考虑光压力的人造地球卫星轨道运动持续时间的近似计算

IF 0.7 Q3 PHYSICS, MULTIDISCIPLINARY Journal of Physical Studies Pub Date : 2021-01-29 DOI:10.30970/JPS.25.1901
M. M. Koval'chuk, Y. Vovchyk, O. Baran, A. Bilinsky, I. P. Laushnyk, M. Stodilka, M. Hirnyak
{"title":"考虑光压力的人造地球卫星轨道运动持续时间的近似计算","authors":"M. M. Koval'chuk, Y. Vovchyk, O. Baran, A. Bilinsky, I. P. Laushnyk, M. Stodilka, M. Hirnyak","doi":"10.30970/JPS.25.1901","DOIUrl":null,"url":null,"abstract":"A comprehensive research was conducted to establish the in(cid:29)uence of solar pressure on the existence of arti(cid:28)cial Earth satellites in their orbit. Six low-orbit satellites and one satellite with a high-elliptical orbit moving in orbit during 2001(cid:21)2020 were selected for the study. We used the USSTRATCOM database of the satellites’ orbital elements (http://www.space-track.org/), additional data were taken from CalSky (https://www.calsky.com) and TLEtools (https://tletools.readthedocs.io). Taking into account light pressure, we re(cid:28)ned the calculation of the duration of a satellite’s orbital motion, which we had performed earlier [M. M. Koval’chuk, Bull. Natl. Univ. Kyiv. Astron. 55, 39 (2017)], and clari(cid:28)ed the moment of its destruction. Using the proposed method allowed us to reduce the di(cid:27)erence between the calculated and the real lifetime of satellites: for low-orbit satellites, the di(cid:27)erence between the calculated and the real time of their existence in orbit does not exceed ± 1 day, for a satellite with a highly elliptical orbit it is +2 days. Such accuracy is su(cid:30)cient to produce proper forecasts. Thus, consideration of light pressure gives a small correction in the calculations in the case of low-orbit satellites, but this correction can be signi(cid:28)cant for low-mass and large-surface objects moving in medium and high (geostationary) orbits [Ch. Lucking, C. Colombo, C. R. McInnes, Acta Astronaut. 77, 197 (2012)].Keywords:","PeriodicalId":43482,"journal":{"name":"Journal of Physical Studies","volume":"20 1","pages":""},"PeriodicalIF":0.7000,"publicationDate":"2021-01-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Approximate evaluation of the duration of the orbital motion of artificial Earth satellites taking into account light pressure\",\"authors\":\"M. M. Koval'chuk, Y. Vovchyk, O. Baran, A. Bilinsky, I. P. Laushnyk, M. Stodilka, M. Hirnyak\",\"doi\":\"10.30970/JPS.25.1901\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A comprehensive research was conducted to establish the in(cid:29)uence of solar pressure on the existence of arti(cid:28)cial Earth satellites in their orbit. Six low-orbit satellites and one satellite with a high-elliptical orbit moving in orbit during 2001(cid:21)2020 were selected for the study. We used the USSTRATCOM database of the satellites’ orbital elements (http://www.space-track.org/), additional data were taken from CalSky (https://www.calsky.com) and TLEtools (https://tletools.readthedocs.io). Taking into account light pressure, we re(cid:28)ned the calculation of the duration of a satellite’s orbital motion, which we had performed earlier [M. M. Koval’chuk, Bull. Natl. Univ. Kyiv. Astron. 55, 39 (2017)], and clari(cid:28)ed the moment of its destruction. Using the proposed method allowed us to reduce the di(cid:27)erence between the calculated and the real lifetime of satellites: for low-orbit satellites, the di(cid:27)erence between the calculated and the real time of their existence in orbit does not exceed ± 1 day, for a satellite with a highly elliptical orbit it is +2 days. Such accuracy is su(cid:30)cient to produce proper forecasts. Thus, consideration of light pressure gives a small correction in the calculations in the case of low-orbit satellites, but this correction can be signi(cid:28)cant for low-mass and large-surface objects moving in medium and high (geostationary) orbits [Ch. Lucking, C. Colombo, C. R. McInnes, Acta Astronaut. 77, 197 (2012)].Keywords:\",\"PeriodicalId\":43482,\"journal\":{\"name\":\"Journal of Physical Studies\",\"volume\":\"20 1\",\"pages\":\"\"},\"PeriodicalIF\":0.7000,\"publicationDate\":\"2021-01-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Physical Studies\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.30970/JPS.25.1901\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Physical Studies","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.30970/JPS.25.1901","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0

