| Jun 02, 2020 |
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(Nanowerk News) The Sun is the brightest object in the sky and has been studied for hundreds of years, but it continues to hide some secrets. We all know that the visible Sun is extremely hot, at temperature of about 5500 degrees.
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Surprisingly, on top of this sits a layer of gas, called the corona, which is at a temperature of almost 2 million degrees, over 300 times hotter than the surface of the Sun! What heats up the corona to 2 million degrees is one of the most challenging puzzles about the Sun and no one found a satisfactory answer to this until date.
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One efficient way of extracting this energy from the magnetic fields involves numerous tiny explosions taking place all over the Sun, all the time. Individually these explosions are too weak, but collectively they have sufficient energy to heat the entire corona due to sheer numbers.
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Many attempts have been made to look for X-rays and ultraviolet light emitted by these explosions and none has been successful. It was concluded that if they exist, these tiny explosions are too weak to be detected by even the best instruments available today.
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These explosions also expected to give rise to tiny flashes of radio lights, but till now there were no telescopes sensitive enough to detect them. This work reports the first ever detection of these flashes.
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A group of scientists working at the National Centre for Radio Astrophysics (NCRA), a part of the Tata Institute of Fundamental Research, has recently discovered tiny flashes of radio light from all over the Sun. They have identified these as the smoking guns for small magnetic explosions. These are the first ever evidence for their existence and can potentially explain the long-standing coronal heating problem. |
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This work was led by Surajit Mondal, under the supervision of Prof. Divya Oberoi, along with Dr. Atul Mohan, formerly at NCRA, and now at the Rosseland Centre for Solar Physics, Norway. In their journey to unravel this mystery, scientists have already figured out that the extra energy heating up the corona must be coming from the solar magnetic fields, but exactly how this happens is still not known.
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“What made this breakthrough possible,” said Prof. Divya Oberoi, “is the availability of data from a new technology instrument, the Murchison Widefield Array (MWA), and the work which we have been doing for the past few years at NCRA-TIFR to build the techniques and tools to make the most sensitive solar radio images from this data. The very weak radio flashes we have discovered are about 100 times weaker than the weakest bursts reported till now.”
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Surajit Mondal, the lead author of this work (The Astrophysical Journal Letters, “First Radio Evidence for Impulsive Heating Contribution to the Quiet Solar Corona”) said, “What makes this really exciting is that these flashes are present everywhere on the Sun and at all times, including in the regions of weak magnetic fields, the so-called ‘quiet Sun’ regions.”
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Dr. Atul Mohan added that, “Our preliminary estimates suggest that these tiny magnetic explosions should collectively have enough energy to heat the corona, which is exactly what is needed for solving the coronal heating problem.”
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