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THE ASTROPHYSICAL JOURNAL, 565 : 1376È1380, 2002 February[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. THE POTENTIAL FOR ATMOSPHERIC PATH LENGTH COMPENSATION IN STELLAR INTERFEROME
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Document Date: 2005-06-13 13:51:54


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City

New York / /

Company

Hale D. D. / /

Country

United States / /

Currency

pence / /

Facility

Mount Wilson Observatory / University of Toronto / Clemson University / Massachusetts Institute of Technology / Haystack Observatory / Le Conte Hall / University of California / University of Wisconsin / /

IndustryTerm

telescope imaging a†ected / particular site / /

Movie

A. I. / /

NaturalFeature

Mount Wilson Observatory / Mount Wilson / /

OperatingSystem

L3 / /

Organization

Army Research Office / National Science Foundation / University of California / Berkeley / York Univ. / Massachusetts Institute of Technology / American Astronomical Society / Clemson University / University of Toronto / University of Wisconsin / POTENTIAL FOR ATMOSPHERIC PATH LENGTH COMPENSATION IN STELLAR INTERFEROMETRY C. H. TOWNES Department of Physics / /

Person

Thomas Duck / John W. Meriwether / Lowe / Truehaft / RAMAN SCATTERING / /

Position

R. N. / light bucket ÏÏ collector / /

ProvinceOrState

Wisconsin / California / Massachusetts / /

PublishedMedium

THE ASTROPHYSICAL JOURNAL / /

Technology

radiation / laser / lasers / /

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