Was the eclipse comet of 1893 a disconnected coronal mass ejection?

Details Was the eclipse comet of 1893 a disconnected coronal mass ejection? Was the eclipse comet of 1893 a disconnected coronal mass ejection?

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..122..319c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 122, no. 2, 1989, p. 319-333.

Astronomy and Astrophysics

Astronomy

11

Coronal Loops, Solar Eclipses, Stellar Mass Ejection, Astronomical Photography, Magnetic Field Reconnection, Comets, Eclipses, History, Ejection, Disconnection, Diagrams, Sun, Earth-Based Observations, Hypotheses, Astronomy, Geometry, Photography

Scientific paper

A re-evaluation of observations of the April 16, 1893 solar eclipse suggests that the 'comet' photographed during totality was, in fact, a disconnected coronal mass ejection. Like the disconnection event in 1980 reported by Illing and Hundhausen (1983), the outward speed of the convex (toward the sun) surface for the 1893 event was relatively low (about 90 km/s). Candidate disconnection events were also observed during solar eclipses in 1860 and 1980.

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