|Corona from Svalbard composed of 29 eclipse images. © 2015 Miloslav Druckmüller, Shadia Habbal, Peter Aniol, Pavel Starha.
The international Solar Wind Sherpas team, led by Dr. Shadia Habbal of the University of Hawaii at Manoa Institute for Astronomy, braved Arctic weather to successfully observe the total solar eclipse of March 20 from Longyearbyen on the island of Spitsbergen in the Svalbard archipelago east of northern Greenland. Their preliminary results are being presented Thursday at the Triennial Earth-Sun Summit in Indianapolis, IN.
It was no easy feat. Ever-changing weather predictions, subfreezing temperatures of –4 degrees F (–20 C) and the danger from polar bears were some of the challenges the team faced, but their years of preparation paid off. The sky over the snow-covered landscape was crystal clear before, during and after totality, so they were able to capture a beautiful solar corona.
Because the Svalbard archipelago, like the Hawaiian Islands, has microclimates, the team observed at two locations to increase its chances of seeing the eclipse. With local support, the team was able to set up its equipment inside the old Northern Light Observatory and observe the event through specially designed doors that replaced the old windows, and to use an airport hangar located 10 miles away.
Identical sets of imaging instruments were set up at both locations, with six digital SLR cameras fitted with different focal length lenses, and four astrophotography cameras with special filters to observe the colors of light given off by ionized iron atoms, stripped of 10 and 13 electrons. These highly ionized atoms probe the high temperature outer layers, or corona, of the sun. In addition, a special instrument, called a dual-channel imaging spectrograph was used at the observatory to measure the motions of these ions in the sun’s corona. At the airport, Dr. Haosheng Lin (IfA) used a spectropolarimeter that he designed and constructed to measure the sun’s magnetic fields.
The shadow bands, thin bands of light and dark observed prior to and during totality, were remarkable as the snow-covered landscape offered ideal conditions for seeing them. The corona of the eclipsed sun, which was at an altitude of 12 degrees, was shimmering throughout the 2 minutes and 20 seconds of totality, with one large prominence clearly visible to the naked eye.
To further maximize the likelihood of observing the corona during this eclipse, the other members of the Solar Wind Sherpas team observed from three other sites: the Faroe Islands, located between Iceland and Norway; a Falcon Dassault flying at 49,000 feet (15,000 m) over the Faroe Islands, and an Irish Air Corps CASA CN235 flying out of Dublin. All were successful except for the group on the Faroe Islands, where rain prevented them from observing totality.
Members of the team are currently working on the calibration and analysis of the data and will be presenting preliminary results at the upcoming Triennial Earth-Sun Summit (TESS) meeting in Indianapolis. Their results will be published once the analysis is completed.
The 2015 members of the Solar Wind Sherpas and their respective institutions and corporations are Shadia Habbal, Haosheng Lin and Garry Nitta, Institute for Astronomy, University of Hawaii at Manoa; Adalbert Ding, Technische Universitat and Institute for Technical Physics, Berlin; Judd Johnson, Electricon, Boulder, Colorado; Miloslav Druckmüller, Pavel Starha, Jana Hoderova and Jan Malec, Brno University of Technology, Czech Republic; Petr Starha, Brno, Czech Republic; Peter Aniol, Astelco Corporation, Germany; Martin Dietzel, Zeiss Corporation, Germany; Feras Habbal, University of Texas, Austin; Yaseen Almleaky, King Abdullah University, Saudi Arabia; Huw Morgan, Duraid Al-Shakarshi, Nathalia Alzate and Joe Hutton, Aberystwyth University, Wales; Martina Arndt, Bridgewater State University, Massachusetts; and Scott Gregoire Granite Mountain Research, Boulder. In addition, Peter Gallagher of Trinity College, Dublin, was instrumental in securing the CASA CN235 flight. He and Joe McCauley were involved in setting up the equipment and acquiring the observations from that platform. The Northern Light Observatory was made available by the director of University Centre in Svalbard, Prof. Fred Sigernes, and Dr. Sebastian Sikora. The airport hangar was made available by airport manager Morten Ulsnes.
The dual-channel imaging spectrograph was designed and constructed by Prof. Adalbert Ding (Technische Universitat and Institute for Technical Physics, Berlin).
Financial support for the eclipse expedition was provided by NSF grants AGS-1144913, AGS-1255894 and AGS-1358239, and NASA grant NNX13AG11G to the University of Hawaii. Additional support was provided by King Abdullah University and Astelco Corporation.
Svalbard. Photo by Dr. Miloslav Druckmüller. 3.7 Mb JPEG
Eclipse over Svalbard. Photo by Dr. Miloslav Druckmüller. 3.1 Mb JPEG
Equipment setup at the airport by members of the Solar Wind Sherpas (from the left) Peter Aniol, Pavel Starha, and Haosheng Lin. Photo
by Dr. Miloslav Druckmüller. 4.5 Mb JPEG
The solar eclipse of March 20 showing what the corona looks like in the colors of light given off by ionized iron atoms stripped of 13 electrons. Image
by Solar Wind Sherpas. 177 kb JPG
The solar eclipse of March 20 showing what the corona looks like in the colors of light given off by ionized iron atoms stripped of 10 electrons. Image
by Solar Wind Sherpas. 104 kb JPEG
Spectrum of the iron stripped of 13 electrons showing large mass motions. It was taken with the dual-channel spectrograph developed by Adalbert Ding. Image by Adalbert Ding. 1.9 Mb JPEG
Permission is given to use these illustrations, including the one at the top of the page, to illustrate an article about the subject of this press release.
Founded in 1967, the Institute for Astronomy at the University of Hawaii at Manoa conducts
research into galaxies, cosmology, stars, planets, and the
sun. Its faculty and staff are also involved in astronomy education,
deep space missions, and in the development and management
of the observatories on Haleakala and Maunakea. The Institute operates facilities on the islands of Oahu, Maui, and Hawaii.