Semakan pada 09:21, 25 November 2015 sunting Polar (bincang \| sumb.) Penyelia 53,106 suntingan →‎Amalan umat Islam ← Suntingan sebelumnya		Semakan pada 09:24, 25 November 2015 sunting batalkan Polar (bincang \| sumb.) Penyelia 53,106 suntingan →‎Kepenuhan Suntingan berikutnya →
Baris 207: === Kepenuhan === <!--▼ It is safe to observe the total phase of a solar eclipse directly with the unaided eye, binoculars or a telescope, only when the Sun's photosphere is completely covered by the Moon. During this period the sun is too dim to be seen through filters. The Sun's faint [[corona]] will be visible, and the [[chromosphere]], [[solar prominence]]s, and possibly even a [[solar flare]] may be seen. However, viewing the Sun after totality can be dangerous. [[Fail:TheSun beads.jpg\|thumb\|[[Baily's beads]]]]▼ Adalah selamat untuk memerhatikan keseluruhan fasa gerhana matahari secara terus dengan mata kasar, binokular atau teleskop, hanya apabila fotosfera Matahari benar-benar dilindungi seluruhnya oleh Bulan. Dalam tempoh ini, matahari adalah terlalu malap untuk dilihat melalui penuras. [[Korona]] malap Matahari akan dapat dilihat, dan [[kromosfera]], [[semarak suria]], dan mungkin juga [[suar suria]] boleh dilihat. Walau bagaimanapun, melihat Matahari selepas kepenuhan boleh membahayakan. ▲[[Fail:TheSun beads.jpg\|thumb\|[[~~Baily's~~Manik ~~beads~~Baily]]]] ▲<!-- When the shrinking visible part of the photosphere becomes very small, [[Baily's beads]] will occur. These are caused by the sunlight still being able to reach Earth through lunar valleys, but no longer where mountains are present. Totality then begins with the [[Diamond Ring effect (Solar Eclipse)\|diamond ring effect]], the last bright flash of sunlight.<ref>{{cite web \|author=O. Staiger \|title=The Experience of Totality \|url=http://www.mreclipse.com/Totality/TotalityCh01.html}}</ref>

Gerhana matahari: Perbezaan antara semakan