MIST

Magnetosphere, Ionosphere and Solar-Terrestrial

Latest news

2026 MIST Council Election Results

It is our pleasure to announce the results of the latest MIST Council Election.

  • Samuel Wharton (University of Leicester) is elected for a 3 year term as a MIST Councillor
  • Jewel Abbey Relampagos (Lancaster University) is elected for a 1 year term as the MIST Student Representative

In addition, due to concerns from the community regarding the ongoing UKRI/STFC funding situation, MIST Council have also decided to charter Mark Lester (University of Leicester) as an additional councillor to inform and steer the council in matters related to this specific brief, as set out in Article 4.5 of the MIST Charter.

We would like to congratulate everyone on their new roles. The full composition of Council can be found on the MIST website (https://www.mist.ac.uk/community/mist-council). We would like to thank all the candidates for putting themselves forward and everyone who took part in the voting. We received votes from 132 people which represents a turnout of 21.5% of people registered to receive the MIST emailing list.

Finally, MIST Council would like to extend their thanks and gratitude to our outgoing members: Fiona Ball and Georgios Nicolaou. We would also like to say a special thank you to Andy Smith who was co-opted to be on MIST council while Rosie Johnson was on maternity leave, thank you for all of your hard work.

Open Letter Ready For Signatories

Protect MIST Science! Sign the MIST Community Open Letter on the STFC funding cuts!

https://sites.google.com/view/uk-mist-community-open-letter

 

Statement from MIST Council regarding the STFC Funding Situation

Statement from MIST Council regarding the STFC Funding Situation

MIST Council is deeply concerned by the ongoing STFC funding uncertainty and its impact on our community and beyond.

The current combination of prospective delayed and reduced funding, together with already volatile financial situations at universities across the UK, is placing significant strain on research groups. In some cases, institutions may be unable to support researchers through gaps between projects, increasing precarity across the community and adding significant pressure on early-career researchers.

We are concerned that continued uncertainty risks accelerating a brain drain from the UK, as skilled researchers reconsider their future in a system offering limited stability. The loss of expertise at any career stage would have lasting consequences for UK space science.

 

What is going on?

For those that are unaware of the situation, it is complex and evolving. We suggest the following sources to get up to speed on the current developments.

https://www.sciencecampaign.org.uk/analysis-and-publications/detail/what-is-happening-with-ukri-funding-and-the-stfc-cuts/

https://ras.ac.uk/news-and-press/news/proposed-budget-cuts-catastrophe-uk-astronomy

https://www.newscientist.com/article/2514481-physicists-warn-of-catastrophic-impact-from-uk-science-cuts/

 

What are we doing about it?

Behind the scenes, MIST Council is actively engaging with relevant parties to understand the scale of the challenge and to identify constructive ways forward.

  • We are seeking seasoned members of the community to join MIST Council on a task force to help develop options and represent the needs of our community. If you would like to be involved, please reach out to us via the MIST Council email (This email address is being protected from spambots. You need JavaScript enabled to view it.) by the end of this week (13th February 2026).
  • In addition to the task force, we want to provide an open forum for discussion and collective input among all members of the wider MIST community. We are exploring options and will be in touch as soon as possible with further details.
  • We believe in working together in the face of the current challenges and we are collaborating with UKSP and others to strive for a fair and positive outcome for all. We are reaching out to members of the SSAP (Solar System Advisory Panel) to explore the hosting of a community town hall meeting, like the one already being organised by the AAP (Astronomy Advisory Panel), to provide an open forum for discussion and collective input.

 

What can you do to help?

There are several open letters representing people in various career stages that have been made available to sign. We encourage you to read the relevant letter(s) and to sign them if you support them:

The Royal Astronomical Society are also urging Fellows to lobby their MPs against the cuts, and have included a template letter that can be used to do so:
https://ras.ac.uk/news-and-press/news/ras-fellows-urged-lobby-against-unprecedented-cuts

 

MIST Council will continue to advocate for transparency, stability, and funding structures that recognise both the long-term nature of our science and the people who deliver it.
We thank you for your continued support in this period of uncertainty.

