建筑物的正面
发表于 2025-3-21 17:18:34
书目名称General Theory of Light Propagation and Imaging Through the Atmosphere影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0382138<br><br> <br><br>书目名称General Theory of Light Propagation and Imaging Through the Atmosphere读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0382138<br><br> <br><br>
演讲
发表于 2025-3-21 23:41:44
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弯腰
发表于 2025-3-22 00:41:34
Rajeev Kumar Jaiman,Vaibhav Joshirates into the atmospheric MTF. For any atmospheric path, the latter function determines the resolution that can be obtained when observing over that path. The development of scintillation is examined in the space below the layer, the extent to which it occurs depends crucially on the size of the turbulence structures in the layer.
flaunt
发表于 2025-3-22 07:51:55
https://doi.org/10.1007/3-540-31103-3 the autocorrelation function of that fluctuation, ρ(ξ, η). These two measures provide the essential statistical information about turbulence structure in the path. They also provide the essential statistical properties of the complex amplitudes and intensities in star images formed by telescopes observing over the path.
Monotonous
发表于 2025-3-22 10:09:15
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小淡水鱼
发表于 2025-3-22 13:30:02
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小淡水鱼
发表于 2025-3-22 17:56:30
https://doi.org/10.1007/978-3-7091-0947-2 by .; at near-IR wavelengths resolution is typically ~0.1 arcsec. Though image cores generally appear over a wide range of wavelengths, one particular wavelength—referred to as the optimum wavelength—gives rise to maximum irradiance at core center. This wavelength has obvious significance to HEL weapon systems.
BOON
发表于 2025-3-22 23:27:17
Computer Modeling of Atherosclerosis, of the telescope; speckle size is not affected by aberrations. In polychromatic speckle, individual speckles are chromatically stretched into rainbow-like features by an amount proportional to the feature’s radial distance from image center. Stellar speckle is a form of image noise; various speckle reduction strategies are analyzed.
etidronate
发表于 2025-3-23 04:53:21
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heckle
发表于 2025-3-23 09:29:08
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