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Coronal mass ejections are usually visible in white-light coronagraphs. A coronal mass ejection (CME) is a significant ejection of magnetic field and accompanying plasma mass from the Sun's corona into the heliosphere.
Se denomina eyección de masa coronal o CME (por sus siglas en inglés: Coronal Mass Ejection) a una onda hecha de radiación y viento solar que se desprende del Sol en el periodo llamado Actividad Máxima Solar.
Coronal Mass Ejections. Coronal Mass Ejections (CMEs) are large expulsions of plasma and magnetic field from the Sun’s corona. They can eject billions of tons of coronal material and carry an embedded magnetic field (frozen in flux) that is stronger than the background solar wind interplanetary magnetic field (IMF) strength.
18 de may. de 2024 · Coronal mass ejection (CME), large eruption of magnetized plasma from the Sun’s outer atmosphere, or corona, that propagates outward into interplanetary space. The CME is one of the main transient features of the Sun.
24 de jun. de 2022 · Coronal mass ejections (CMEs) are large expulsions of plasma and magnetic field from the sun's atmosphere — the corona. Compared to solar flares — bursts of electromagnetic radiation that...
Coronal Mass Ejections disrupt the flow of the solar wind and produce disturbances that strike the Earth with sometimes catastrophic results. The Large Angle and Spectrometric Coronagraph on the Solar and Heliospheric Observatory has observed a large number of CMEs.
24 de sept. de 2014 · Unlike the energy and X-rays produced in a solar flare – which can reach Earth at the speed of light in eight minutes – coronal mass ejections are giant clouds of solar material that take one to three days to reach Earth.
