| 词条 | Solar eclipse of October 3, 2005 | |||
| 释义 |
An annular solar eclipse occurred on Monday, 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.[1] 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.[1] 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.[2][3] The eclipse caused a 1–1.4 K drop in the temperature of the ionosphere.[4] Images
Related eclipsesSolar eclipses 2004-2007{{Solar eclipse set 2004-2007}}Saros 134{{Solar Saros series 134}}Metonic cycle{{Solar Metonic series 2001 December 14}}Notes1. ^1 {{cite web | first=Fred | last=Espenak | title=Annular Solar Eclipse of 2005 October 03 | publisher=NASA/GSFC | accessdate=2009-09-23 | url=http://eclipse.gsfc.nasa.gov/SEmono/ASE2005/ASE2005.html }} 2. ^{{cite journal | first=N. | last=Jakowski | title=Ionospheric behavior over Europe during the solar eclipse of 3 October 2005 | journal=Journal of Atmospheric and Solar-Terrestrial Physics | volume=70 | issue=6 |date=April 2008 | pages=836–853 | doi=10.1016/j.jastp.2007.02.016 |bibcode = 2008JASTP..70..836J |display-authors=etal}} 3. ^{{cite journal | first=P. | last=Šauli | title=Acoustic–gravity waves during solar eclipses: Detection and characterization using wavelet transforms | journal=Journal of Atmospheric and Solar-Terrestrial Physics | volume=69| issue=17–18 |date=December 2007 | pages=2465–2484 | doi=10.1016/j.jastp.2007.06.012 |bibcode = 2007JASTP..69.2465S |display-authors=etal}} 4. ^{{cite journal | title=Tropospheric-ionospheric effects of the 3 October 2005 partial solar eclipse in Kharkiv | last=Burmaka | first=V. P. | journal=Kosmichna Nauka I Tekhnologiya | volume=13 | issue=6 | pages=74–86 | date=2007 | bibcode=2007KosNT..13f..74B |display-authors=etal| doi=10.15407/knit2007.06.074 }} References{{Solar eclipse NASA reference|2001/SE2005Oct03A|20050103}}Photos:
4 : Annular solar eclipses|2005 in science|21st-century solar eclipses|October 2005 events |
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