The kinematics of solar inner coronal transients

Solar Physics

Volumn 89, Issue 1, 1983, Pages 89-102

  MacQueen, R M ^a   Fisher, R R ^a  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33751515901     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/BF00211955     Document Type: Article

References (26)

1. Coronal activity below 2 solar radii - 1980 February 15-17
2. On the coronal transient-eruptive prominence of 1980 August 5
3. Mass ejections from the Sun: A view from Skylab
4. Abrupt Depletions of the Inner Corona
5. Conductive solar wind models in rapidly diverging flow geometries
6. Studies of the corona with the Solar Maximum Mission coronagraph/polarimeter
7. The observation of a coronal transient directed at earth
8. Energy addition in the solar wind
9. Eruptive solar magnetic fields
10. The initiation of a coronal transient
11. The Outer Solar Corona as Observed from Skylab: Preliminary Results
12. Expansion and broadening of coronal loop transients - A theoretical explanation
13. Physical properties of a polar coronal hole from 2 to 5 solar radii
14. Dynamical Properties of Stellar Coronas and Stellar Winds. I. Integration of the Momentum Equation.
15. Initial observations with the SOLWIND coronagraph
16. Magnetohydrodynamics of atmospheric transients. IV - Nonplane two-dimensional analyses of energy conversion and magnetic field evolution