Image-processing techniques in precisely measuring positions of Jupiter and its Galilean satellites
文献类型:期刊论文
作者 | Peng, QY1,2,3,4![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2003-04 |
卷号 | 401期号:2页码:773-779 |
关键词 | techniques : image processing planets and satellites : individual : Jupiter astrometry |
ISSN号 | 0004-6361 |
产权排序 | 第四完成单位 |
通讯作者 | Peng, QY (reprint author), Jinan Univ, Dept Comp Sci, Guangzhou 510632, Peoples R China. |
英文摘要 | Two image-processing techniques are developed to measure precisely the positions of Jupiter and its Galilean satellites. One is used to detect the edge of Jupiter's CCD image and fit it with an ellipse, thereby obtaining the planetary center. The other is used to remove the positional effect of Jupiter's scattering light that has on the measurement of a close satellite. 133 frames of CCD images are measured by using these techniques, and these measured positions of Galilean satellites are compared to the ones computed with the ephemerides of Jacobson's JUP204 and Arlot's G5. Preliminary analysis of the data as Jupiter-satellite or inter-satellite positions shows that a standard error (i.e. internal precision) as small as 0.03 arcsec can be reached in right ascension and declination. It is believed that these techniques would be useful for astrometric and photometric CCD observations of Galilean satellites, especially for CCD observations in the forthcoming mutual phenomena of Galilean satellites. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | EXTRAGALACTIC RADIO-SOURCES ; OPTICAL POSITIONS ; CCD ASTROMETRY ; OUTER PLANETS ; SATURN |
收录类别 | SCI ; EI |
原文出处 | http://www.aanda.org/articles/aa/abs/2003/14/aa2853/aa2853.html |
语种 | 英语 |
WOS记录号 | WOS:000181708800040 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4166] ![]() |
专题 | 云南天文台_其他 |
作者单位 | 1.Department of Computer Science, Jinan University, Guangzhou 510632, PR China 2.National Astronomical Observatories, CAS, Beijing 100012, PR China 3.Joint Laboratory for Optical Astronomy, CAS, Kunming 650011, PR China 4.Center of Astrophysics, Guangzhou University, Guangzhou 510400, PR China 5.Department of Mathematics, Jinan University, Guangzhou 510632, PR China 6.Yunnan Observatory, National Astronomical Observatories, CAS, Kunming 650011, PR China |
推荐引用方式 GB/T 7714 | Peng, QY,Han, YB,Zhang, CL,et al. Image-processing techniques in precisely measuring positions of Jupiter and its Galilean satellites[J]. ASTRONOMY & ASTROPHYSICS,2003,401(2):773-779. |
APA | Peng, QY,Han, YB,Zhang, CL,&Li ZL.(2003).Image-processing techniques in precisely measuring positions of Jupiter and its Galilean satellites.ASTRONOMY & ASTROPHYSICS,401(2),773-779. |
MLA | Peng, QY,et al."Image-processing techniques in precisely measuring positions of Jupiter and its Galilean satellites".ASTRONOMY & ASTROPHYSICS 401.2(2003):773-779. |
入库方式: OAI收割
来源:云南天文台
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