Discovery of a loop-top hard X-ray source in impulsive solar flares

Advances in Space Research

Volumn 17, Issue 4-5, 1996, Pages 63-66

  Masuda, S ^a   Kosugi, T ^b   Tsuneta, S ^c   Hara, H ^b  

^a NAGOYA UNIVERSITY   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0012914644     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00543-N     Document Type: Article

References (14)

1. The Hard X-ray Telescope (HXT) for the Solar-A mission
2. The Soft X-ray Telescope for the Solar-A mission
3. The Solar-A mission: an overview
4. Observation of a solar flare at the limb with the Yohkoh Soft X-ray Telescope
5. Solar flares as onging magnetic reconnection
6. A model of solar flares
7. Theoritical model of solar flares and prominences I: evaporating flare model
8. Magnetic reconnection in the corona and the loop prominence phenomenon
9. Hard X-ray imaging of two flares in active region 2372
10. X-ray imaging of three flares during the impulsive phase
11. Hard X-ray imaging observations of footpoint sources in impulsive solar flares
12. A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection
13. The deduction of energy spectra of non-thermal electrons in flares from the observed dynamic spectra of hard X-ray bursts
14. Indirect estimation of energy disposition by non-thermal electrons in solar flares