声音会爆炸 发表于 2025-3-21 16:46:00

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情感 发表于 2025-3-21 21:33:06

Exploring Methods of Effective Data Display in an Interactive Astronomical Data-Processing Environmend polemics), you are also astronomers with a strong motivation to sift out of your data the useful information on the physics of cosmic radio sources, and to do it in the most efficient way possible.

吞噬 发表于 2025-3-22 01:31:21

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烦忧 发表于 2025-3-22 06:15:34

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围裙 发表于 2025-3-22 11:19:07

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defeatist 发表于 2025-3-22 15:19:47

Fundamental Aspects of Aperture Synthesis with Limited or No Phase Informations and the mutual coherence function itself and the phase uncertainties introduced by the ionospheric and tropospheric irregularities are often the factor limiting the quality of radioastronomical maps.

reject 发表于 2025-3-22 20:00:55

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热心助人 发表于 2025-3-23 00:32:20

0067-0057 during the period 10-12 August 1978. The colloquium was attended by 108 participants from 14 countries (U.S.A. 29, the Netherlands 20, U.K. 19, Germany 10, France 7, Australia 5, Canada 5, Japan 4, India 2, New Zea­ land 2, Sweden 2, Argentina I, Belgium I, Israel I). It was sponsored by the Netherl

GAVEL 发表于 2025-3-23 03:19:53

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extinguish 发表于 2025-3-23 09:28:59

“Kneading”: The Adjustment of Instrumental Phase and Gain Parameters to Suppress Error Patterns in aere interference from other sources would be too strong, their influence may be reduced by Cleaning the map prior to model fitting. One example of the results for atmospheric position scintillation and one for baseline calibration errors will be shown.
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查看完整版本: Titlebook: Image Formation from Coherence Functions in Astronomy; Proceedings of IAU C Cornelis Schooneveld Conference proceedings 1979 D. Reidel Publ