Monday, January 26, 2015

The discovery of the British scientists are likely to illuminate for other stars as well as the mec


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London, Tuesday (MTI), 5 February batas 2013 - British scientists have found an explanation for decades mystery of why the sun is hotter crown as the surface: a perception that the energy required batas for magnetic hydrodynamic (MHD) waves are delivered inside a star outer layers of the atmosphere.
Three UK - the Northumbria, batas Sheffield and Belfast - University researchers led by Richard Morton, a proprietary, high-resolution imaging telescope (Rapid Oscillation in the Solar Atmosphere batas / ROSA) very sharp photos could make the sun kromoszférájáról. They formed a picture using magnetic hydrodynamic batas waves of speed and strength of the basis of the information obtained and were able to calculate how much energy is transmitted from the solar surface of the crown.
The news website ScienceDaily was reported that the calculations confirmed that certainly in the MHD waves are responsible for ensuring that the Sun's surface six thousand degrees Celsius multiplied a million degrees flat can be heated in the gas layer above it.
"Our observations allowed us to estimate the amount of energy delivered by the MHD waves and on the basis of the data obtained, it became clear that it is entirely energy waves satisfy batas the extremely high temperature rise of the Sun's corona causing energy needs" - said Morton, explaining serving the phenomenon previously considered mysterious .
The discovery of the British scientists are likely to illuminate for other stars as well as the mechanism by which crowns can be hundreds of times hotter than fotoszférájuk - the region where the light is generated - even though much further away from the heat source, the star of the inner core.
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