Magnetosphere, Ionosphere and Solar-Terrestrial
web page for the UK Sun-Planetary scientific community
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MIST AcronymsPlease 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 XYZAA: 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 Return to MIST home page
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