小流星烧蚀模型:应用于英仙座观测

IF 0.4 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Contributions of the Astronomical Observatory Skalnate Pleso Pub Date : 2021-12-01 DOI:10.31577/caosp.2021.51.3.186

V. Efremov, O. Popova, D. Glazachev, A. Margonis, J. Oberst, A. Kartashova

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引用次数: 1

摘要

V.Efremov、O.Popova、D.Glazachev、A.Margonis、J.Oberst和A.Kartashova 1萨多夫斯基地圈动力学研究所，俄罗斯莫斯科，（电子邮件：efremov.vv@phystech.edu)2俄罗斯莫斯科物理技术研究所3柏林理工大学、德国柏林大地测量和地理信息科学研究所4德国航空航天中心、德国柏林行星研究所5俄罗斯莫斯科RAS天文研究所

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Small meteor ablation model: Applying to Perseid observations

V. Efremov, O. Popova, D. Glazachev, A. Margonis, J. Oberst and A. Kartashova 1 Sadovsky Institute of Geosphere Dynamics RAS, Moscow, Russia, (E-mail: efremov.vv@phystech.edu) 2 Moscow Institute of Physics and Technology Moscow, Russia 3 Technische Universität Berlin, Institute of Geodesy and Geoinformation Science Berlin, Germany 4 German Aerospace Center (DLR), Institute of Planetary Research Berlin, Germany 5 Institute of Astronomy RAS Moscow, Russia

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来源期刊

Contributions of the Astronomical Observatory Skalnate Pleso 地学天文-天文与天体物理

CiteScore

1.10

自引率

20.00%

发文量

审稿时长

>12 weeks

期刊介绍： Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.