Nishikawa, Takara (1983) Origin of the weakening of EUV emission lines formed in the chromosphere-corona transition zone. Solar Physics, 85 (1). 65-82 doi:10.1007/bf00148258
| Reference Type | Journal (article/letter/editorial) | ||
|---|---|---|---|
| Title | Origin of the weakening of EUV emission lines formed in the chromosphere-corona transition zone | ||
| Journal | Solar Physics | ||
| Authors | Nishikawa, Takara | Author | |
| Year | 1983 (May) | Volume | 85 |
| Issue | 1 | ||
| Publisher | Springer Science and Business Media LLC | ||
| DOI | doi:10.1007/bf00148258Search in ResearchGate | ||
| Generate Citation Formats | |||
| Mindat Ref. ID | 8917506 | Long-form Identifier | mindat:1:5:8917506:6 |
| GUID | 0 | ||
| Full Reference | Nishikawa, Takara (1983) Origin of the weakening of EUV emission lines formed in the chromosphere-corona transition zone. Solar Physics, 85 (1). 65-82 doi:10.1007/bf00148258 | ||
| Plain Text | Nishikawa, Takara (1983) Origin of the weakening of EUV emission lines formed in the chromosphere-corona transition zone. Solar Physics, 85 (1). 65-82 doi:10.1007/bf00148258 | ||
| In | (1983, May) Solar Physics Vol. 85 (1) Springer Science and Business Media LLC | ||
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