A bubbling ball of gas (w/ Video)
November 11, 2009
The IMaX instrument not only depicts the solar surface, it also makes magnetic fields visible; these appear as black or white structures in the polarised light. SUNRISE enables tiny magnetic fields on the surface of the Sun to be measured at a level of detail never before achieved. Credit: Image: MPS/IMAX consortium
The Sun is a bubbling mass. Packages of gas rise and sink, lending the sun its grainy surface structure, its granulation. Dark spots appear and disappear, clouds of matter dart up - and behind the whole thing are the magnetic fields, the engines of it all. The SUNRISE balloon-borne telescope, a collaborative project between the Max Planck Institute for Solar System Research in Katlenburg-Lindau and partners in Germany, Spain and the USA, has now delivered images that show the complex interplay on the solar surface to a level of detail never before achieved.
The largest solar telescope ever to have left Earth was launched from the ESRANGE Space Centre in Kiruna, northern Sweden, on June 8, 2009. The total equipment weighed in at more than six tons on launch. Carried by a gigantic helium balloon with a capacity of a million cubic metres and a diameter of around 130 metres, SUNRISE reached a cruising altitude of 37 kilometres above the Earth's surface.
FLV player
This video shows the surface of the sun in close up. Credit: Max Planck Institute for Solar System Research
The observation conditions in this layer of the atmosphere, known as the stratosphere, are similar to those in outer space: for one thing, the images are no longer affected by air turbulence; and for another, the camera can also zoom in on the Sun in ultraviolet light, which would otherwise be absorbed by the ozone layer. After separating from the balloon, SUNRISE parachuted safely down to Earth on June 14th, landing on Somerset Island, a large island in Canada's Nunavut Territory situated in the Northwest Passage, the seaway through the Arctic Ocean between the Atlantic and the Pacific.The work of analysing the total of 1.8 terabytes of observation data recorded by the telescope during its five-day flight has only just begun. Yet the first findings already give a promising indication that the mission will bring our understanding of the Sun and its activity a great leap forward. What is particularly interesting is the connection between the strength of the magnetic field and the brightness of tiny magnetic structures. Since the magnetic field varies in an eleven-year cycle of activity, the increased presence of these foundational elements brings a rise in overall solar brightness - resulting in greater heat input to the Earth.
The variations in solar radiation are particularly pronounced in ultraviolet light. This light does not reach the surface of the Earth; the ozone layer absorbs and is warmed by it. During its flight through the stratosphere, SUNRISE carried out the first ever study of the bright magnetic structures on the solar surface in this important spectral range with a wavelength of between 200 and 400 nanometres (millionths of a millimetre).
Grainy sun: the images show the so-called granulation in four different wavelengths in near ultraviolet light. The image section depicts 1/20,000 of the entire surface. The smallest recognisable structures have an angular resolution equal to that of looking at a coin from a distance of 100 kilometres. The light structures are the foundational elements of the magnetic fields. Credit: Image: MPI for Solar System Research
"Thanks to its excellent optical quality, the SUFI instrument was able to depict the very small magnetic structures with high intensity contrast, while the IMaX instrument simultaneously recorded the magnetic field and the flow velocity of the hot gas in these structures and their environment," says Dr. Achim Gandorfer, project scientist for SUNRISE at the Max Planck Institute for Solar System Research.Previously, the observed physical processes could only be simulated with complex computer models. "Thanks to SUNRISE, these models can now be placed on a solid experimental basis," explains Prof. Manfred Schüssler, solar scientist at the MPS and co-founder of the mission.
Source: Max-Planck-Gesellschaft (news : web)
Oct 23, 2007 |
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At those temperatures, that 'gas' is ionized- a plasma. It is obeying Maxwell's Laws, not thermodynamic ones.
It also explains the patently obvious cellular structure appearance- hence why the 1st state of matter was dubbed 'plasma' to begin with- it very strongly resembles blood plasma.
I can state with some conviction, that I do not see a single 'bubble' in any of those graphics...
BTW- if those are magnetic fields surrounding plasma, where do they suppose the electric currents are flowing? They MUST be there after all- unless Maxwell's Laws have been repealed?
I smell a paradigm shift in the wind... ;)
Mike H.
They mentioned the resolution as being like a coin seen at 100 km. I assumed the coin was one cm, and that works out to a resolution of roughly 0.1 arc second, a nice telescope indeed! That makes the Hubble only twice as good! Not bad for a scope dangling from a helium balloon! And the fact it survived recovery sounds like a sequel is in the works!
That is not the behavior that one would expect of plasma. The sun is mostly a plasma since it is mostly ionized. There would be no bubbles rising and falling from gravity.. There would be structures probably in the shape of a toroid around the equator under the surface from the plasma flows, creating an electric current.
The sun spots and photosphere granulation are the result of columns of plasma flows. Same phenomena that you see on the surface of a electrode in a thin plasma. This is definitely not a fluid flow especially at the "surface" of the sun. You notice how everything generally goes outward and heats up. This leads on to posit that (using the simplest mechanism for ion acceleration) there is an electric field present.