coronal mass ejections (CMEs) tagged posts

Superflare with Massive, High-Velocity Prominence Eruption

Artist’s impression of the superflare observed on one of the stars in the V1355 Orionis binary star system. The binary companion star is visible in the background on the right. (Credit: NAOJ) 

A team of Japanese astronomers used simultaneous ground-based and space-based observations to capture a more complete picture of a superflare on a star. The observed flare started with a very massive, high-velocity prominence eruption. These results give us a better idea of how superflares and stellar prominence eruptions occur.

Some stars have been seen releasing superflares over 10 times larger than the largest solar flare ever seen on the Sun. The hot ionized gas released by solar flares can influence the environment around the Earth, referred to as space weather...

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NASA Protects its Super Heroes from Space Weather

NASA's Human Research Program aims to mitigate the harmful effects of the space radiation environment on astronaut health outside of the relative protection of the Earth's magnetosphere. Credit: NASA/SOHO

NASA’s Human Research Program aims to mitigate the harmful effects of the space radiation environment on astronaut health outside of the relative protection of the Earth’s magnetosphere. Credit: NASA/SOHO

NASA’s Human Research Program (HRP) is studying the effects radiation plays on the human body and developing ways to monitor and protect against this silent hazard. High-energy galactic cosmic rays (GCRs) which are remnants from supernovas and solar storms like solar particle events (SPEs) and coronal mass ejections (CMEs) from the sun can cause harm to the body and spacecraft. These are all components of space weather

“Dosimeters and modeling techniques are used to determine how much energy is deposited in the space explorer’s bodies along with inflight tools to try to estimate what type...

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Under pressure: Extreme Atmosphere Stripping may Limit Exoplanets’ Habitability

Under pressure -- Extreme atmosphere stripping may limit exoplanets' habitability

Artist’s impression of HD189733b, showing the planet’s atmosphere being stripped by the radiation from its parent star. Credit: Ron Miller

New models of massive stellar eruptions hint at an extra layer of complexity when considering whether an exoplanet may be habitable or not. Models developed for our own Sun have now been applied to cool stars favoured by exoplanet hunters, in research presented by Dr Christina Kay, of the NASA Goddard Flight Center, on Monday 3rd July at the National Astronomy Meeting at the University of Hull.

Coronal mass ejections (CMEs) are huge explosions of plasma and magnetic field that routinely erupt from the Sun and other stars...

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Sun Eruptions hit Earth like a ‘Sneeze’, say scientists

M.J. Owens, M. Lockwood and L.A. Barnard (2017). ‘Coronal mass ejections are not coherent magnetohydrodynamic structures’. Nature Scientific Reports. Doi: 10.1038/s41598-017-04546-3

M.J. Owens, M. Lockwood and L.A. Barnard (2017). ‘Coronal mass ejections are not coherent magnetohydrodynamic structures’. Nature Scientific Reports. Doi: 10.1038/s41598-017-04546-3

Long-term power cuts, destruction of electronic devices and increased cancer risk for aeroplane passengers are all potential effects of the Earth being hit by a powerful solar eruption. Yet, new research has found space scientists have their work cut out to predict when these coronal mass ejections (CMEs) are on a collision course with Earth.

A study of CMEs by scientists at the University of Reading has found they have cloud-like structures...

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