A new mechanism of coronal heating

Space Science Reviews

Volumn 95, Issue 1-2, 2001, Pages 95-106

  Lee, L C ^a  

^a NATIONAL CHENG KUNG UNIVERSITY   (Taiwan)

Author keywords

[No Author keywords available]

Indexed keywords

ION; PROTON;

ATMOSPHERE; HEATING; MAGNETIC FIELD; RADIATION PHYSICS; REVIEW; SOLAR ENERGY; SOLAR RADIATION; SUN;

EID: 0035143714     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1005232332548     Document Type: Review

References (29)

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4. Evolution of solar magnetic arcades. II. Effect of resistivity and solar eruptive processes
5. An empirical model of a polar coronal hole at solar minimum
6. Spectroscopic constraints on models of ion cyclotron resonance heating in the polar solar corona and high-speed solar wind
7. Explosive events and magnetic reconnection in the solar atmosphere
8. Evidence for ion jets in the high-speed solar wind
9. α-particle observations in the solar wind
10. Coronal cass ejections: An overview
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12. Sizes and locations of coronal mass ejections - SMM observations from 1980 and 1984-1989
13. First results from the SOHO ultraviolet coronagraph spectrometer
14. Uvcs/Soho empirical determinations of anisotropic velocity distributions in the solar corona
15. Heating and acceleration of protons and minor ions by fast shocks in the solar corona
16. Increase of ion kinetic temperature across a collisionless shock: I. A new mechanism
17. Generation of rotational discontinuities by magnetic reconnection associated with microflares
18. Acceleration of the solar wind
19. Solar-wind models from the sun to 1 AU - Constraints by in-situ and remote-sensing measurements
20. The effects of high-frequency Alfvén waves on coronal heating and solar-wind acceleration
21. Solar wind helium ions: Observations of the helios solar probes between 0.3 and 1 AU
22. Chromospheric and coronal heating mechanisms 2
23. Ulysses observation of differential alpha-proton streaming in the solar wind
24. Solar-wind acceleration by aolitary waves in coronal holes
25. Differences between the bulk speeds of hydrogen and helium in the solar wind
26. Heating solar coronal holes
27. Rotational discontinuities and the structure of the magnetopause
28. Two-fluid model for heating of the solar corona and acceleration of the solar-wind by high-frequency Alfvén waves
29. Coronal heating