Spawning and Shedding Helical Magnetic Fields in the Solar Atmosphere

Geophysical Research Letters

Volumn 21, Issue 4, 1994, Pages 241-244

  Rust, D M ^a  

^a JOHNS HOPKINS UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 85005519683     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/94GL00003     Document Type: Article

References (28)

1. The topology of the Sun's magnetic field and the 22‐year cycle
2. Rigorous new limits on magnetic helicity dissipation in the solar corona
3. Magnetic loop behind an interplanetary shock: Voyager, Helios and IMP 8 observations
4. A statistical study of the spiral spots on the solar disc
5. An investigation of macroscopic motions using the Ca+ lines in the prominence of 15 October 1969
6. Coronal heating by reconnection in DC current systems, a theory based on Taylor's hypothesis
7. A map of the horizontal flows in the solar convection zone
8. A magneto‐kinematic model of the solar cycle
9. Magnetic field structure of interplanetary magnetic clouds at 1 AU
10. Magnetohydrostatic fields
11. Magnetic field configurations basic to filament channels and filaments
12. On the topology of filaments and chromospheric fibrils near sunspots
13. The formation of sunspots from the solar toroidal field
14. The nature of solar hydrogen vortices
15. Magnetic fields in quiescent solar prominences I. Observations
16. Electric current helicity in the solar atmosphere
17. Two‐dimensional inversion for solar internal rotation
18. Stability of prominences exposing helical‐like patterns
19. Are interplanetary magnetic clouds manifestations of coronal transients at 1 AU?
20. On the association of magnetic clouds with disappearing filaments