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Re-examination of The Contribution Function by General Perturbation Method for the Observed Perturbation of Intensity
http://hdl.handle.net/10295/424
http://hdl.handle.net/10295/424d4a97654-a759-4bbe-88c3-f4fc37cdb5ad
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
KJ00000701557.pdf (3.9 MB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||||||
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| 公開日 | 2008-01-05 | |||||||||
| タイトル | ||||||||||
| タイトル | Re-examination of The Contribution Function by General Perturbation Method for the Observed Perturbation of Intensity | |||||||||
| 言語 | ||||||||||
| 言語 | eng | |||||||||
| 主題 | ||||||||||
| 主題Scheme | Other | |||||||||
| 主題 | line formation | |||||||||
| 主題 | ||||||||||
| 主題Scheme | Other | |||||||||
| 主題 | observed intensity | |||||||||
| 主題 | ||||||||||
| 主題Scheme | Other | |||||||||
| 主題 | contribution function | |||||||||
| 主題 | ||||||||||
| 主題Scheme | Other | |||||||||
| 主題 | perturbation method-gas cloud | |||||||||
| 主題 | ||||||||||
| 主題Scheme | Other | |||||||||
| 主題 | terrestrial atmosphere | |||||||||
| 主題 | ||||||||||
| 主題Scheme | Other | |||||||||
| 主題 | solar atmosphere | |||||||||
| 資源タイプ | ||||||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||||
| 資源タイプ | departmental bulletin paper | |||||||||
| 作成者 |
lto, Yutaka
× lto, Yutaka
× 伊藤, 胖
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| 内容記述 | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | We try to re-examine validity of our previously proposed Contribution Function (CFI) (Y.Ito,1988) from a view point of our Perturbation Method for observed Intensity I(O), (Y.Ito,1997), which was also previously proposed in order to get the exact and general solution of observed perturbation of intensity, δI(O). And, we examine the essential important problem, that is, integral of our Contribution Function (CFI) is not equal to observed Intensity I(O). We define new Contribution Function (CFII) that is contriution of perturbation at a layer (z) to observed perturbation of intensity, δI(O). So, integral of new Contribution Function (CFII) is capable of being not equal to observed Intensity I(O). Good point of new Contribution Function (CFII) is able to use, not only in the case of emission (for example, the case of solar atmosphere) but also in the case of no emission (for example, the case of gas cloud, the case of terrestrial atmosphere and so on). Many other Contribution Functions never can use in the case of no emission. | |||||||||
| 出版タイプ | ||||||||||
| 出版タイプ | VoR | |||||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||||
| 書誌情報 |
秋田大学教育文化学部 紀要 自然科学 巻 58, p. 55-69, 発行日 2003-03-31 |
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| ISSN | ||||||||||
| 収録物識別子タイプ | ISSN | |||||||||
| 収録物識別子 | 13485296 | |||||||||
| ISSN | ||||||||||
| 収録物識別子タイプ | ISSN | |||||||||
| 収録物識別子 | 03651649 | |||||||||
| NCID | ||||||||||
| 収録物識別子タイプ | NCID | |||||||||
| 収録物識別子 | AA11458582 | |||||||||
| 出版者 | ||||||||||
| 出版者 | 秋田大学教育文化学部 | |||||||||
