By Megan GannonPublished July 29, 2013
Space.com
The European Space Agency/NASA Solar and Heliospheric Observatory, or SOHO, captured this image of a gigantic coronal hole hovering over the sun’s north pole on July 18, 2013, at 9:06 a.m. EDT. (ESA&NASA/SOHO)
A space telescope aimed at the sun has spotted a gigantic hole in the solar atmosphere — a dark spot that covers nearly a quarter of our closest star, spewing solar material and gas into space.
The so-called coronal hole over the sun's north pole came into view between July 13 and 18 and was observed by the Solar and Heliospheric Observatory, or SOHO. NASA released a video of the sun hole as seen by the SOHO spacecraft, showing the region as a vast dark spot surrounded by solar activity.
Coronal holes are darker, cooler regions of the sun's atmosphere, or corona, containing little solar material. In these gaps, magnetic field lines whip out into the solar wind rather than looping back to the sun's surface. Coronal holes can affect space weather, as they send solar particles streaming off the sun about three times faster than the slower wind unleashed elsewhere from the sun's atmosphere, according to a description from NASA.
"While it’s unclear what causes coronal holes, they correlate to areas on the sun where magnetic fields soar up and away, failing to loop back down to the surface, as they do elsewhere," NASA's Karen Fox at the agency's Goddard Space Flight Center in Greenbelt, Md., explained in an image description.
These holes are not uncommon, but their frequency changes with the solar activity cycle. The sun is currently reaching its 11-year peak in activity, known as the solar maximum. Around the time of this peak, the sun's poles switch their magnetism. The number of coronal holes typically decreases leading up to the switch.
After the reversal, new coronal holes appear near the poles. Then as the sun approaches the solar minimum again, the holes creep closer to the equator, growing in both size and number, according to NASA.
The $1.27-billion SOHO satellite was launched in 1995 and is flying a joint mission between NASA and the European Space Agency (ESA). It watches solar activity from an orbit about the Lagrange Point 1, a gravitationally stable spot between Earth and the sun that is about 932,000 miles from our planet.
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While magnetic field lines are invisible, they force charged particles of plasma along their lengths, making them visible in images. Space telescopes pick up the lines as they arch and move along the frame of the lens. Su observed two bundles of lines move towards each other and then disconnect and reconnect.
The video offers scientists an entirely new resource since it allows them to see the phenomena in recorded time and animated, as opposed to simple photos that only offer an indication of what is happening. The team, led by Su, turned to the Reuven Ramaty High Energy Solar Spectroscopic Imager, known as RHESSI, to confirm that they were actually observing magnetic reconnection in action. RHESSI shows where hot pockets are, indicating where space weather is occurring. By combining the data, scientists were able to describe the entire process of magnetic reconnection, confirming many theories about the process as well as learning new information that they were able to observe for the first time.
Magnetic reconnection does not only occur on the surface of the sun, it also occurs near stars and within Earth’s own magnetic field, making it a key player in space weather patterns.