COMPARISON OF DARK PIXELS OBSERVED BY VIS AND UVI - IN DAYGLOW IMAGES

Citation
G. Parks et al., COMPARISON OF DARK PIXELS OBSERVED BY VIS AND UVI - IN DAYGLOW IMAGES, Geophysical research letters, 25(16), 1998, pp. 3063-3066
Citations number
4
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
00948276
Volume
25
Issue
16
Year of publication
1998
Pages
3063 - 3066
Database
ISI
SICI code
0094-8276(1998)25:16<3063:CODPOB>2.0.ZU;2-9
Abstract
Frank and Sigwarth [1997a] claim that the dark pixels observed in dayg low images obtained by the Earth sensor of the Visible Imaging System (VIS) are due to bombardment of Earth by 20 to 40 ton cosmic snowballs . We have independently studied the VIS data and compared the dark pix els from the VIS images to those obtained from the overlapping images from the Ultraviolet Imager (UVI). We find the occurrence distribution s of the dark pixels, single and multiple, from VIS and UVI are nearly identical. The distributions also do not show any altitude dependence . A search for evidence of spacecraft ''wobble'' motion, whose presenc e would indicate that the source is external to the camera, has found that pairs of dark pixel clusters are uniformly distributed in orienta tion and no preference is observed in the wobble direction. Instrument artifacts as the source of the dark pixels is the most likely explana tion for these results. The conclusion of this study is that neither V IS nor UVI provide any scientific evidence that the dark pixels are ge ophysical.