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Titlebook: Very High Angular Resolution Imaging; Proceedings of the 1 J. G. Robertson,W. J. Tango Conference proceedings 1994 Springer Science+Busines

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發(fā)表于 2025-3-21 17:34:42 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Very High Angular Resolution Imaging
副標題Proceedings of the 1
編輯J. G. Robertson,W. J. Tango
視頻videohttp://file.papertrans.cn/983/982608/982608.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: Very High Angular Resolution Imaging; Proceedings of the 1 J. G. Robertson,W. J. Tango Conference proceedings 1994 Springer Science+Busines
描述The 1990s are proving to be a very exciting p&iod for high angular resolution astronomy. At radio wavelengths a combination of new array instruments and pow- erful imaging algorithms have generated images of unprecedented resolution and quality. In the optical and infrared, the great technical difficulties associated with constructing separated-aperture interferometers have been largely overcome, and many new instruments are now operating or are being developed. As these pro- grams start to produce observational results they will be able to draw extensively on the experience gained by the radio-interferometry community. Thus it seemed that the time was ripe for a meeting which would bring together workers from all wavelength ranges to discuss the details of the science and art of "Very High Angular Resolution Imaging" . While the main emphasis of Symposium No. 158 was on high resolution tech- niques from the radio, mm-wave, infrared and optical bands, it also provided an opportunity for presentation of astronomical results from these techniques. As well as giving our colleagues from the Northern Hemisphere a break from midwinter, the location of the Symposium in Australia recognise
出版日期Conference proceedings 1994
關(guān)鍵詞algorithms; astronomy; instruments; interferometry; observatory; optical interferometry; radio astronomy; s
版次1
doihttps://doi.org/10.1007/978-94-011-0880-5
isbn_softcover978-0-7923-2633-5
isbn_ebook978-94-011-0880-5Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightSpringer Science+Business Media Dordrecht 1994
The information of publication is updating

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International Astronomical Union Symposiahttp://image.papertrans.cn/v/image/982608.jpg
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https://doi.org/10.1007/978-94-011-0880-5algorithms; astronomy; instruments; interferometry; observatory; optical interferometry; radio astronomy; s
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發(fā)表于 2025-3-22 19:14:58 | 只看該作者
SeeingAtmospheric turbulence limits the resolution of ground-based high-resolution telescopes. In the optical and radio regimes, the seeing may be described in similar ways, although the parameters are different.
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發(fā)表于 2025-3-23 01:17:54 | 只看該作者
Recent Results from the VLBAThe VLBA construction phase is now over and in the spring of 1993 it is hoped that full VLBA observing can begin. However the VLBA antennas have been operational for some time and several astronomy programs have been run on them. Below we shall present some of these latest results.
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The Southern Hemisphere VLBI Experiment program, SHEVEThe Southern Hemisphere VLBI Experiment (SHEVE) program is aimed at producing high-resolution images of southern radio sources. The radio telescopes of the present SHEVE array are described below and some recent results presented.
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發(fā)表于 2025-3-23 07:14:34 | 只看該作者
T. J. Cornwellsammenhang zwischen holomorphen und harmonischen Funktionen hergestellt und das Dirichlet-Problem für Kreisscheiben gel?st, sowie die Green’sche Funktion zum Laplace-Operator eingeführt. Au?erdem wird das Verhalten ebener Str?mungen auf dem Rand untersucht.
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