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A detailed temperature analysis of coronal region 54
Electron density in the solar corona during the eclipse of February 25, 1952
Is the photoelectric detection of the K outer corona easier in the infrared than in the visible?
Problem of the photographic detection of the polarized light of the white corona
An absolute calibration of the Climax intensity scale for coronal lines
Microphotometer determination of final coronal line intensities
Feasibility of the photoelectric detection of the K-outer corona
A hypothesis for the origin of solar flares
Photospheric "hump" on 6 January 1955
The sky brightness near the Sun
Quarterly Research Report 1955-1
The Director's Quarterly Report 1955-4
Quarterly Research Report 1955-2
Quarterly Research Report 1955-3
Solar prominences and geomagnetic disturbance
A theory of solar corpuscular emission
The role of active solar regions in the formation of magnetic storms
Study of spatial movements in solar prominance
Study of the broadening of coronal lines in active centers
Identification of the yellow coronal line: A5694.4

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