NASA's Solar Dynamics Observatory Catches "Surfer" Waves on the Sun
Cue the surfing music. Scientists have spotted the iconic surfer's wave rolling through the atmosphere of the sun. This makes for more than just a nice photo-op: the waves hold clues as to how energy moves through that atmosphere, known as the corona. Read more
W. Dean Pesnell of the NASA Solar Dynamics Observatory presents an illustrated lecture on new observations and views of solar phenomena.
Speaker Biography: W. Dean Pesnell has published 80 papers in several research areas, including variable stars, the sun-earth connection, quantum mechanics and meteors in planetary atmospheres. He received his doctorate in 1983 from the University of Florida. After postdoctoral study at the University of Colorado and a visiting professorship at New Mexico State University, Pesnell came to NASA Goddard as a contractor in 1990. One project was to design the Living With a Star geospace missions. He started work on NASA's Solar Dynamics Observatory mission in 2004 and became the project scientist in 2005.
Title: Faint young Sun paradox remains Authors: Colin Goldlatt, Kevin J. Zahnle
The Sun was fainter when the Earth was young, but the climate was generally at least as warm as today; this is known as the 'faint young Sun paradox'. Rosing et al. [1] claim that the paradox can be resolved by making the early Earth's clouds and surface less reflective. We show that, even with the strongest plausible assumptions, reducing cloud and surface albedos falls short by a factor of two of resolving the paradox. A temperate Archean climate cannot be reconciled with the low level of CO2 suggested by Rosing et al. [1]; a stronger greenhouse effect is needed.
Nasa is working with the University of Central Lancashire (UCLan) to unravel the mysteries of the Sun in unprecedented detail by watching its magnetic field and corona See more
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Taking advantage of a relatively new technology, the daguerreotype, French physicists Louis Fizeau and Leon Foucault made the first successful photographs of the sun on April 2, 1845. Read more
Researchers Crack the Mystery of the Missing Sunspots
In 2008-2009, sunspots almost completely disappeared for two years. Solar activity dropped to hundred-year lows; Earth's upper atmosphere cooled and collapsed; the sun's magnetic field weakened, allowing cosmic rays to penetrate the Solar System in record numbers. It was a big event, and solar physicists openly wondered, where have all the sunspots gone? Read more
Scientists say they are closer to understanding why the Sun's outer atmosphere is hotter than its surface. The corona, as it is known, is millions of degrees hotter than the star's visible surface layer, or photosphere. Two satellites have now identified jets of super-heated gas, called spicules, shooting up from just above the Sun's surface into the outer atmosphere. Researchers tell the journal Science that this process could be what maintains the temperature difference. Read more
It's been a mystery for more than half a century: why, in the short distance from the Sun's surface to its corona, or outer atmosphere, does the temperature leap from a few thousand to a few million degrees? The answer, researchers say, might lie in hot jets of plasma erupting from the Sun's surface.