Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Big Bear Solar Obs., California Inst. of Technology
Big Bear Solar Observatory, Pasadena, CA
California Institute of Technology, Pasadena.
Big Bear Solar Observatory, Hale Observatoires, California Institute of Technology, Carnegie Institute of Washington
California Institute of Technology, Pasadena, California, USA
Big Bear Solar Observatory, California Institute of Technology, Carnegie Institution of Washington
Big Bear Solar Observatory, California Institute of Technology
California Institute of Technology, Pasadena, CA, US
Solar Astronomy Department, California Institute of Tech-nology, Pasadena, California 91125, USA
Solar Astronomy, California Institute of Technology, Pasadena CA 91125, USA
Big Bear Solar Observatory
Mount Wilson and Palomar Observatoires, Carnegie Institute of Washington, California Institute of Technology
Smithsonian Astrophysical Observatory, Cambridge, MA, US
Mount Wilson and Palomar Observatoires, Carnegie Institution of Washington;, California Institute of Technology
Space Research Laboratory, University of Turku, Turku SF-20520, FinlandGennadiKovaltsovA. F. Ioffe Physical- Technical Institute, St. Petersburg 194021, RussiaJarmoTorstiSpace Research Laboratory, University of Turku, Turku SF-20520, FinlandIlyaUsoskinA. F. Ioffe Physical- Technical Institute, St. Petersburg 194021, RussiaHaroldZirinBig Bear Solar Observatory, Caltech, Pasadena, California 91125AnttiAnttilaRamiVainioSpace Research Laboratory, University of Turku, Turku SF-20520, Finland
California Institute of Technology, MC 264-33, Pasadena, CA 91125 Bear Solar Observatory, California Institute of Technology, Pasadena, California 91125, USA
Solar Astronomy, 264-33 Caltech, Pasadena, CA 91125, USA
Mount Wilson and Palomar Observatoires, Carnegie Institution of Washington, and California Institute of Technology
Mount Wilson and Palomar Observatoires, Carnegie Institution of Washington, California Institut
10830 A He I observations of 455 stars
32-Channel Spectrophotometry of Stellar Flares
A continuum bright point at the penumbral edge
A Frequency Angle Interferometer for Solar Microwave Spectroscopy
A ground-based CaII K-line index as a proxy for the UARS Lyman α irradiance
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