| Literature DB >> 23145245 |
Abstract
For those fortunate enough to have personally witnessed and photographed the visible corona surrounding the Sun during a solar eclipse, pictures are usually a let down for not living up to the visual view. After 150 years of investigating the corona, we understand it more fully and now know this difference to be real. The difference stems from our inability to either see or image the true distribution of simultaneous brightness because of its large dynamic range (eg, Rodriguez, Woods, 2008 Digital Image Processing, Upper Saddle River: Pearson Prentice Hall). Brightness in the corona is unprecedented, as it falls by three orders of magnitude over a distance of only one solar radius from the Sun.Entities:
Keywords: coronal streamers; image artefact; optical illusion; solar eclipses
Year: 2011 PMID: 23145245 PMCID: PMC3485804 DOI: 10.1068/i0424
Source DB: PubMed Journal: Iperception ISSN: 2041-6695
Figure 1.A photograph (top) and a woodcut of a naked-eye observation (bottom) of the corona during the solar eclipse of July 29, 1878 (from Ranyard 1881). The large-scale tapering structures in the drawing are known as coronal streamers.
Figure 2.White-light images of the solar eclipse of June 30, 1973 (adapted from Woo 2005). (a) Taken without a radial brightness gradient filter (unprocessed). (b) Taken by a camera equipped with a radial brightness gradient filter (processed). The streamer illusion seen by eye and captured in the sketch of Figure 1 is absent in the unprocessed picture, but artificially generated as the streamer artefact in the processed picture.