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A hypothesis for the origin of solar flares
Observation of the K corona from aircraft
Coronal emission in the yellow line region of 20 April 1956
Serial washing of films
Indirect measurement of solar energy variations in the extreme ultraviolet and x-ray region
Recent auroras seen in Japan
Relation between K-coronal intensity maxima and geomagnetic disturbance
The role of active solar regions in the formation of magnetic storms
Plans for the calibration of the X-coronameter
Observation of polarized light in flare continuum
Flare profile study at Climax
Identification of the yellow coronal line: A5694.4
Electron density in the solar corona during the eclipse of February 25, 1952
Utilization of transit of mercury for research purposes
Magnetic intensification on the sunspot spectra
Evaluation of Climax coronal intensities
Brondened H? absorption lines spectra, 14 May 1951
Studies of solar granulation. The frequency spectrum at long spatial wave lengths
Study of the broadening of coronal lines in active centers
Photometry and polarimetry of the Earthshine with the coronagraph and photoelectric polarimeter

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