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Michael Mozina
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I'm trying to ascertain if there is any "consensus" on the cause of coronal loops in current theory?
Magnetic fields.Michael Mozina said:I'm trying to ascertain if there is any "consensus" on the cause of coronal loops in current theory?
Garth said:Magnetic fields.
Garth
Garth said:The corona is a plasma of fast following ions constrained by magnetic fields, of course there are electric currents - its astrophysical MHD.
Garth
Garth said:The corona is a plasma of fast following ions constrained by magnetic fields, of course there are electric currents - its astrophysical MHD.
Garth
You might find this paper useful http://scitation.aip.org/getpdf/servlet/GetPDFServlet?filetype=pdf&id=PHPAEN000001000005001684000001&idtype=cvips&prog=normalMichael Mozina said:This brings me back to one issue that seems to be in considerable dispute.
If these are MHD loops, where do they originate? Do they begin below the photosophere or do they originate higher in the solar atmosphere?
Fresh magnetic fluxes are continually injected into the low corona from below by the solar dynamo. Flaring activities are obviously the hydromagnetic and plasma responses of the corona to this flux injection, although the nature of these complex processes are not understood well.’ Observation suggests that a significant part of the emergent magnetic flux is in the form of lines of force with the two ends anchored in the dense photosphere. Hence, the magnetic field in the corona continues to be energized by the photosphere through the turbulent transport ( ~1/2 km/s) of the magnetic footpoints. This is the basis for the popular notion that magnetic energy can build up on a time scale long compared to the typical coronal Alfven transit time of the order of minutes, to be released in spurts of 1031-32 ergs as sporadic flares.
Astronuc said:Thanks for that paper, Garth!
The MHD effect is primarily IxB and plasma waves. One may wish to look into plasma instabilities.
Also - NASA is redoing websites, including Goddard's. Links from other sites outside NASA might become invalid.
http://www.nasa.gov/centers/goddard/2004solar.html
Nereid said:How do these images "show the coronal loops originating underneath the photosphere and coming through the photosphere ..." (my bold)?
Observation suggests that a significant part of the emergent magnetic flux is in the form of lines of force with the two ends anchored in the dense photosphere. Hence, the magnetic field in the corona continues to be energized by the photosphere through the turbulent transport ( -$ km s-i) of the magnetic footpoints.
I mean, by definition, isn't the photosphere the zone on the Sun beneath which images cannot be obtained (from Earth), because the mean free path of (optical, NIR, UV) photons is small?
Garth said:You might find this paper useful http://scitation.aip.org/getpdf/servlet/GetPDFServlet?filetype=pdf&id=PHPAEN000001000005001684000001&idtype=cvips&prog=normal
Or if you want a picture from APOD Heating Coronal Loops.
Yes, there is discussion and new evidence encourages new ideas to be properly tried and tested.
Garth
The steepening to a tangential discontinuity leads to its resistive dissipation, despite the high conductivity. Thus a small part of the built-up energy goes to heat the corona. This is a remarkable process in which high conductivity itself promotes resistive dissipation. Coronal
heating is a central problem that is far from resolved, observationally and theoretically
Garth said:The problem of heating the corona, and coronal loops within it, has not been solved although there are two main suggested processes that might be responsible: wave energy or magnetic reconnection.
The waves might be sound waves, magneto-acoustic waves or Alfven waves.
The energy in the coronal loops is enormous, but as the corona is very tenuous it needs only a small amount of energy to heat it to high temperature, about 1 Kw/metre2 of the Sun's surface area, or about 0.000016% of the total solar energy emitted.
Garth said:Magnetic fields.
Garth
Coronal loops are structures of hot, ionized gas found in the Sun's corona. They are shaped like loops or arches and are often observed near sunspots.
The exact cause of coronal loops is not fully understood, but they are believed to be formed by magnetic field lines that are twisted and tangled due to the Sun's rotation and convection. This creates areas of concentrated energy that can heat up the surrounding gas and form the loops.
Coronal loops play a crucial role in the dynamics and activity of the Sun. They are associated with solar flares and coronal mass ejections, which can have significant impacts on Earth's space weather and technological systems. Studying coronal loops can help us better understand and predict these events.
Coronal loops are primarily observed using instruments on space-based telescopes such as the Solar Dynamics Observatory and the Solar and Heliospheric Observatory. These instruments can capture images and data in different wavelengths of light, allowing scientists to study the temperature and structure of the loops.
Yes, coronal loops have been observed on other stars similar to the Sun. However, they may appear different in size and shape due to variations in the strength and structure of magnetic fields on different stars.