Medium resolution observations have been used to find the fractional emitting area c~ in three transition region lines. It is found that a is given by DI~kβ’ where k varies from 0.78 to 0.51 in the temperature range 2x 105 to 7 β’ 105 K. The average emitting area in O vl deduced by this method is in g
β¦ LIBER β¦
EUV observations of the chromospheric network
β Scribed by E. M. Reeves; W. H. Parkinson
- Book ID
- 104674425
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 576 KB
- Volume
- 24
- Category
- Article
- ISSN
- 0038-0938
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