George Ellery Hale
1868 – 1938
50 works on record
Works
Beyond the milky way
The National importance of scientific and industrial research
The spectra of stars of Secchi's fourth type
The modern spectroscope
The solar faculae
The ultra-violet spectrum of the solar prominences
The Astrophysical Observatory of the California Institute of Technology
The new heavens
Fabrica et uso di alcuni stromenti horarii universali
The national value of scientific research
On the probable existence of a magnetic field in sun-spots
Some opportunities for astronomical work with inexpensive apparatus
Some recent contributions to our knowledge of the sun
The George Ellery Hale papers, 1882-1937, at the Mount Wilson and Palomar Observatories Library, Pasadena, California
The study of stellar evolution
The Solar observatory of the Carnegie Institution of Washington
On the condition of the sun's surface in June and July, 1892, as compared with the record ofterrestrial magnetism
Photography of the corona without an eclipse
The new heavens
National academies and the progress of research
The Rumford spectroheliograph of the Yerkes Observatory
Magnetic observations of sunspots, 1917-1924 ... b̀y George E. Hale ànd Seth B. Nicholson
The Yerkes observatory of the University of Chicago
Some recent contributions to our knowledge of the sun
Co-operation in research
The magnetic polarity of sun-spots
The five-foot spectroheliograph of the Solar Observatory
A vertical coelostat telescope
A study of the conditions for solar research at Mt. Wilson, California
Photographic observations of the spectra of sun-spots
Photography of the solar prominences
Beyond the milky way
The rotation period of the sun as determined from the motions of the calcium flocculi
Some new applications of the spectroheliograph
The depths of the universe
A national focus of science and research
Magnetic observation of sunspots, 1917-1924 ..
On the probability of chance coincidence of solar and terrestrial phenomena
A photographic comparison of the spectra of the limb and the center of the sun
Signals from the stars
The rotation period of the sun as determined from the motion of the calcium flocculi
A remarkable solar disturbance
Preliminary paper on the cause of the characteristic phenomena of sun-spot spectra
On some attempts to photograph the solar corona without an eclipse
The ultra-violet spectrum of the solar prominences
A program of solar research
Sun-spot lines in the spectra of red stars
Ten years' work of a mountain observatory
Some tests of the snow telescope
The spectrum of the high potential discharge between metallic electrodes in liquids and in gases at high pressures