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Charles H. Townes

Researcher at University of California, Berkeley

Publications -  345
Citations -  19936

Charles H. Townes is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Infrared Spatial Interferometer & Interferometry. The author has an hindex of 62, co-authored 345 publications receiving 19318 citations. Previous affiliations of Charles H. Townes include University of California & University of California, Santa Cruz.

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Proceedings ArticleDOI

Sparse-Aperture Adaptive Optics

TL;DR: In this article, a fusion of aperture masking interferometry and adaptive optics (AO) is presented, where an aperture mask is placed downstream of an AO system to recover structure from the traditionally difficult regime of the AO-corrected transfer function.
Journal ArticleDOI

Distribution of Ammonia Density, Velocity, and Rotational Excitation in the Region of Sagittarius B2

TL;DR: Ammonia inversion radiation in Sgr B2 region, observing distribution of density, velocity and rotational excitation was observed in this article, where the distribution of the density, velocities, and excitations was analyzed.
Journal ArticleDOI

The Orion Molecular Clouds OMC-1 and OMC-2 Mapped in the Far-Infrared Fine-Structure Line Emission of C+ and O0

TL;DR: In this paper, the Orion Molecular Ridge (OMC-1 and OMC-2) was mapped in the fine-structure lines [C II] 158 μm and [O I] 63 and 146 μm.
Journal ArticleDOI

How the Laser Happened: Adventures of a Scientist

Charles H. Townes, +1 more
- 01 Dec 1999 - 
TL;DR: The Light That Shines Straight as discussed by the authors is a classic example of a light-that-shines-straight story about a light that shines straight in the sky, and it can be seen as a metaphor for the Rains of Orion.
Journal ArticleDOI

First Surface-resolved Results with the IOTA Imaging Interferometer: Detection of Asymmetries in AGB stars

TL;DR: In this article, the authors measured non-zero closure phases for about 29% of the AGB stars using the 3-telescope Infrared Optical Telescope Array (IOTA) interferometer at near-infrared wavelengths (H band) and with angular resolutions in the range 5-10 milliarcseconds.