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The Detection of the motion of radio meteor reflection point of Geminids by HRO
https://nagano-nct.repo.nii.ac.jp/records/251
https://nagano-nct.repo.nii.ac.jp/records/25199602b2e-a58b-4fd6-8540-ae31d970bc9d
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
nagano_nct-35-15.pdf (1.3 MB)
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| Item type | Departmental Bulletin Paper(1) | |||||
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| 公開日 | 2013-02-19 | |||||
| タイトル | ||||||
| タイトル | The Detection of the motion of radio meteor reflection point of Geminids by HRO | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| キーワード | ||||||
| 言語 | en | |||||
| 主題Scheme | Other | |||||
| 主題 | meteor | |||||
| キーワード | ||||||
| 言語 | en | |||||
| 主題Scheme | Other | |||||
| 主題 | Geminids | |||||
| キーワード | ||||||
| 言語 | en | |||||
| 主題Scheme | Other | |||||
| 主題 | HRO | |||||
| 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 | |||||
| 著者 |
OHNISHI, Kouji
× OHNISHI, Kouji× ISHIKAWA, Toshiyuki× HATTORI, Shinobu× NISHIMURA, Osamu× MIYAZAWA, Akiko× YANAGISAWA, Masatoshi× ENDO, Makoto× KAWAMURA, Masaki× MARUYAMA, Toshiyuki× HOSAYAMA, Kai× TOKUNAGA, Mai× MAEGAWA, Kimio× ABE, Shinsuke |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | Ham-band Radio Observation (HRO) is one of the observational techniques for the forward scatter observation of meteors. We observe the meteor echo with two-element loop antennas (F/B ratio is 10 dB) at the Nagano National College of Technology (Nagano, JAPAN) using the continuous transmission of beacon signals for meteor observations at 53.750MHz, 50W from Fukui National College of Technology (Fukui, JAPAN). To prove that the radio echo is really the echo due to meteor, we construct the Direction Determination System using the paired antennas that can detect the direction roughly where the radio echo come from. The direction of one of this paired antennas was West toward Sabae and the other was East which has proved to be the most sensitive for this research. Using this system, we detected the change of the direction of reflection point of meteor radio signal of Geminids in 2000; from the westward to eastward before and after the culmination of the radiant which is consistent the formula of reflection point of meteors. At the same time, we detected the change of an intensity and a trend of the Doppler shift of meteor echoes. This result is consistent of the meteor wind data of MU Rader of Radio Science Center for Space & Atmosphere (RASC), Kyoto University. | |||||
| 書誌情報 |
長野工業高等専門学校紀要 巻 35, p. 93-100, 発行日 2001-12-27 |
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| 出版者 | ||||||
| 出版者 | 長野工業高等専門学校 | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 0286-1909 | |||||
| 書誌レコードID | ||||||
| 収録物識別子タイプ | NCID | |||||
| 収録物識別子 | AN00179170 | |||||
| フォーマット | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | application | |||||
| 著者版フラグ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
