EGU2020-18662
https://doi.org/10.5194/egusphere-egu2020-18662
EGU General Assembly 2020
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Dome C North radar, a new radar of the SuperDARN network: the first year of observations.

Maria Federica Marcucci, Igino Coco, Stefano Massetti, Simona Longo, David Biondi, Enrico Simeoli, Alessandro Cirioni, Andrea Satta, Angelo De Simone, and Aurélie Marchaudon
Maria Federica Marcucci et al.
  • INAF, IAPS, Roma, Italy (federica.marcucci@iaps.inaf.it)

In January 2019 the new Super Dual Auroral Radar Network (SuperDARN) radar installed at the Concordia Station in Antarctica and denominated Dome C North (DCN) saw the first light. SuperDARN is an international network of HF radars that observe the effects produced in the ionosphere by the chain of phenomena taking place in the Earth's space environment. DCN and its companion radar Dome C East (DCE) are positioned nearby the southern geomagnetic pole with their Field of View extending towards the auroral latitudes. Here we present the analysis of the first year of observations as a function of the interplanetary conditions.

How to cite: Marcucci, M. F., Coco, I., Massetti, S., Longo, S., Biondi, D., Simeoli, E., Cirioni, A., Satta, A., De Simone, A., and Marchaudon, A.: Dome C North radar, a new radar of the SuperDARN network: the first year of observations., EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-18662, https://doi.org/10.5194/egusphere-egu2020-18662, 2020

Displays

Display file