摘要

为了确定太阳压力对人造地球卫星在轨存在的影响,进行了全面的研究。选取2001(cid:21)2020年在轨运行的6颗低轨道卫星和1颗高椭圆轨道卫星作为研究对象。我们使用了USSTRATCOM卫星轨道要素数据库(http://www.space-track.org/),其他数据来自CalSky (https://www.calsky.com)和TLEtools (https://tletools.readthedocs.io)。考虑到光的压力,我们(cid:28)需要计算卫星轨道运动的持续时间,我们之前已经做过了。科瓦尔丘克先生,布尔。国家的。大学,基辅。天文学,55,39(2017)],而克拉丽(cid:28)则记录了它毁灭的时刻。采用该方法可以减小卫星计算寿命与实际寿命之间的差值(cid:27):对于低轨道卫星,其计算寿命与实际在轨生存时间的差值不超过±1天,对于高椭圆轨道卫星,其差值为+2天。这样的精确度对于做出正确的预测是非常重要的。因此,在低轨道卫星的情况下,考虑光压的计算误差很小,但对于在中、高(地球静止)轨道上运行的低质量和大表面物体,这种误差可能很大(cid:28) [Ch. Lucking, C. Colombo, C. R. McInnes,《宇航员学报》,77,197(2012)]。关键词:
本文章由计算机程序翻译,如有差异,请以英文原文为准。
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
Approximate evaluation of the duration of the orbital motion of artificial Earth satellites taking into account light pressure
A comprehensive research was conducted to establish the in(cid:29)uence of solar pressure on the existence of arti(cid:28)cial Earth satellites in their orbit. Six low-orbit satellites and one satellite with a high-elliptical orbit moving in orbit during 2001(cid:21)2020 were selected for the study. We used the USSTRATCOM database of the satellites’ orbital elements (http://www.space-track.org/), additional data were taken from CalSky (https://www.calsky.com) and TLEtools (https://tletools.readthedocs.io). Taking into account light pressure, we re(cid:28)ned the calculation of the duration of a satellite’s orbital motion, which we had performed earlier [M. M. Koval’chuk, Bull. Natl. Univ. Kyiv. Astron. 55, 39 (2017)], and clari(cid:28)ed the moment of its destruction. Using the proposed method allowed us to reduce the di(cid:27)erence between the calculated and the real lifetime of satellites: for low-orbit satellites, the di(cid:27)erence between the calculated and the real time of their existence in orbit does not exceed ± 1 day, for a satellite with a highly elliptical orbit it is +2 days. Such accuracy is su(cid:30)cient to produce proper forecasts. Thus, consideration of light pressure gives a small correction in the calculations in the case of low-orbit satellites, but this correction can be signi(cid:28)cant for low-mass and large-surface objects moving in medium and high (geostationary) orbits [Ch. Lucking, C. Colombo, C. R. McInnes, Acta Astronaut. 77, 197 (2012)].Keywords:
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Journal of Physical Studies
Journal of Physical Studies PHYSICS, MULTIDISCIPLINARY-
CiteScore
1.00
自引率
20.00%
发文量
19
期刊最新文献
Deformed Heisenberg algebras of different types with preserved weak equivalence principle High selective absorption by a planar multilayer structure with two low absorbing materials in the core Chaotic dynamics of magnetic fields generated by thermomagnetic instability in a nonuniformly rotating electrically conductive fluid Relation between flare activity and magnetic complexity of active regions on the Sun Using the Fabry–Pérot interferometer as a spectral mask
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1