Super Dual Auroral Radar Network
The Super Dual Auroral Radar Network is an international scientific radar network
consisting of 35
high frequency radars located in both the Northern and Southern Hemispheres. SuperDARN radars are primarily used to map high-latitude plasma convection in the F region of the ionosphere, but the radars are also used to study a wider range of geospace phenomena including field aligned currents, magnetic reconnection, geomagnetic storms and substorms, magnetospheric MHD waves, mesospheric winds via meteor ionization trails, and interhemispheric plasma convection asymmetries. The SuperDARN collaboration is composed of radars operated by JHU/APL, Virginia Tech, Dartmouth College, the Geophysical Institute at the University of Alaska Fairbanks, the Institute of Space and Atmospheric Studies at the University of Saskatchewan, the University of Leicester, Lancaster University, La Trobe University, and the Solar-Terrestrial Environment Laboratory at Nagoya University.
History
In the 1970s and 1980s, the Scandinavian Twin Auroral Radar Experiment very high frequency coherent scatter radars were used to study field aligned E region ionospheric irregularities. Using two radars with overlapping fields of view, it was possible to determine the 2D velocity vector of E region ionospheric plasma flow. However, irregularities were only observed when the radar wavevector was perpendicular to the magnetic field in the scattering region.This meant that there was a problem with operating at VHF since VHF frequencies don't allow for very much refraction of the transmitted radar wave vector; thus, the perpendicularity requirement could not be easily met at high latitudes. At HF frequencies, however, refraction of the radar wavevector is greater, and this allows for the perpendicularity requirement to be met at high latitudes. Refraction of radio waves in the ionosphere is a complicated non-linear phenomenon governed by the Appleton–Hartree equation.
In 1983, a steerable-beam HF radar with 16 log-periodic antennas began operations at Goose Bay, Labrador, Canada. Comparing measurements of F region ionopheric plasma velocity from the Goose Bay radar with the Sondestrom Incoherent Scatter Radar revealed that the Goose Bay radar was capable of measuring the F region plasma convection velocity. A magnetically conjugate radar was constructed in Antarctica at Halley Research Station in 1988 as part of the Polar Anglo–American Conjugate Experiment. PACE provided simultaneous conjugate studies of ionospheric and magnetospheric phenomena.
From PACE, which was only able to determine a single component of the 2D ionospheric velocity, it became apparent that determining the 2D ionospheric velocity would be advantageous. Combining velocity measurements from Goose Bay with a second coherent-scatter radar in Schefferville in 1989 allowed for a 2D determination of the F region ionospheric velocity.
This work led to SuperDARN, a network of HF radars with pairs of radars having overlapping fields of view. This arrangement allowed for the determination of the full 2D ionospheric plasma convection velocity. Due to the advancement of data assimilation models, radars recently added to the network do not necessarily have overlapping fields of view. Using data from all SuperDARN radars in the northern or southern hemisphere, an ionospheric plasma convection pattern—a map of high-latitude plasma velocity at F region altitudes —can be determined.
Primary Goals
The primary goals of SuperDARN are to determine or study:- Structure of global convection—to provide a global-scale view of the configuration of plasma convection in the high-latitude ionosphere;
- Dynamics of global convection—to provide a global-scale view of the dynamics of plasma convection in the high-latitude ionosphere. ;
- Substorms—to test various theories of polar cap expansion and contraction under changing IMF conditions and observe the large-scale response of the nightside; convection pattern to substorms:
- Gravity waves,
- High-latitude plasma structures, and
- Ionospheric irregularities
Operations
Each beam is divided into 75 range gates each 45 km in distance, and so in each full scan the radars each cover 52° in azimuth and over 3000 km in range; an area encompassing the order of 1 million square km.
The radars measure the Doppler velocity of plasma density irregularities in the ionosphere.
Since Linux became popular, it has become the default operating system for the SuperDARN network. The operating system.
SuperDARN sites
The following is a list of SuperDARN sites, based on a list maintained by Virginia Tech College of Engineering. As of 2009, an expansion project was underway for expanding the network into the middle latitudes, including the addition of sites in Hays, Kansas, Oregon, and the Azores, in order to support mapping outside of the auroral regions during large magnetic storms.*: Part of the Southern Hemisphere Auroral Radar Experiment
Coverage
Northern Hemisphere- Because the SuperDARN network evolved in the west during the late Cold War, coverage of Russia's arctic regions is poor.
- Although there is no shortage of possible sites to cover Russia's Arctic regions from Northern Europe and Alaska, the coverage would probably not be of high quality.
- Although Russian universities have worked with the University of Leicester and installed a HF radar in Siberia, national funding issues have limited the radar operations.
- The Polar Research Institute of China has extended mid-latitude coverage, christening the extension to SuperDARN "AgileDARN"
- Although Antarctica is covered reasonably well, the Sub-Antarctic regions do not have uniform coverage due to the large expanse of ocean.
- Java VM real time display software interoperability is still a work in progress.
Annual SuperDARN Workshops
| Year | Venue | Host Institution |
| 2019 | Fujiyoshida, Yamanashi, Japan | National Institute of Information and Communications Technology |
| 2018 | Banyuls-sur-Mer, France | L'Institut de Recherche en Astrophysique et Planétologie |
| 2017 | San Quirico D'Orcia, Siena, Italy | Institute for Space Astrophysics and Planetology of the National Institute for Astrophysics |
| 2016 | Fairbanks, Alaska, USA | Geophysical Institute, University of Alaska Fairbanks |
| 2015 | Leicester, UK | Radio and Space Plasma Physics Group, University of Leicester |
| 2014 | Longyearbyen, Svalbard, Norway | The University Centre in Svalbard |
| 2013 | Moose Jaw, Saskatchewan, Canada | University of Saskatchewan |
| 2012 | Shanghai, China | Polar Research Institute of China |
| 2011 | Hanover, New Hampshire, USA | Dartmouth College |
| 2010 | Hermanus, South Africa | SANSA Space Science |
| 2009 | Cargèse, Corsica, France | Le Centre national de la recherche scientifique |
| 2008 | Newcastle, New South Wales, Australia | School of Mathematical & Physical Sciences, Newscastle University |
| 2007 | Abashiri, Hokkaido, Japan | Institute for Space-Earth Environmental Research, Nagoya University |
| 2006 | Chincoteague, USA | Johns Hopkins University, Applied Physics Laboratory |
| 2005 | Cumbria, UK | British Antarctic Survey |
| 2004 | Saskatoon, Canada | University of Saskatchewan |
| 2003 | Kiljava, Finland | |
| 2002 | Valdez, Alaska, USA | Geophysical Institute, University of Alaska Fairbanks |
| 2001 | Venice, Italy | |
| 2000 | Beechworth, Victoria, Australia | La Trobe University |
| 1999 | Reykjavik, Iceland | |
| 1998 | Tokyo, Japan | National Institute of Polar Research |
| 1997 | Ithala Game Reserve, South Africa | |
| 1996 | Ellicott City, MD, USA | |
| 1995 | Madingley Hall, Cambridge, UK |