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 …
30 December, 2023 by Emily Newton
How does a woman born in 1950s England go on to earn a PhD in geology, spend weeks at a time researching in Antarctica, become the director of the British …
3 August, 2020 by David Vaughan
BLOG. BAS Director of Science, Professor David Vaughan describes his ambition for more diversity in science.
17 December, 2024 by Richard Horne, Sarah Glauert, Thomas Daggitt
The density of low energy charged particles trapped in Earth's magnetic field can influence how higher energy trapped electrons are affected by natural radio waves within the magnetic field. We…7 December, 2024 by Nigel Meredith, Richard Horne
Relativistic electrons cause internal charging on satellites and are a significant space weather hazard. In this study we analyze approximately 20 years of data from the US Global Positioning System…Read more on Strong Relativistic Electron Flux Events in GPS orbit
6 December, 2024 by Emma Woodfield, Richard Horne
An abundant multi-MeV electron population beyond the orbit of Io is required to explain the intense inner radiation belt (electrons >50 MeV) at Jupiter and its synchrotron radiation. In order…6 December, 2024 by Emma Woodfield, Richard Horne
The spatial distribution of whistler-mode wave emissions in the Jovian magnetosphere measured during the first 45 perijove orbits of Juno is investigated. A double-belt structure in whistler-mode wave intensity is…Read more on Jupiter’s Whistler-mode Belts and Electron Slot Region
1 October, 2024 by Richard Horne
The 23–24 April 2023 double-peak (SYM-H intensities of −179 and −233 nT) intense geomagnetic storm was caused by interplanetary magnetic field southward component Bs associated with an interplanetary fast-forward shock-preceded…Read more on The April 2023 SYM‐H = −233 nT Geomagnetic Storm: A Classical Event
26 September, 2024 by Anthony Fox, Ashley Bennison, Dan McKenzie, Elizabeth Holmes, Elaine Fitzcharles, Freya Blockley, George Day, Isabel Stubbs, Jennifer Forster Davidson, Jaume Forcada, Kevin Hughes, Marcia Blyth, Michael Dunn, Norman Ratcliffe, Richard Phillips, Rosamund Hall, Steven Marshall, Simon Morley, Stacey Adlard
Capsule: HPAI H5N1 was documented for the first time in the subantarctic region on Bird Island, South Georgia, resulting in the mortality of Brown Skuas Stercorarius antarcticus, Gentoo Penguins Pygoscelis…28 July, 2024 by Anna Jones, Evelyn Workman, Katrin Linse
Sea-air methane flux was measured directly by the eddy-covariance method across approximately 60,000 km of Arctic and Antarctic cruises during a number of summers. The Arctic Ocean (north of 60°N,…17 July, 2024 by Richard Horne
Updated summaries of the August 1972 and March 1989 space weather events have been constructed. The features of these two events are compared to the Carrington 1859 event and a…28 June, 2024 by Nigel Meredith, Richard Horne, Sarah Glauert, Thomas Daggitt
The plasma density is one of the most fundamental quantities of any plasma yet measuring it in space is exceptionally difficult when the density is low. Measurements from particle detectors…8 June, 2024 by Jack Atkinson, Johnathan Ross, Richard Horne, Sarah Glauert
As the number of satellites on orbit grows it is increasingly important to understand their operating environment. Physics-based models can simulate the behavior of the Earth's radiation belts by solving…29 May, 2024 by Anna Jones, Thomas Lachlan-Cope
Antarctica and the Southern Ocean are the most pristine areas of the globe and represent ideal places to investigate aerosol-climate interactions in an unperturbed atmosphere. In this study, we present…15 May, 2024 by Richard Horne, Sarah Glauert
The Near-Earth Space Radiation and Plasma Environment falls within the realm of G3 Cluster (G3 refers to ‘Near-Earth Radiation and Plasma Environment’ of the ‘Coupled Geospace System’) under the COSPAR…23 April, 2024 by Alexander Lozinski, Richard Horne, Sarah Glauert
The proton radiation belt contains high fluxes of adiabatically trapped protons varying in energy from ∼one to hundreds of megaelectron volts (MeV). At large radial distances, magnetospheric field lines become…1 April, 2024 by Richard Horne
Observations from Van Allen Probes are analyzed to obtain the statistical wave normal distribution of lightning-generated whistlers (LGWs). An automatic algorithm is developed to identify burst mode waveform data with…27 February, 2024 by Richard Horne, Sarah Glauert, Thomas Daggitt
Earth’s radiation belts consist of high-energy charged particles trapped by Earth’s magnetic field. Strong pitch angle diffusion of electrons caused by wave-particle interaction in Earth’s radiation belts has primarily been…26 February, 2024 by Alistair Crame, Jane Francis
The Cretaceous period is particularly well represented by a thick sequence of clastic sedimentary rocks exposed in the Antarctic Peninsula region of western Antarctica. This was an active margin throughout…Read more on Cretaceous stratigraphy of Antarctica and its global significance
11 February, 2024 by Richard Horne
In a case study using Van Allen Probe B, we investigate chorus wave observations near the western edge of a plasmaspheric plume characterized by steep density gradients. Initially, wave vectors…Read more on Propagation of Very Oblique Chorus Waves Near a Plasmaspheric Plume Boundary
27 January, 2024 by Jade Reidy, Jenny Wong, Johnathan Ross, Mark Clilverd, Nigel Meredith, Richard Horne, Sarah Glauert, Jade Reidy
High energy electron precipitation from the Earth's radiation belts is important for loss from the radiation belts and atmospheric chemistry. We follow up investigations presented in Reidy et al. (2021,…1 January, 2024 by Jenny Wong, Johnathan Ross, Nigel Meredith, Richard Horne, Sarah Glauert
Relativistic electrons in the Earth's outer radiation belt are a significant space weather hazard. The belt, which lies at altitudes from 13,000 to 40,000 km in the Earth's magnetic equatorial…Read more on New Chorus Diffusion Coefficients for Radiation Belt Modeling
1 November, 2023 by Alistair Crame, Jane Francis, Rowan Whittle, Vanessa Bowman
Lower Paleocene marine siliciclastics of the Sobral Formation (Seymour Island, Antarctica) form an important component of a key southern high latitude reference section for the Maastrichtian–Eocene. The formation comprises a…
