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The 2001 Leonid Multi-Instrument Aircraft Campaign - An early review
https://jaxa.repo.nii.ac.jp/records/36697
https://jaxa.repo.nii.ac.jp/records/36697de7de97a-d0ff-4e32-82b5-572d3f27780d
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
SA4636312.pdf (1.4 MB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| 公開日 | 2015-03-26 | |||||||||
| タイトル | ||||||||||
| タイトル | The 2001 Leonid Multi-Instrument Aircraft Campaign - An early review | |||||||||
| 言語 | en | |||||||||
| 言語 | ||||||||||
| 言語 | eng | |||||||||
| 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 |
Peter, JENNISKENS
× Peter, JENNISKENS
× Ray, W. RUSSELL
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| 著者所属（英） | ||||||||||
| en | ||||||||||
| SETI Institute | ||||||||||
| 著者所属（英） | ||||||||||
| en | ||||||||||
| The aerospace Corporation | ||||||||||
| 出版者 | ||||||||||
| 出版者 | 宇宙科学研究所 | |||||||||
| 出版者（英） | ||||||||||
| 出版者 | Institute of Space and Astronautical Science | |||||||||
| 書誌情報 |
en : The Institute of Space and Astronautical Science report. S.P. : Proceedings of the 2002 International Science Symposium on the Leonid Meteor Storms 巻 15, p. 3-15, 発行日 2003-03 |
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| 抄録（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | Following a successful deployment in 1999 and predictions of further Leonid stormsin 2001 and 2002, a new set of two airborne missions was prepared in the Leonid Multi-InstrumentAircraft Campaign. Geopolitical circumstances affected the scope of the 2001 mission more thanusual. The NKC-135 "FISTA" aircraft executed a CONUS single-plane deployment with 19 UScitizen researchers onboard out of Edwards AFB, CA. The researchers traveled to Alabama and,after 08:50 UT, slowly returned back to base on a westward trajectory at an altitude of 37,000ft. Non US citizen participants observed from various ground sites. The 1767-dust trail of comet55P/Tempel-Tuttle was well observed. Key results were: a) measurements of meteor flux todiscriminate among meteor storm prediction models; b) high resolution optical spectra that set astrong lower limit to the CN abundance in meteor plasma and measured plasma temperatures asa function of meteoroid mass; c) further mid-IR detections of meteors with simultaneous opticalimaging; d) HDTV recorded low-resolution optical spectra for studies of compositional anomalies inlarge cometary meteoroids; e) the surprising detection of persistent train emission in a slow and notso-bright Taurid fireball, as well as f) the observation of an elve at the peak of the storm. Resultsfrom ground-based efforts included flux measurements of the 1866 storm peak in Australia, the firsthigh frame-rate images of meteors showing a shock-like feature, and the detection of recombinationlines, the UV OH A-X band, and unidentifled near-IR emission in meteor persistent emissions. Thispaper gives a brief overview of the airborne effort and puts the new results in the context of priorwork. | |||||||||
| ISSN | ||||||||||
| 収録物識別子タイプ | ISSN | |||||||||
| 収録物識別子 | 0288-433X | |||||||||
| 書誌レコードID | ||||||||||
| 収録物識別子タイプ | NCID | |||||||||
| 収録物識別子 | AA10455137 | |||||||||
| 資料番号 | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | 資料番号: SA4636312000 | |||||||||
