Coma morphology and dust-emission pattern of periodic comet Halley. III - Additional high-resolution images taken in 1910

Astronomy and Astrophysics – Astronomy

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Astronomical Photography, Comet Heads, Cosmic Dust, Halley'S Comet, Image Processing, Data Sampling, High Resolution, Photographic Plates, Tables (Data), Comet, Morphology, Dust, Emissions, Patterns, Halley, Image Processing, Telescope Methods, Observations, Comae, Rotation, Features, Description

Scientific paper

The image-processing algorithm introduced by the authors in Paper I (Larson and Sekanina, 1984) is applied to high-resolution images of periodic comet Halley taken at the Lick, Helwan, Lowell, and Vienna Observatories during the period of May 12 - June 2, 1910 to close the gap between the May and June sequences of the Mount Wilson plates already processed in Paper I and subsequently analyzed in Paper II (Sekanina and Larson, 1984). With the exception of five days around the time of P/Halley's transit across the Sun's disk, the combined set of the Mount Wilson, Lick, Helwan, Lowell, and Vienna images presents a daily, and sometimes twice daily, record of coma features between May 5 and June 6, 1910. General characteristics of the coma features in this augmenting sample of images are discussed.

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