Loading...
This page describes an image Solar corona
شرح الصورة:
Solar corona composite during the totality of the April 8th, 2024 solar eclipse. Solar prominences are also visible on the right side edge. This image was processed using a Larson-Sekanina-style technique. Multiple exposures ranging from 1/500 second to 4 seconds were stacked and combined with a rotational gradient filter to reveal fine structural detail across the corona's extreme brightness range. This is done because the inner corona saturates at longer exposures, while the outer corona and the Moon are only visible at those same longer exposures. The 4-second exposure was excluded from this image, since only the Moon was captured in this frame.
انتقل إلى الشروح بلغات أخرى
مصدر الصورة: Carolin Liefke
تمّت كتابة وترجمة ومراجعة تسميات ملفات الوسائط المعروضة على موقع OAE من خلال جهد جماعي من قِبل OAE، ومراكز وعُقد OAE، والمنسقين الوطنيين لتعليم الفلك (NAECs)، ومتطوعين آخرين. يمكنك الاطلاع على القائمة الكاملة للجهات المشاركة في مشروع الترجمة هنا. تُنشر جميع تسميات ملفات الوسائط بموجب رخصة Creative Commons CC BY-4.0 ويجب نسبها إلى "IAU OAE". أما ملفات الوسائط نفسها فقد تخضع لتراخيص مختلفة (انظر أعلاه) ويجب نسبها كما هو موضح في قسم "الحقوق".
شروح بلغات مختلفة:
الإنجليزيّة
شرح الصورة: Solar corona composite during the totality of the April 8th, 2024 solar eclipse. Solar prominences are also visible on the right side edge. This image was processed using a Larson-Sekanina-style technique. Multiple exposures ranging from 1/500 second to 4 seconds were stacked and combined with a rotational gradient filter to reveal fine structural detail across the corona's extreme brightness range. This is done because the inner corona saturates at longer exposures, while the outer corona and the Moon are only visible at those same longer exposures. The 4-second exposure was excluded from this image, since only the Moon was captured in this frame.
مصدر الصورة: Carolin Liefke
شرح الصورة: Solar corona composite during the totality of the April 8th, 2024 solar eclipse. Solar prominences are also visible on the right side edge. This image was processed using a Larson-Sekanina-style technique. Multiple exposures ranging from 1/500 second to 4 seconds were stacked and combined with a rotational gradient filter to reveal fine structural detail across the corona's extreme brightness range. This is done because the inner corona saturates at longer exposures, while the outer corona and the Moon are only visible at those same longer exposures. The 4-second exposure was excluded from this image, since only the Moon was captured in this frame.
مصدر الصورة: Carolin Liefke
