The interesting observation & measurement in the report posted by TalonThorn is this quote:
The long-sought clue to prediction lies in changes in twisting magnetic fields beneath the surface of the sun in the days leading up to a flare, according to the authors.
So, beneath the surface of the Sun there are "twisting magnetic fields" leading up to a flare, also called a Coronal Mass Ejection (CME).
Well, also, it has been observed & measured that once CME's have been ejected out into the heliosphere as part of the solar wind (a charged particle plasma flow) have the shape of a "croissant". Obviously, the French pastry has a twist and this twisted shape owes to the CME's magnetic field.
As reported by NASA: The Surprising Shape of Solar Storms (see link below):
http://science.nasa.gov/headlines/y2009/14apr_3dcme.htmApril 14, 2009: This just in: The Sun is blasting the solar system with croissants.
Researchers studying data from NASA's twin STEREO probes have found that ferocious solar storms called CMEs (coronal mass ejections) are shaped like a French pastry. The elegance and simplicity of the new "croissant model" is expected to dramatically improve forecasts of severe space weather.
Coronal mass ejections are billion-ton clouds of hot magnetized gas [plasma] that explode away from the sun at speeds topping a million mph. Sometimes the clouds make a beeline for Earth and when they hit they can cause geomagnetic storms, satellite outages, auroras, and power blackouts. The ability to predict the speed and trajectory of a CME is key to space weather forecasting.
"This is an important advance," says Lika Guhathakurta, STEREO program scientist at NASA headquarters in Washington DC. From a distance, CMEs appear to be a complicated and varied population. Almost all of the 40-plus CMEs we have studied so far with STEREO have a common shape--akin to a croissant."
Vourlidas says he is not surprised that CMEs resemble French pastries. "I have suspected this all along. The croissant shape is a natural result of twisted magnetic fields on the sun..."
"That's how CMEs get started—as twisted ropes of solar magnetism. When the energy in the twist reaches some threshold, there is an explosion [exploding double layers?] which expels the CME away from the sun. It looks like a croissant because the twisted ropes are fat in the middle and thin on the ends."
But there is more that NASA researchers want to find out:
The shape alone, however, does not tell the full story of a CME. The contents of the CME must be considered, too. How much plasma does it contain? What is the orientation and strength of its internal magnetic field? When a CME strikes, the havoc it causes will depend on the answers—answers the croissant model does not yet provide.
"There is more work to do. We must learn to look at a CME and not only trace its shape, but also inventory in contents," says Guhathakurta. "We are halfway there."
So, from below the surface of the Sun and continuing far from the Sun's surface "twisted magnetic fields" are observed & measured.
Interesting...