 

Please contact This email address is being protected from spambots. You need JavaScript enabled to view it. if you have further suggestions.
MIST Council

Announcement of New MIST Council 2025

We are very pleased to announce the following members of the community have been elected to MIST Council:

  • Gemma Bower (University of Leicester), MIST Councillor
  • Tom Elsden (University of St Andrews), MIST Councillor
  • Cameron Patterson (Lancaster University), MIST Councillor
  • Fiona Ball (University of Southampton), Student Representative

They will begin their terms in July 2025.

We thank outgoing MIST Council members: Maria Walach, Chiara Lazzeri and Emma Woodfield. Andy Smith will remain on council a little longer as a co-opted member to cover Rosie Johnson's maternity leave.

The current composition of Council can be found on our website (https://www.mist.ac.uk/community/mist-council).

Announcement of New MIST Councillors.

We are very pleased to announce the following members of the community have been elected unopposed to MIST Council:

  • Rosie Johnson (Aberystwyth University), MIST Councillor
  • Matthew Brown (University of Birmingham), MIST Councillor
  • Chiara Lazzeri (MSSL, UCL), Student Representative

Rosie, Matthew, and Chiara will begin their terms in July. This will coincide with Jasmine Kaur Sandhu, Beatriz Sanchez-Cano, and Sophie Maguire outgoing as Councillors.

The current composition of Council can be found on our website, and this will be amended in July to reflect this announcement (https://www.mist.ac.uk/community/mist-council).

MIST Acronyms

Please notify any corrections/ additions to the MIST webmaster A B C D E F G H I J K L M N O P Q R S T U V W XYZ


