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Titlebook: Laser Guide Star Adaptive Optics for Astronomy; N. Ageorges,C. Dainty Book 2000 Springer Science+Business Media Dordrecht 2000 ASTER.adapt

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樓主: 反抗日本
11#
發(fā)表于 2025-3-23 12:21:48 | 只看該作者
Stephen T. Ridgwayrch in two related areas: limit theorems for sums of independent Banach space valued random vectors and general Gaussian processes. An important feature in these past research studies has been the fact that they highlighted the es- sential probabilistic nature of the problems considered. In part, th
12#
發(fā)表于 2025-3-23 15:36:56 | 只看該作者
13#
發(fā)表于 2025-3-23 19:34:59 | 只看該作者
Jack D. Drummondrch in two related areas: limit theorems for sums of independent Banach space valued random vectors and general Gaussian processes. An important feature in these past research studies has been the fact that they highlighted the es- sential probabilistic nature of the problems considered. In part, th
14#
發(fā)表于 2025-3-23 22:19:59 | 只看該作者
15#
發(fā)表于 2025-3-24 06:20:20 | 只看該作者
16#
發(fā)表于 2025-3-24 06:34:04 | 只看該作者
Cláudia S. Rolad . are arbitrary real numbers such that θ > ?(ρ + 1)/2. The eigenfunctions of these expansions have simple expressions in terms of Bessel functions ..(?) and J.(?) of the first kind with indexes ./(2. + . + 1) and . ? 1 = ?(2. + 1)/(2. + . + 1). The corresponding eigenvalues have simple expressions
17#
發(fā)表于 2025-3-24 11:43:13 | 只看該作者
g., [. – .]). However, the related considerations have only been concerned with Banach spaces. (In general, both absolutely summing mappings and measures in nonnormed spaces are studied very poorly.) The basic result of this paper, Theorem 3.1, appears purely topological, for no measures are mention
18#
發(fā)表于 2025-3-24 15:05:53 | 只看該作者
Adaptive Optics with Laser Guide Stars: Basic Concepts and Limitations,ical adaptive optics: the limited sky coverage due to the requirement of having a bright object within the isoplanatic angle, which is needed for wavefront sensing. This article gives a brief introduction into the formation of laser guide stars, either through Rayleigh backscattering in the lower at
19#
發(fā)表于 2025-3-24 20:31:24 | 只看該作者
The Physics of the Sodium Atom,d by resonant scattering of sodium atoms in the mesosphere are attractive for large telescopes because the size of telescope that can be corrected at a given wavelength with a single beacon scales as its height. However, efficient generation of a compact sodium beacon is harder to achieve than for a
20#
發(fā)表于 2025-3-25 02:19:10 | 只看該作者
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