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EI2GYB > ASTRO 26.08.21 13:31l 89 Lines 4819 Bytes #999 (0) @ WW
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Subj: Researchers solve 20-year-old paradox in solar physics
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Researchers solve 20-year-old paradox in solar physics
In 1998, the journal Nature published a seminal letter concluding that a
mysterious signal, which had been discovered while analyzing the
polarization of sunlight, implies that the solar chromosphere
(an important layer of the solar atmosphere) is practically
unmagnetised, in sharp contradiction with common wisdom.
This paradox motivated laboratory experiments and theoretical
investigations, which instead of providing a solution, raised new
issues, and even led some scientists to question the quantum theory
of matter-radiation interaction.
Today, researchers at the Istituto Ricerche Solari (IRSOL) in
Locarno-Monti (affiliated to USI Universit… della Svizzera italiana),
and the Instituto de Astrofˇsica de Canarias (IAC) in Tenerife,
have found the solution to this intriguing paradox, opening up a new
window for exploring the elusive magnetic fields of the solar chromosphere
in the present new era of large-aperture solar telescopes.
Their findings are published in Physical Review Letters.
Twenty-five years ago, an enigmatic signal was discovered while analyzing
the polarization of sunlight with a new instrument, the Zurich Imaging
Polarimeter (ZIMPOL), developed at ETH Zurich and later installed at IRSOL.
This mysterious linear polarization signal, produced by scattering
processes, appears at the wavelength of a neutral sodium line
(the so-called D1 line), where, according to quantum mechanics, no such
scattering polarization should be present.
This signal was therefore totally unexpected, and its interpretation
immediately opened an intense scientific debate.
The mystery further increased two years later, when the journal Nature
published an explanation implying that the layer of the solar atmosphere
known as the chromosphere is completely unmagnetised, in apparent
contradiction with established results; researchers believed that
(outside sunspots) this region is permeated by magnetic fields in the gauss
range. The new findings opened a serious paradox that has challenged solar
physicists for many years, and even led some scientists to question the
available quantum theory of matter-radiation interaction.
Now, in an article published by Physical Review Letters, Ernest Alsina
Ballester (IRSOL, IAC), Luca Belluzzi (IRSOL), and Javier Trujillo Bueno (IAC)
show the solution to this intriguing paradox.
The findings were achieved by carrying out the most advanced theoretical
modeling of the solar D1 line polarization ever attempted,
involving three years of work carried out through a close cooperation
between the Istituto Ricerche Solari (IRSOL) in Locarno-Monti
(affiliated to USI Universit… della Svizzera italiana) and the POLMAG
group of the Instituto de Astrofˇsica de Canarias (IAC) in Tenerife.
The researchers explain: "This result has very important consequences.
Scattering polarization signals, like the one observed in the D1
line of sodium, are extremely interesting because they encode unique
information on the elusive magnetic fields present in the solar chromosphere.
This key interface layer of the solar atmosphere, located between the
underlying cooler photosphere and the overlying million-degree corona,
is at the core of several enduring problems in solar physics, including
the understanding and prediction of the eruptive phenomena that may strongly
impact our technology-dependent society.
The magnetic field is known to be the main driver of the spectacular
dynamical activity of the solar chromosphere, but our empirical knowledge
of its intensity and geometry is still largely unsatisfactory.
The solution of the long-standing paradox of solar D1 line polarization
proves the validity of the present quantum theory of spectral line
polarization, and opens up a new window to explore the magnetism of
the solar atmosphere in the present new era of large-aperture solar
telescopes."
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