A high-temperature component in coronal holes observed with Yohkoh SXT

Advances in Space Research

Volumn 17, Issue 4-5, 1996, Pages 231-234

  Hara, H ^a   Tsuneta, S ^b   Acton, L W ^c   Bruner, M E ^d   Lemen, J R ^d   Ogawara, Y ^e  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c MONTANA STATE UNIVERSITY   (United States)

^d LOCKHEED MARTIN   (United States)

^e JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0002387956     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00575-Y     Document Type: Article

References (13)

1. The coronal temperature and nonthermal motions in a coronal hole compared with other solar regions
2. Analysis of extreme-ultraviolet observations of a polar coronal hole
3. Determination of plasma parameters from soft X-ray images for coronal holes /open magnetic field configurations/ and coronal large-scale structures /extended closed-field configurations/
4. Properties of a Coronal "hole" Derived from Extreme-Ultraviolet Observations
5. The energy balance in coronal holes and average quiet-sun regions