AA: Auroral Absorption
ACE: Advanced Composition Explorer
ACF: Autocorrelation Function
ADAF: AGONet Data Analysis Facility
AE: Auroral Electrojet (auroral activity index)
AG: Annales Geophysicae
AGO: Automatic Geophysical Observatory
AGONet: Antarctic Geospace Observatory Network
AGU: American Geophysical Union
AGW: Atmospheric Gravity Wave
AIS: Advanced Ionospheric Sounder
AL: Auroral Lower (auroral activity index)
ALOMAR: Arctic Lidar Observatory for Middle Atmosphere Research
AMIE: Assimilative Mapping of Ionospheric Electrodynamics
AMPTE: Active Magnetospheric Particle Tracer Explorers
Ap: (Planetary magnetic activity index)
AU: Astronomical Unit
AU: Auroral Upper (auroral activity index)
AVDAS: Advanced VLF Data Analysis System
AXO: Atmospheric X-ray Observatory
BAS: British Antarctic Survey
BGS: British Geological Survey
BNSC: British National Space Centre
BTW: By the way
CAMMICE: Charge and Mass Magnetospheric Ion Composition Experiment (on Polar)
CANOPUS: Canadian Auroral Network for the OPEN Program Unified Study
CAPS: Cassini Plasma Spectrometer 
CCD: Charge-Coupled Device
CDAW: Coordinated Data Analysis Workshop
CDF: Common Data Format
CDHF: Co-ordinated Data Handling Facility
CEDAR: Coupling, Energetics and Dynamics of Atmospheric Regions
CEPPAD: Comprehensive Energetic Particle and Pitch Angle Distribution Experiment (on Polar)
CIR: Co-rotating Interaction Region
CIS: Cluster Ion Spectrometry Experiment (Cluster)
CMAT: Coupled Middle Atmosphere and Thermosphere (model)
CME: Coronal Mass Ejection
CNA: Cosmic Noise Absorption
CNES: Centre Nationale des Etudes Spatiales (France)
Co-I: Co-Investigator
COSPAR: Commission on Space Research
CP: Common Programme (EISCAT, SuperDARN etc)
CRRES: Combined Release / Radiation Effects Satellite
CTIM: Coupled Thermosphere Ionosphere Magnetosphere (model)
CTIP: Coupled Thermosphere Ionosphere Plasmasphere (model)
CUTLASS: Collaborative UK Twin-Located Auroral Sounding System
DABS: Data Access and Browsing System
DASI: Digital All-Sky Imager
DAT: Digital Audio Tape
DE: Dynamics Explorer
DFT: Discrete Fourier Transform
DMSP: Defense Meteorological Satellite Program
DSP: Digital Signal Processing
Dst: Disturbance storm time (geomagnetic index)
DWP: Digital Wave Processing Experiment (Cluster)
ECH: Electron Cyclotron Harmonic
ECPC: Expanding-Contracting Polar Cap
EFW: Electric Fields and Waves (Cluster)
EGS: European Geophysical Society
EGU: European Geophysical Union
EIS: EUV Imaging Spectrometer
EISCAT: European Incoherent Scatter Radar
ELF: Extremely Low Frequency
EMIC: Electromagnetic Ion Cyclotron Waves
ENA: Energetic Neutral Atom
EPC: EISCAT Project Committee
EPCI: Electron Pedersen Conductivity Instablity
ESA: European Space Agency
ESR: EISCAT Svalbard Radar
ESTEC: European Space Research and Technology Centre
ETAP: EISCAT Time Allocation Panel
EUV: Extreme UltraViolet
FAC: Field Aligned Current
FAQ: Frequently asked Questions
FAST: Fast Auroral SnapshoT explorer
FBI: Farley-Buneman Instability
FFT: Fast Fourier Transform
FGM: Fluxgate Magnetometer
FLR: Field Line Resonance
FOV: Field Of View
FPI: Fabry-Perot Interferometer
FTE: Flux Transfer Events
FTP: File Transfer Protocol
FWIW: For what it's worth
FYI: For Your Information
GCM: Global Circulation Model
GEM: Geospace Environment Modelling
GEOS: GEOstationary Satellite
GFM: Global Field Model
GGS: Global Geospace Study
GIC: Geomagnetically Induced Current
GIF: Graphics Interchange Format
GIME: Global Imaging of Magnetospheric Electrodynamics
GMT: Greenwich Mean Time (same as UT)
GOES: Geostationary Orbiting Environmental Satellite
GPS: Global Positioning System
GRL: Geophysical Research Letters
GSE: Geocentric Solar Earth (coordinates)
GSFC: Goddard Space Flight Center (NASA)
GSM: Geocentric Solar Magnetic (coordinates)
HCS: Heliospheric Current Sheet
HESSI: High Energy Solar Spectroscopic Imager
