Gerhana matahari: Perbezaan antara semakan

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Polar (bincang | sumb.)
Polar (bincang | sumb.)
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== Cerapan lain ==
[[Fail:2008-08-01 Solar eclipse progression with timestamps.jpg|thumb|Perkembangan gerhana matahari pada 1 Ogos 2008 di [[Novosibirsk]], [[Russia]]. Semua masa UTC (waktu tempatan adalah UTC+7). Jangka masa antara gambar adalah tiga minit.]]
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For [[astronomers]], a total solar eclipse forms a rare opportunity to observe the [[corona]] (the outer layer of the Sun's atmosphere). Normally this is not visible because the [[photosphere]] is much brighter than the corona. According to the point reached in the [[solar cycle]], the corona may appear small and symmetric, or large and fuzzy. It is very hard to predict this prior to totality.<ref>{{cite web |title=The science of eclipses |publisher=ESA |url=http://www.esa.int/esaSC/SEMYK9R1VED_index_0.html |accessdate=2007-08-04}}</ref>
 
Bagi ahli [[astronomi]], gerhana matahari penuh memberi peluang yang jarang untuk memerhatikan [[korona]] (lapisan luar atmosfera Matahari). Biasanya ini tidak kelihatan kerana [[fotosfera]] adalah lebih cerah daripada korona. Berdasarkan titik dicapai dalam [[kitaran suria]], korona mungkin kelihatan kecil dan simetri, atau besar dan kabur. Hal ini sangat sukar untuk diramalkan sebelum kepenuhan.<ref>{{cite web |title=The science of eclipses |publisher=ESA |url=http://www.esa.int/esaSC/SEMYK9R1VED_index_0.html |accessdate=2007-08-04}}</ref>
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During a solar eclipse, special (indirect) observations can also be achieved with the unaided eye only. Normally the spots of light which fall through the small openings between the leaves of a tree, have a circular shape. These are images of the Sun. During a partial eclipse, the light spots will show the partial shape of the Sun, as seen on the picture.