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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
The Climax- March 1962
The Director's Report
Relation between K-coronal intensity maxima and geomagnetic disturbance
The role of active solar regions in the formation of magnetic storms
The Climax- March 1963
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
The Climax- October 1961
The Director's Report
Utilization of transit of mercury for research purposes
Magnetic intensification on the sunspot spectra

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