HF: High Frequency
HIREX: High-Resolution X-ray Explorer
HST: Hubble Space Telescope
HXT: Hard X-ray Telescope
IAGA: International Association of Geomagnetism and Aeronomy
IBIZA/IMPACT: Investigation BIsatellitaire des Zones Aurorales/Investigation of Magnetospheric Particles Acceleration and Turbulence
IC: Imperial College
ICME: Interplanetary Coronal Mass Ejection
ICSU: International Council of Scientific Unions
IDF: Ion Distribution Function
IDI: Imaging Doppler Interferometer
IDL: Interactive Data Language
IGBP: International Geosphere Biosphere Programme
IGRF: International Geomagnetic Reference Field
IGY: International Geophysical Year
IHV: Inter-Hourly Variation
IHY: International Heliophysical Year
IKI: Inter-Kosmos Institute (Russian Space Research)
ILWS: International Living with a Star (program)
IMAGE: International Monitor for Auroral Geomagnetic Effects
IMAGE: Imager for Magnetopause-to-Aurora Global Exploration
IMF: Interplanetary Magnetic Field
IMHO: In my humble opinion
IMP: Interplanetary Magnetic Probe
INPE: Instituto de Pesquisas Espaciais (Brazil)
IPS: Interplanetary Scintillations
IPY: International Polar Year
IRI: International Reference Ionosphere
IRIS: Imaging Riometer for Ionospheric Studies
IRM: Ion Release Module (of AMPTE)
IS: Incoherent Scatter
ISAS: Institute of Space and Astronautical Science (Japan)
ISEE: International Sun-Earth Explorer
ISTP: International Solar Terrestrial Physics Programme
ITM: Ionosphere Thermosphere and Mesosphere
JAG: Joint Association of Geophysics
JATP: Journal of Atmospheric and Terrestrial Physics
JGR: Journal of Geophysical Research
JGR: Journal of Geomagnetism and Geoelectricity
JIM: Jovian Ionospheric Model
KCL: Kings College, London
KHI: Kelvin-Helmholtz Instability
Kp: (Planetary magnetic activity index)
L: McIlwain's geomagnetic coordinate
LANL: Los Alamos National Laboratory
LASCO: Large Angle and Spectrometric Coronagraph (on SOHO)
LENA: Low Energy Neutral Atom (IMAGE)
LEO: Low Earth Orbit
LEP: Lightning-induced Electron Precipitation
LEPA: Low Energy Plasma Analyzer
LF: Low Frequency
LIE: Lightning-induced ionisation enhancement
LLBL: Low latitude boundary layer
LT: Local Time
LWPC: Long Wave Propagation Capability
LWS: Living with a Star
MACCS: Magnetometer Array for Cusp and Cleft Studies
MAGIC: Magnetometer Array on the Greenland Ice Cap
MAGPIES: MAGnetospheric Plasma Imaging Explorer Satellites
MALT: Mesosphere And Lower Thermosphere
MC: Magnetic Cloud
MF: Medium Frequency
MHD: Magneto-hydrodynamics
MIAOW: Mirrow and Slow Mode Waves
MICS: Magnetosphere Ionosphere Coupling Satellite
MIDAS: Multi-Instrument Data Analysis System
MIST: Magnetosphere Ionosphere and Solar Terrestrial (community in the UK)
MLAT: Magnetic Latitude
MLT: Magnetic Local Time
MPI: Max Planck Institute
MR: Magnetospherically Reflected
MSIS: Mass-Spectrometer-Incoherent-Scatter (neutral atmosphere model)
MSSL: Mullard Space Science Laboratory
NARMAX: Nonlinear AutoRegressive moving average model with eXogenous Inputs
NASA: National Aeronautics and Space Administration
NCAR: National Centre for Atmospheric Research
NENL: Near Earth Neutral Line
NERC: Natural Environment Research Council
NIPR: National Institute for Polar Research (Japan)
NLC: Noctilucent Cloud
NOAA: National Oceanographic and Atmospheric Administration
NRC: National Research Council (USA)
NRF: Non-Radial Flow
NSF: National Science Foundation (USA)
NSSDC: National Space Science Data Centre (USA)
OCB: Open-Closed fieldline Boundary
OPP: Office of Polar Programs (USA)
OST: Office of Science and Technology
PACE: Polar Anglo-American Conjugate Experiment
Pc: Pulsation continuous
PC: Polar Cap (magnetic activity index)
PCA: Polar Cap Absorption
PCB: Polar Cap Boundary
PDF: Probability Distribution (or Density) Function
PEACE: Plasma Electron And Current Experiment (Cluster)
