谆谆教诲
发表于 2025-3-26 23:50:08
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glamor
发表于 2025-3-27 03:50:51
The SAO Submillimeter Wavelength Arrayith baselines from 9 to 470 m and resolutions as fine as 0‘.‘. Eight receivers will cover all bands from 180 to 900 GHz in linear polarization; two orthogonal polarizations will be available at 350 GHz. Multiyear site testing on Mauna Kea shows that the precipitable water vapor is less than 1 nun fo
迷住
发表于 2025-3-27 05:58:20
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他一致
发表于 2025-3-27 12:25:51
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peptic-ulcer
发表于 2025-3-27 14:59:50
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燕麦
发表于 2025-3-27 20:49:36
Lunar Occultationsss of astronomical sources: from stellar angular diameters to close binaries, from circumstellar shells to the Galactic Centre..Theresolution and sensitivity offered by lunar occultations still compare favorably withthe capabilities of other more modern methods in the optical and near-infrared. Arem
Tinea-Capitis
发表于 2025-3-28 01:05:03
Beam Combination for Wide Field Imaginge beam combination method. A beam combination in the pupil plane can completely overcome one of them. In the image plane, a beam combination obeying the rules of geometrical optics can overcome both limitations in principle, but is difficult to achieve in practice. We discuss particularly the real c
OREX
发表于 2025-3-28 04:42:49
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miracle
发表于 2025-3-28 07:19:58
Source-Noise in Radio Synthesis Images of Polarised Sourcesrms noise at any location in the polarisation images. We compare these results with those for the images of unpolarised sources and discuss the usefulness of deconvolution of snap-shot images in reducing the source-noise from the off-source regions in the images.
上涨
发表于 2025-3-28 13:41:00
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