The BAS Executive Team is responsible for strategic planning. Members advise and support the Director and help provide the overall leadership, direction and management of the Survey to achieve its mission.
Terms of Reference
16 May, 2018
On Monday 14 May, the British Antarctic Survey (BAS) and the Instituto Antártico Argentino (IAA) signed a memorandum of understanding that aims to provide a formal framework to joint scientific …
16 January, 2017
British Antarctic Survey (BAS) has decided not to winter at Halley VI Research Station for safety reasons. The station, which is located on the floating Brunt Ice Shelf in Antarctica, …
31 December, 2016
Two leading polar scientists at the British Antarctic Survey (BAS) have received awards in the 2017 New Year Honours list from Her Majesty the Queen. BAS Director, Professor Jane Francis, …
5 August, 2013
Independent evaluation of British Antarctic Survey research excellence The outcome of an independent evaluation of the research excellence within NERC (Natural Environment Research Council) Research Centres is published today. The …
3 August, 2020 by David Vaughan
BLOG. BAS Director of Science, Professor David Vaughan describes his ambition for more diversity in science.
23 February, 2023 by Richard Horne
In this study, we use approximately 3 years of observations from the Exploration of energization and Radiation in Geospace (ERG/Arase) satellite to statistically study the meridional distribution of wave power…Read more on Latitudinal dependence of ground VLF transmitter wave power in the inner magnetosphere
23 November, 2022 by Richard Horne
Owing to the ever-present solar wind, our vast solar system is full of plasmas. The turbulent solar wind, together with sporadic solar eruptions, introduces various space plasma processes and phenomena…21 November, 2022 by Johnathan Ross, Richard Horne, Sarah Glauert
Efforts to model and predict energetic electron fluxes in the radiation belts are highly sensitive to local wave-particle interactions. In this study, we use multi-point measurements of precipitating and trapped…13 October, 2022 by Johnathan Ross, Nigel Meredith, Richard Horne, Sarah Glauert
Kinetic wave-particle interactions in Earth's outer radiation belt energize and scatter high-energy electrons, playing an important role in the dynamic variation of the extent and intensity of the outer belt.…Read more on Temporal variability of quasilinear pitch-angle diffusion
1 October, 2022 by Mark Clilverd, Richard Horne
Intervals of Pulsations of Diminishing Periods (IPDPs) are a subtype of Electromagnetic Ion Cyclotron (EMIC) waves that can be triggered by substorm onset. Pi1B waves are Ultra Low Frequency (ULF)…25 September, 2022 by Johnathan Ross, Nigel Meredith, Richard Horne, Sarah Glauert
The banded structure of Electromagnetic Ion Cyclotron (EMIC) wave spectra and their resonant interactions with radiation belt electrons depend on the cold ion composition. However, there is a great deal…Read more on The importance of ion composition for radiation belt modeling
1 September, 2022 by Jane Francis
The Royal Geographical Society (with IBG) annual Medals and Awards recognise achievements in researching, communicating and teaching a wide range of geographical knowledge. The speeches and citations are a record…Read more on Royal Geographical Society (with IBG) Medals and Awards celebration 2022 [Speech]
10 August, 2022 by Mervyn Freeman, Richard Horne, Sarah Glauert, Thomas Daggitt
We analyse a set of events in which both electron flux dropouts caused by magnetopause shadowing and geosynchronous magnetopause crossings (GMCs) are observed. These observations are compared to event-specific last…15 April, 2022 by Jenny Wong, Johnathan Ross, Nigel Meredith, Richard Horne, Sarah Glauert
We conduct a global survey of magnetosonic waves and compute the associated bounce and drift averaged diffusion coefficients, taking into account co-located measurements of fpe/fce, to assess the role of…Read more on Electron diffusion by magnetosonic waves in the Earth’s radiation belts
12 April, 2022 by Richard Horne
In this study, we report the statistical properties of whistler mode low hybrid (LH) emissions in the ionosphere, which have structureless spectra with a lower frequency boundary that matches the…
17 March, 2022 by Edward Brown, Nigel Meredith, Richard Horne
Extreme ultraviolet images taken by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory make it possible to use deep vision techniques to forecast solar wind speed - a…1 March, 2022 by Richard Horne
During magnetospheric storms, radiation belt electrons are produced and then removed by collisions with the lower atmosphere on varying timescales. An efficient loss process is microbursts, strong, transient precipitation of…Read more on Ducted chorus waves cause sub‐relativistic and relativistic electron microbursts
1 February, 2022 by Andrew Kavanagh, Emma Woodfield, Richard Horne, Sarah Glauert
Plasmaspheric hiss waves at the Earth are well known for causing losses of electrons from the radiation belts through wave particle interactions. At Saturn, however, we show that the different…Read more on Acceleration of electrons by whistler-mode hiss waves at Saturn
16 December, 2021 by Richard Horne
Whistler-mode chorus waves are critical for driving resonant scattering and loss of radiation belt relativistic electrons into the atmosphere. The resonant energies of electrons scattered by chorus waves increase at…Read more on Conjugate observation of magnetospheric chorus propagating to the ionosphere by ducting
14 December, 2021 by Peter Kirsch, Richard Horne, Sarah Glauert
With new satellite constellations being launched into low Earth orbit, the growing use of medium Earth orbit for radio-navigation and timing signals, slot region orbits for telecommunications and the introduction…Read more on The Satellite Risk Prediction and Radiation Forecast System (SaRIF)
12 December, 2021 by Alexander Lozinski, Richard Horne, Sarah Glauert
Geomagnetically trapped protons forming Earth’s proton radiation belt pose a hazard to orbiting spacecraft. In particular, solar cell degradation is caused by non-ionising collisions with protons at energies of several…Read more on Modelling inner proton belt variability at energies 1 to 10MeV using BAS‐PRO
1 December, 2021 by Peter Kirsch, Richard Horne, Sarah Glauert
Increasing numbers of satellites are orbiting through the Earth's radiation belts, and the range of orbits being commonly used is also growing. As a result, there is an increasing need…Read more on Evaluation of SaRIF high-energy electron reconstructions and forecasts
1 December, 2021 by Johnathan Ross, Nigel Meredith, Richard Horne, Sarah Glauert
The interactions between electromagnetic ion cyclotron (EMIC) waves and relativistic electrons are influential in diffusing radiation belt electrons into the loss code from which the electrons are lost into the…
