You are seeing Ask web results for coronal mass ejection.
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Coronal mass ejection - Wikipedia, the free encyclopedia
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Coronal Mass Ejections ... Coronal mass ejections (or CMEs) are huge bubbles of gas threaded with magnetic field lines that are ejected from the Sun over the course of several hours. ... Coronal Mass Ejection Web Links...
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Cosmicopia at NASA/GSFC - Sun - Solar Activity - Coronal Mass Ejections ... MSU Coronal Mass Ejection FAQs; Back to Solar Activity; ... May 27, 2008: Cartwheel coronal mass ejection -- Science@NASA; January 21, 2008: Ring around the Sun -- NASA HEAPOW; November 26, 2007: Outburst pulls magnetic slingshot --
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Coronal Mass Ejection Prediction Page ... Coronal mass ejection (CME) is the name given to an ejection of a large amount of matter from the Sun's outer atmosphere. These ejections typically comprise millions of tons of material in the form of charged particles, and can be seen because the material reflects sunlight.
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While hints of these explosive events, called coronal mass ejections or CMEs, were discovered by spacecraft in the early 70s this dramatic image is part of a detailed record of this CME's development from the presently operating SOlar and ... Sun Storm: A Coronal Mass Ejection ; Credit: SOHO Consortium, ESA, NASA...
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Coronal mass ejections (CMEs) are eruptions into interplanetary space of as much as a few billion tons of plasma and embedded magnetic fields from the Sun's corona.
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A coronal mass ejection and prominence eruption observed in white light from the SMM (Solar Maximum Mission) spacecraft. The time of each panel increases from left to right. The dashed inner circle in each panel is the solar radius, the occulting radius is at 1.6 solar radii.
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The January 6-11, 1997, Coronal Mass Ejection Event ... The April 7, 1997, Coronal Mass Ejection and Solar Flare ... The above image shows two examples of a coronal mass ejection (CME). The black disk blocks out the bright light from the Sun, creating an artificial eclipse so that the dim light from the CME can be observed.
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This animation shows a "full halo" coronal mass ejection recorded by SOHO coronagraphs on July 14, 2000. The many speckles in the latter half of the movie are energetic particles from a related solar flare bombarding SOHO's electronic detectors.
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