20. Properties of a coronal “hole” derived from extreme-ultraviolet observations
21. Solar coronal holes as sources of recurrent geomagnetic disturbances
22. Solar corpuscles responsible for geomagnetic disturbances
23. The solar wind and the temperature-density structure of the solar corona
24. A model combining the polar and the sector structured solar magnetic fields
25. The structure and evolution of coronal holes
26. Identification analysis of structures in the corona from X-ray photography