Semakan pada 09:28, 25 November 2015 sunting Polar (bincang \| sumb.) Penyelia 53,106 suntingan →‎Kepenuhan ← Suntingan sebelumnya		Semakan pada 09:32, 25 November 2015 sunting batalkan Polar (bincang \| sumb.) Penyelia 53,106 suntingan →‎Fotografi Suntingan berikutnya →
Baris 216: === Fotografi === Mengambil gambar gerhana boleh dilakukan dengan peralatan kamera yang agak biasa. Bagi membolehkan cakera matahari/bulan boleh dilihat dengan mudah, pembesaran [[kanta telefoto]] yang agak tinggi is needed (70–200 mm untuk kamera 35 mm), dan untuk cakera untuk mengisi kebanyakan bingkai, kanta yang lebih panjang diperlukan (lebih 500 mm). Seperti melihat matahari secara langsung, melihat melalui pemidang tilik [[kamera]] boleh menghasilkan kerosakan pada retina, jadi dinasihatkan berwaspada.<ref>{{cite web\|url=http://www.eclipse-chasers.com/eclphot.htm \|title=Photographing the Total Solar Eclipse \|publisher=Eclipse-chasers.com \|date= \|accessdate=2010-03-07}}</ref> <!--▼ Photographing an eclipse is possible with fairly common camera equipment. In order for the disk of the sun/moon to be easily visible, a fairly high magnification [[telephoto lens]] is needed (70–200 mm for a 35 mm camera), and for the disk to fill most of the frame, a longer lens is needed (over 500 mm). As with viewing the sun directly, looking at it through the viewfinder of a [[camera]] can produce damage to the retina, so care is advised.<ref>{{cite web\|url=http://www.eclipse-chasers.com/eclphot.htm \|title=Photographing the Total Solar Eclipse \|publisher=Eclipse-chasers.com \|date= \|accessdate=2010-03-07}}</ref> == ~~Other~~Cerapan ~~observations~~lain == [[Fail:2008-08-01 Solar eclipse progression with timestamps.jpg\|thumb\|~~The~~Perkembangan ~~progression~~gerhana ofmatahari apada ~~solar~~1 ~~eclipse on August 1,~~Ogos 2008 indi [[Novosibirsk]], [[Russia]]. ~~All~~Semua ~~times~~masa UTC (~~local~~waktu ~~time~~tempatan ~~was~~adalah UTC+7). ~~The time~~Jangka ~~span~~masa ~~between~~antara ~~shots~~gambar isadalah ~~three~~tiga ~~minutes~~minit.]] ▲<!-- 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>

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