Exploring the Sun via helium balloon almost sounds like an adventure for an animated movie, but the SUNRISE balloon-borne telescope has captured data and images that show the complex interplay on the solar surface to a level of detail never before achieved. As in the video above, SUNRISE shows our local star to be a bubbling, boiling mass where packages of gas rise and sink, lending the sun its grainy surface structure. Dark spots appear and disappear, clouds of matter dart up – and behind the whole thing are the magnetic fields, the engines of it all.
“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,” said 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,” said Manfred Schüssler, co-founder of the mission.
SUNRISE is the largest solar telescope ever to have left Earth. It 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 meters and a diameter of around 130 meters, SUNRISE reached a cruising altitude of 37 kilometers above the Earth’s surface.
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In the stratosphere, observational conditions are similar to those in outer space. The images are no longer affected by air turbulence, and the camera can also zoom in on the Sun in ultraviolet light, which would otherwise be absorbed by the ozone layer. After making its observations, SUNRISE separated from the balloon, and parachuted safely down to Earth on June 14th, landing on Somerset Island, a large island in Canada’s Nunavut Territory.
The work of analyzing 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 nanometers (millionths of a millimeter).
SUNRISE is a collaborative project between the Max Planck Institute for Solar System Research in Katlenburg-Lindau, with partners in Germany, Spain and the USA.