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・ Solar eclipse of October 21, 1930
・ Solar eclipse of October 21, 1949
・ Solar eclipse of October 22, 1911
・ Solar eclipse of October 23, 1957
・ Solar eclipse of October 23, 1976
・ Solar eclipse of October 23, 2014
・ Solar eclipse of October 24, 1995
・ Solar eclipse of October 24, 2060
・ Solar eclipse of October 24, 2079
・ Solar eclipse of October 24, 2098
・ Solar eclipse of October 25, 2022
・ Solar eclipse of October 25, 2041
・ Solar eclipse of October 26, 2087
・ Solar eclipse of October 27, 1780
・ Solar eclipse of October 3, 1986
Solar eclipse of October 3, 2005
・ Solar eclipse of October 3, 2043
・ Solar eclipse of October 31, 1902
・ Solar eclipse of October 4, 2051
・ Solar eclipse of October 4, 2070
・ Solar eclipse of October 4, 2089
・ Solar eclipse of October 7, 1801
・ Solar eclipse of October 7, 2135
・ Solar eclipse of September 1, 1951
・ Solar eclipse of September 1, 2016
・ Solar eclipse of September 10, 1923
・ Solar eclipse of September 10, 1942
・ Solar eclipse of September 11, 1969
・ Solar eclipse of September 11, 1988
・ Solar eclipse of September 11, 2007


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Solar eclipse of October 3, 2005 : ウィキペディア英語版
Solar eclipse of October 3, 2005

An annular solar eclipse occurred on October 3, 2005 with a magnitude of 0.958. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
It was visible from a narrow corridor through the Iberian peninsula and Africa. A partial eclipse was seen from the much broader path of the Moon's penumbra, including all of Europe, Africa and southwestern Asia.
The path of the eclipse began in the North Atlantic ocean at 08:41 universal time (UT). The antumbra reached Madrid, Spain at 08:56 UT, lasting four minutes and eleven seconds and 90% of the Sun was covered by the Moon. The antumbra reached Algiers at 09:05 UT, then passed through Tunisia and Libya before heading southeast through Sudan, Kenya and Somalia. The shadow then moved out over the Indian Ocean until it terminated at sunset, 12:22 UT.
The maximum eclipse duration occurred in central Sudan at 10:31:42 UT, where it lasted for 4m 31s when the Sun was 71° above the horizon.〔 The theoretical maximum duration for a modern solar eclipse is 7 minutes, 32 seconds.
The motion of the shadow was supersonic and it generated gravity waves that were detectable as disturbances in the ionosphere. These gravity waves originate in the thermosphere at an altitude of about 180 km. Because of the obscuration of solar radiation, the ionization level dropped by 70% during the eclipse. The eclipse caused a 1–1.4 K drop in the temperature of the ionosphere.〔
== Images ==


Image:Partial_Eclipse_Chennai_Oct2005.jpg|Chennai, India : Partial
File:SE2005Oct03A.gif|Animated path
File:031005 anular eclipse.jpg|Spain
File:Sombra del Eclipse anular.JPG|Eclipse shadows from a tree

Degania A, Israel : Partial

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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