On VI Emission Line Detection Limit of Far-Ultraviolet Imaging Spectrograph
There have been a few attempts to measure diffuse line emission between 900 //A and 1200 //A, and only in a limited number of sight lines has it been detected. The main contributions to the equilibrium radiative cooling curve between 10^4.5 K to 10^6 K are from the doublet of O VI 1032 and 1038 in t...
I tiakina i:
| Ngā kaituhi matua: | , , , , , , , , , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
The Korean Space Science Society
2000-06-01
|
| Rangatū: | Journal of Astronomy and Space Sciences |
| Urunga tuihono: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v17n1_77.pdf |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
|