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This page describes an image A Coronal Mass Ejection

تنزيل الملف ( صورة 596.22 kB)

شرح الصورة: A burst of solar material can be seen erupting from the Sun in this view, illustrating a coronal mass ejection (CME)—a large eruption of plasma and magnetic field from the Sun’s outer atmosphere, or corona. These CMEs are caused by magnetic explosions in the Sun's corona. During a CME, huge amounts of electrically charged particles are launched into space at great speeds, carrying part of the Sun’s magnetic field with them. These events are driven by changes in the Sun’s magnetic structure and release vast clouds of hot gas that travel outward into the solar system. When a CME moves through space, it can interact with a planet’s magnetic field and atmosphere, sometimes creating spectacular auroras or, in strong cases, interfering with artificial satellites and power systems.

CMEs are often associated with a temporary brightening of the region of the Sun where the CME originated. This is known as a solar flare. Stars other than the Sun can also have CMEs and flares.

This image was taken by NASA's Solar Dynamics Observatory (SDO). This is a space mission to monitor the Sun. The image here is taken at a special wavelength which partially ionised helium emits strongly at.
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مصدر الصورة: NASA/Goddard/SDO رابط المصدر

مصطلحات معجم ذات صلة: الشمس , قذف الكتلة الإكليلي (CME)

ترخيص الصورة: الملكية العامة الملكية العامة أيقونات

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".

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الإنجليزيّة
شرح الصورة: A burst of solar material can be seen erupting from the Sun in this view, illustrating a coronal mass ejection (CME)—a large eruption of plasma and magnetic field from the Sun’s outer atmosphere, or corona. These CMEs are caused by magnetic explosions in the Sun's corona. During a CME, huge amounts of electrically charged particles are launched into space at great speeds, carrying part of the Sun’s magnetic field with them. These events are driven by changes in the Sun’s magnetic structure and release vast clouds of hot gas that travel outward into the solar system. When a CME moves through space, it can interact with a planet’s magnetic field and atmosphere, sometimes creating spectacular auroras or, in strong cases, interfering with artificial satellites and power systems.

CMEs are often associated with a temporary brightening of the region of the Sun where the CME originated. This is known as a solar flare. Stars other than the Sun can also have CMEs and flares.

This image was taken by NASA's Solar Dynamics Observatory (SDO). This is a space mission to monitor the Sun. The image here is taken at a special wavelength which partially ionised helium emits strongly at.
مصدر الصورة: NASA/Goddard/SDO
مصطلحات معجم ذات صلة: Coronal Mass Ejection (CME) , Sun