A Mechanical Theory of the Solar Corona

Cover A Mechanical Theory of the Solar Corona
A Mechanical Theory of the Solar Corona
John Martin Schaeberle
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No photographs; the one drawing, which does not agree with the description by the observer, shows great equatorial exten- sion, with only a few short rays at the pole. (Minimum of spots, 1867. 5. ) 1868, August 18.
All the drawings agree in giving evidence of a considerable inclination of the Sun's axis. (Compare the drawings with the denser portions of Figure 5, Plate I. ) The majority of the drawings give evidence of an eastward inclination of the inner 32 A Mechanical Theory of the Solar Cor
...ona, coronal axis corresponding to a positive value of ft. (Mini- mum of spots, 1867. 5; maximum, 1870. 5. ) 1869, August 7.
Both the photograph and the drawing are in accord with the theory. In the drawing of MEEK and SCHOTT the extension in the equatorial region is greatest at the equator, while the gen- eral outlines, both in the photograph and drawing, are quite similar to the inner portions of Figure 5, Plate I. According to the boundaries of the wings as shown on WHIPPLE'S photo- graph, the axis of the inner corona is inclined eastward as required by theory when ft is positive.


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