Flange
发表于 2025-3-21 19:17:51
书目名称Science with the VLT Interferometer影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0862615<br><br> <br><br>书目名称Science with the VLT Interferometer读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0862615<br><br> <br><br>
闲聊
发表于 2025-3-21 21:36:24
Introduction to Interferometry and closure phase, which can then be fitted by a model or used to reconstruct an image. In order to measure fringes, the path lengths from the source to the detector via the different individual apertures must be equalized. This requires some form of fringe tracking, which constrains the type of ob
Metastasis
发表于 2025-3-22 03:10:38
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BRAWL
发表于 2025-3-22 05:12:23
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ostrish
发表于 2025-3-22 12:05:40
Astrometry with Optical/IR Interferometerssed interferometers: global astrometry and narrow angle astrometry. The ultimate limits for both types of measurements are set by the atmosphere. However, the instrumental considerations for the two types of measurements are quite different. This paper gives an overview of the instrumental aspects o
图画文字
发表于 2025-3-22 13:52:11
Solar-System Observations with the VLTIs (from 0.3 AU to more than 50 AU). VLTI observations of Solar-system objects will concentrate on targets with angular dimensions in the range of an arcsec or smaller. Major objectives are expected to be the search for asteroid companions, the morphological study of asteroids, satellites of outer pl
sterilization
发表于 2025-3-22 20:11:26
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补充
发表于 2025-3-22 21:43:28
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Reclaim
发表于 2025-3-23 01:38:50
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金哥占卜者
发表于 2025-3-23 09:29:16
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