Registration Website: http://www.unis.no/superdarn2014/
Meeting Dates: May 25-30, 2014
Deadlines for Registration & Accommodation: 23rd February 2014
Deadline for Abstracts: 25th April 2014
The 2014 SuperDARN meeting is going to be held in Longyearbyen, Svalbard (Norway). Longyearbyen is located on an archipelago at 78˚ North Latitude, making it one of the northernmost towns in the world. Longyearbyen has a long history of auroral and ionospheric research and is home to EISCAT Svalbard Incoherent Scatter Radar, the Kjell Henriksen Auroral Observatory, and the University Centre in Svalbard (UNIS). Longyearbyen is slated to be a future site of a SuperDARN radar.
Pictured: The 32 m dish of the EISCAT Svalbard radar (ESR). This radar operates in the 500 MHz band with a peak transmitter power of 1.0 MW. Foreground: Students from UNIS, the world's northernmost institution for higher education and research.
2014 SuperDARN Workshop is Coming!
The 2014 SuperDARN Workshop will be held from May 25-30 in Longyearbyen, Svalbard (Photo credit: Nathaniel Frissell)
Plot SuperDARN fields-of-view at any date since its beginning, or watch a full time lapse of SuperDARN development.
Mapping the global pattern of ionospheric plasma convection
View global convection maps using the Map Potential Plot tool available on the VT SuperDARN web site.
DaViTpy: the SuperDARN Data Visualization and Analysis Toolkit - in Python
Experience the power of Python to browse, mine and visualize SuperDARN data. Use Github to access and/or contribute to our new analysis toolkit. Presented at the 2013 SuperDARN student workshop.
SuperDARN: An International Collaboration
SuperDARN is made possible through the cooperation and funding of nine different countries... a true international effort!
Footpoints of the RBSP satellites in the ionosphere
Click on this image to see more orbit projections for various days.
First large-scale instantaneous mapping of Sub Auroral Polarization Stream (SAPS)
Map of the line-of-sight plamsa velocity for 08:40 UT, March 9th, 2011 (after Clausen et al. )
Coordinated mapping with Total Electron Content (TEC) obtained from GPS measurements
The SAPS feature observed with SuperDARN is seated in the trough-like feature mapped by TEC
Ray tracing tool
Model HF propagation in the ionosphere for any SuperDARN radars or your own fantasy HF radar...
Construction of the SuperDARN radars at Adak, Alaska (Credit: NSF Mid-Sized Infrastructiure Program)
View of the completed arrays of antenna poles - September, 2012 (Photo credit: N. Frissell)
Heating experiment with EISCAT and SuperDARN/CUTLASS - July 3, 2012
The SuperDARN/CUTLASS radar at Hankasalmi (Finland) observes scatter during 2-min intervals of ionospheric heating
Geometry of heating experiment with EISCAT and SUPERDARN/CUTLASS
The SuperDARN/CUTLASS radars at Pykkvibaer and Hankasalmi look over the site of the EISCAT heater at Tromso (Norway)(credit: Sebastien's 'Radar Finder' tool)
Welcome to SuperDARN!
SuperDARN stands for Super Dual Auroral Radar Network. The network consists of over 30 low-power HF radars that look into Earth's upper atmosphere beginning at mid-latitudes and extending into the polar regions. The radars operate continuously and observe the motion of charged particles (plasma) in the ionosphere and other effects that provide scientists with information on Earth's space environment. The knowledge gained from this work provides insight into space weather hazards including radiation exposure for high-altitude travelers and disruptions to communication networks, navigation systems (GPS), and electrical power grids.
The SuperDARN Research Group at Virginia Tech (VT) collaborates with an international community of scientists and engineers to operate the radars and share data. The VT Group operates five radars. For a summary of the radars and their affiliations, visit our Radar Maps/Tables/Links page.
By: Nathaniel Frissell on: Sun., Dec. 08, 2013 02:42 PM EST (353 Reads)
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Read All SuperDARN Technical News Articles.