EGU25-6290, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-6290
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 08:30–10:15 (CEST), Display time Thursday, 01 May, 08:30–12:30
 
Hall X4, X4.133
Statistical analysis of Multistatic meteor radar observations
Gunter Stober1, Alan Liu2, Alexander Kozlovsky3, Diego Janches4, Erin Dawkins4, Loretta Pearl Poku1, Zichun Qiao2, Masaki Tsutsumi5,6, Mark Lester9, Njål Gulbrandsen7, Satonori Nozawa8, Johan Kero10, Tracy Moffat-Griffin11, and Nicholas Mitchell11,12
Gunter Stober et al.
  • 1University Bern, Institute of Applied Physics, Microwave Physics, Bern, Switzerland (gunter.stober@unibe.ch)
  • 2Center for Space and Atmospheric Research, Department of Physical Sciences, Embry-Riddle Aeronautical University, Daytona Beach, Florida, USA
  • 3Sodankylä Geophysical Observatory, University of Oulu, Oulu, Finland
  • 4ITM Physics Laboratory, Mail Code 675, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
  • 5National Institute of Polar Research, Tachikawa, Japan
  • 6The Graduate University for Advanced Studies (SOKENDAI), Tokyo, Japan
  • 7Tromsø Geophysical Observatory UiT – The Arctic University of Norway, Tromsø, Norway
  • 8Division for Ionospheric and Magnetospheric Research Institute for Space-Earth Environment Research, Nagoya University, Japan
  • 9Department of Physics and Astronomy, University of Leicester, Leicester, UK
  • 10Swedish Institute of Space Physics (IRF), Kiruna, Sweden
  • 11British Antarctic Survey, Cambridge, UK
  • 12Department of Electronic & Electrical Engineering, University of Bath, Bath, UK

Multistatic meteor radar networks have become a valuable tool to study the spatial and temporal variability of mesosphere/lower thermosphere winds. Combined with advanced and tomographic analysis such as the 3DVAR+DIV or VVP algorithm it is possible to infer spectral information related to the horizontal wavelength and the temporal spectrum. Here we present a statistical analysis of almost 5 years of observations recorded with the Nordic Meteor Radar Cluster and CONDOR. Our initial results show a seasonal variability of the spectral slopes for different spatial scales indicating a reduced gravity wave activity during the spring for the Northern hemispheric data. Furthermore, we find a transition from a k-3 to a k-5/3 slope for spatial scales around 150 kilometers. Zonal wavelength spectra at CONDOR exhibit a less clear seasonal pattern compared to the Nordic Meteor Radar Cluster.   

How to cite: Stober, G., Liu, A., Kozlovsky, A., Janches, D., Dawkins, E., Pearl Poku, L., Qiao, Z., Tsutsumi, M., Lester, M., Gulbrandsen, N., Nozawa, S., Kero, J., Moffat-Griffin, T., and Mitchell, N.: Statistical analysis of Multistatic meteor radar observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6290, https://doi.org/10.5194/egusphere-egu25-6290, 2025.