Pi: Pulsation irregular
PI: Principal Investigator
PIF: Pulsed Ionospheric Flow
PLHR: Power Line Harmonic Radiation
PMAF: Polward-moving auroral form
PMSE: Polar Mesospheric Summer Echo
PPARC: Particle Physics and Astronomy Research Council
PSBL: Plasma Sheet Boundary Layer
PSD: Power Spectral Density
PSMOS: Planetary Scale Mesopause Observing System
PSS: Planetary and Space Science
PUS: Public Understanding of Science
PWI: Plasma Wave Instrument
QBO: Quasi Biennial Oscillation
QDC: Quiet Day Curve
QJRAS: Quarterly Journal of the RAS
QP: Quasi-Periodic
RAL: Rutherford Appleton Laboratory
RAPID: Research into Adaptive Particle Imaging Detectors (Cluster)
RAS: Royal Astronomical Society
RF: Radio Frequency
RFI: Radio Frequency Interference
RFI: Resonant Flux Instability
RMS: Root mean square
RS: Royal Society
RWD: Regular World Day
S/C: SpaceCraft
SABRE: Swedish and British Radar Experiment
SAGA: South Atlantic Geomagnetic Anomaly
SAMNET: Sub-Auroral Magnetometer Network
SAMPEX: Solar Anomalous and Magnetospheric Particle Explorer
SAPS: Sub-Auroral Polarization Stream
SAR: Subauroral Red
SAR: Synthetic Aperture Radar
SCAR: Scientific Committee on Antarctic Research
SCE: Substorm Chorus Event
SCOSTEP: Scientific Committee on Solar Terrestrial Physics
SEEP: Stimulated Emission of Energetic Particles (satellite)
SEL: Space Environment Laboratory (USA)
SEP: Solar Energetic Particles
SESAME: Satellite Experiments Simultaneous with Antarctic Measurements
SGO: Sodankyla Geophysical Observatory
SHARE: Southern Hemisphere Auroral Radar Experiment
SID: Sudden Ionospheric Disturbance
SLAMS: Short large-amplitude waves
SNR: Signal to Noise Ratio
SOC: Self-Organised Criticality
SOHO: Solar Heliospheric Observatory
SPEAR: Space plasma exploration by active radar
SSC: Sudden Storm Commencement
SSC: Satellite Situation Centre
STAFF: Spatio-Temporal Analysis of Field Fluctuation (Cluster)
STARE: Scandinavian Twin Aurora Radar Experiment
STEP: Solar Terrestrial Energy Programme
STEREO: Solar Terrestrial Relations Observatory
STP: Solar-Terrestrial Physics
SuperDARN: Super Dual Auroral Radar Network
SUPIM: Sheffield University Plasmasphere-Ionosphere (model)
SXT: Soft X-ray Telescope
TBD: To be decided
TCR: Travelling Compression Region
TCV: Travelling Convection Vortex
TEC: Total Electron Content
TID: Travelling Ionospheric Disturbance
TIMAS: Toroidal Imaging Mass-Angle Spectrograph
TIMED: Thermosphere Ionosphere Mesosphere Energetics and Dynamics
TIROS: Television InfraRed Observation Satellite
TLA: Three letter acronym
TOI: Tongue of Ionisation
TRACE: Transition Region and Coronal Explorer (satellite)
TSS: Tethered Satellite System
UARS: Upper Atmosphere Research Satellite
UCL: University College, London
UCLA: University of California, Los Angeles
UHF: Ultra High Frequency
UKEUG: UK EISCAT Users' Group
UKS: UK Satellite (of AMPTE)
UKSP: UK Solar Physics (community)
ULF: Ultra Low Frequency
UMLT: Upper Mesosphere Lower Thermosphere
UNIS: University Courses in Svalbard (Longyearbyen, Norway)
URSI: Union of Radio Science International
UT: Universal Time
UTC: Universal Time, Coordinated (nearly the same as UT)
UV: UltraViolet
UVI: Ultraviolet Imager
UWA: University of Wales, Aberystwyth
VELOX: VLF/ELF Logger Experiment
VERSIM: VLF/ELF Remote Sensing of the Ionosphere & Magnetosphere
VHF: Very High Frequency
VLF: Very Low Frequency
VO: Virtual Observatory
VSPO: Virtual Space Plasma Observatory
WCS: World class science
WDC: World Data Centre
WEC: Wave Experiment Consortium (Cluster)
WEP: Wave-induced Electron Precipitation
WFT: Windowed Fourier Transform
WHISPER: Waves of High frequency and Sounder for Probing of Electron density by Relaxation (Cluster)
WOT: Waste of time
WPI: Wave - Particle Interaction
WRT: With respect to
WWW: World Wide Web
WYSYWYG: What you see is what you get
YDAC: Yohkoh Data Archive Centre