PRESCIENT
PRESCIENT supports long-term, strategically important measurements and capabilities for the wider science community.
I am the Deputy Science Leader of the Space Weather and Atmosphere Team at BAS, and a member of the NERC supported UK EISCAT Support Group (UKESG).
I started at BAS in January 2012 as part of the Middle Atmosphere Dynamics group in the climate program. I worked on projects involving the dynamics of the middle and upper atmosphere using a variety of instruments, but concentrating on the two Medium Frequency (MF) radars that BAS operated at our research stations at Halley and Rothera. With the restructure of the BAS science programs I joined the newly formed Space Weather and Atmosphere Team.
Being a Space Weather scientist means that I have been lucky enough to spend time in both the Arctic and Antarctic during my career; the polar regions are the primary gateways by which space weather interacts with the Earth’s atmosphere. I am currently the PI for the MF radar at Rothera, which I use to study the coupling of the atmosphere to the space environment.
In my career to date I have worked on a number of projects related to understanding the Sun-Earth system, these have includes studies of the aurora, HF radio absorption, particle dynamics, geomagnetic pulsations, plasma heating and mesospheric dust. I was very lucky to take part in experiments that generated artificial aurora and be the project scientist for a VLF receiver mounted on a Yorkshire school roof that formed part of the AARDDVARK network.
I study how the layers of the atmosphere and the near-Earth space environment couple together – known as vertical coupling.
My main interests are:
Each of these is important for our understanding of space weather events and how they impact our lives.
There is growing evidence that changes in the solar wind can lead to temperature changes in the polar regions. Waves the transfer energy and momentum into the upper atmosphere can modify conditions that affect satellite signal fade-out & scintillation, and the behaviour of electric current systems. Space weather events lead to heating of the upper atmosphere which in turn affects the lifetime of satellites and space debris in Low Earth Orbit (LEO). This is important to understand since LEO is becoming very crowded and collisions with debris can seriously damage satellites.
Part of the EISCAT Science Support Group working with colleagues at RAL Space
Middle & Upper Atmosphere
Energetic Precipitation
Substorms
Ionosphere and Aurora
Reidy, J., Kavanagh, A., & Wild, M. (2025). Data from the EISCAT UHF and VHF between 2001- 2021, integrated at 10 minutes and 1 hour between 50-200km (Version 1.0) [Data set]. NERC EDS UK Polar Data Centre. https://doi.org/10.5285/7d907fd0-8f08-45a6-ab91-89f6f0221b10
Woodfield, E., Glauert, S., Menietti, J., Horne, R., Kavanagh, A., & Shprits, Y. (2022). Acceleration of electrons by whistler-mode hiss waves at Saturn (Version 1.0) [Data set]. NERC EDS UK Polar Data Centre. https://doi.org/10.5285/c6202511-d70b-45ae-9b72-ff30f4888f5f
PRESCIENT supports long-term, strategically important measurements and capabilities for the wider science community.
MesoS2D uses powerful radars and satellites to study a little-understood layer of the atmosphere, the mesosphere.
SWIGS investigated how space weather drives geomagnetically induced currents in power grids, pipelines, and railways.
Joule Heating investigated how space weather affects the upper atmosphere’s ability to slow down orbiting satellite debris.
The Super Dual Auroral Radar Network (SuperDARN) has been operating as an international co-operative organisation for over 25 years, and has proved to be one of the most successful tools for studying dynamical processes in the Earth’s magnetosphere, ionosphere, and neutral atmosphere.
The UK EISCAT support group (UKESG) is a collaboration between the British Antarctic Survey and the Rutherford Appleton Laboratory, funded via the National Centre for Atmospheric Science (NCAS).
DRIIVE researches how polar ionosphere changes affect satellite orbits, communications, and space weather forecasts.
An international team of scientists, including a researcher from British Antarctic Survey (BAS) has, for the first time, successfully measured a planet-wide electric field thought to be as fundamental to Earth as its gravity and magnetic fields.
Dr Andrew Kavanagh of the British Antarctic Survey (BAS) Space Weather team has supported a new National Aeronautics and Space Administration (NASA) rocket experiment which aims to uncover unique features of our atmosphere that enable life on Earth.
A new project to improve scientists understanding of the impact of space weather and climate change on the atmosphere starts this month (January 2022). A team from British Antarctic Survey, […]
The Halley Research Station multiband riometer is a passive instrument that measures radio energy from natural astronomical sources.
A meteor radar that uses the scatter from meteor trails to estimate horizontal neutral winds between 80 and 110 km
The Medium Frequency (MF) radar at Rothera Research Station measures an altitude profile of the horizontal wind in the mesosphere, between 55 and 95 km.
The MF radar at Halley measures an altitude profile of the horizontal wind in the mesosphere, between 55 and 95 km.
The most advanced space weather radar in the world is to be built in the Arctic by an international partnership including the UK, thanks to new investment, including in the […]