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1.
Opt Lett ; 19(17): 1322-4, 1994 Sep 01.
Artigo em Inglês | MEDLINE | ID: mdl-19855508

RESUMO

A diode-pumped laser with greater than 11 W of cw 1064-nm output power and 3.5 W of frequency-doubled average power at a 50-kHz pulse repetition frequency has been developed. A single Nd:YAG rod was pumped with the combined output of three fiber-coupled diode-laser arrays. Each pump laser was capable of 10 W of cw output power. The fiber output of each pump laser was first collimated and then focused with a single lens onto one end of a Nd:YAG rod. The resonator mirrors for the L-shaped cavity were selected such that thermal lensing in the laser crystal was mostly compensated. The 532-nm output beam quality factor (M(2)) was less than 1.5.

2.
Appl Opt ; 30(11): 1396-400, 1991 Apr 10.
Artigo em Inglês | MEDLINE | ID: mdl-20700296

RESUMO

We demonstrate the feasibility of 3-D acoustooptic spectrum analysis with ultrahigh resolution. Sub-Hertz resolution is achieved by processing over a sequence of CCD frames.

3.
Opt Lett ; 15(21): 1245-6, 1990 Nov 01.
Artigo em Inglês | MEDLINE | ID: mdl-19771055

RESUMO

A three-dimensional acousto-optic spectrum analyzer with subhertz resolution is demonstrated experimentally. The first and second dimensions are the two spatial dimensions of the output detector array, and the third dimension is time as sampled by the detector array frame rate. A superfine resolution of 0.12 Hz has been achieved.

4.
Appl Opt ; 29(36): 5317-9, 1990 Dec 20.
Artigo em Inglês | MEDLINE | ID: mdl-20577555

RESUMO

A 2-D acoustooptic spectrum analyzer with the associated reference function generator and real-time image processor has been constructed. The operation of the analyzer and the experimental considerations for obtaining a high resolution spectrum in real time are described.

5.
Science ; 204(4399): 1306-8, 1979 Jun 22.
Artigo em Inglês | MEDLINE | ID: mdl-17813170

RESUMO

Climatically significant variation of the solar constant (the energy output of the sun) implies measurable change in the solar radius. The available data limit variations of the solar radius between 1850 and 1937 to about 0.25 arc second; modeling of the sun indicates that the solar constant did not vary by more than 0.3 percent during that time.

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