Met Office Space Weather Operations and R&D



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Transcription:

Met Office Space Weather Operations and R&D David Jackson Mark Gibbs, Suzy Bingham, Francois Bocquet, Edmund Henley, Sophie Murray WMO / ISES Meeting, August 9-10 2014, Moscow, Russia

Met Office Motivation? 2010 Increasing interest within UK Government Max coinciding with Olympics Space Weather placed on NRR NOAA approached Met Office Met Office become back-up to SWPC Desire to demonstrate increased value of 24x7 operations

National Risk Register Volcanic ash Relative Risk

Identifying the risk Royal Academy of Engineering report Extreme space weather Carrington event Electricity ~13 transformers damaged in UK 2 coastal nodes could experience disconnection Possible short blackouts in urban areas Impact on Satellites, Aviation, GNSS, comms also assessed Need for further technical and forecast mitigation

Met Office Space Weather Operations Centre Embedded in Met Office Hazard Centre 24x7x365 29 April 14 Full capability autumn 14 New member of ISES Collaborate with academia not replicate Operational collaboration with NOAA SWPC & BGS Daily forecast coordination Add UK-centric advice and impacts

NOAA impact scales Category UK Effect US and Global Effect Physical measure Scale Descriptor Duration of event will influence severity of effects Geomagnetic Storms G 5 Extreme Power systems: Localised voltage control and Power systems:widespread voltage control Kp = 9 protective system problems may occur. problems and protective system problems can Spacecraft operations: may experience extensive surface charging, problems with orientation, uplink/downlink and tracking satellites. Other systems: HF (high frequency) radio propagation may be impossible in many areas for one to two days, GPS satellite navigation may be degraded for days, low-frequency radio navigation can be out for hours, and aurora has been seen as low as 40 geomagnetic lat. Spacecraft operations: may experience extensive surface charging, problems with orientation, uplink/downlink and tracking satellites. Other systems: pipeline currents can reach hundreds of amps, HF (high frequency) radio propagation may be impossible in many areas for one to two days, satellite navigation may be degraded for days, low-frequency radio navigation can be out for hours, and aurora has been seen as low as Florida and southern Texas (typically 40 geomagnetic lat.)**. G 4 Severe Power systems: No impact on UK power grid. Power systems: possible widespread voltage control problems and some protective systems will Kp = 8, including a 9- i t k l t i t k t f th id Spacecraft operations: may experience surface charging and tracking problems, corrections may be needed for orientation problems. Spacecraft operations: may experience surface charging and tracking problems, corrections may be needed for orientation problems. Kp values* Average Frequency (1 cycle = 11 years) Number of storm events when Kp level was met; (number of storm days) 4 per cycle (4 days per cycle) 100 per cycle (60 days per cycle) Other systems: HF radio propagation sporadic, GPS satellite navigation degraded for hours, lowfrequency radio navigation disrupted, and aurora has been seen as low as 45 geomagnetic lat. Other systems: induced pipeline currents affect preventive measures, HF radio propagation sporadic, satellite navigation degraded for hours, low-frequency radio navigation disrupted, and aurora has been seen as low as Alabama and northern California (typically 45 geomagnetic lat.)**.

Services

Space weather models at the Met Office Sun to Earth: WSA Enlil At the Sun: CME analysis tools Van Allen Belts (1,000-60,000km): SPACECAST Geosynchronous orbit (~35,000km): REFM Ionosphere (50-600km): MIDAS Ionosphere (D-region, 50-90km): D-RAP

WSA Enlil model Purpose: Models solar wind speed & density from Sun to Earth (IMF modelled but no Bz input). Predicts CME arrival times at Earth, Inputs: WSA uses solar magnetograms to model coronal magnetic field and provide inner BCs for Enlil. CME analysis tools (NASA StereoCAT or NOAA CAT) calculate CME parameters using fit to STEREO A&B and LASCO images. CME parameters input into Enlil Output: Run every 2hrs Forecasts: average error: +_ 7 hrs (Doug Biesecker); lead time: CME transit time a few hrs

Other Products DRAP gives real time prediction of the absorption (radio propagation) conditions in the D region. FP7 project provides forecasts of particle radiation to aid satellite operation. REFM provides daily electron fluence forecasts at GEO orbit. Ionospheric analyses of European sector produced using MIDAS.

Verification Currently planning archiving of data for verification. REFM is currently compared with GOES fluence data on internal webpages. Plan to compare Enlil density & velocity with STEREO A, STEREO B & ACE. Metrics tables to show that forecasters are adding value to models. Verification of alerts, warnings & forecasts using methods already in use e.g. for flood forecasting. Met Office internal webpages

Modelling from Sun to Earth: Current R&D Status Goal: Coupled Sun to Earth models with DA for much enhanced forecast capacity M Owens (Reading Uni) X WSA Enlil Ensembles Solar wind persistence model for benchmarking / validation (Owens et al, 2013; Kohutova) Improved methods of tracking solar wind features (Tucker-Hood) Thermosphere: DA and ionosphere coupling Real time regional TEC (MIDAS) Whole atmosphere model plans

Modelling from Sun to Earth: Future System Goal: Coupled Sun to Earth models with DA for much enhanced forecast capacity WSA Enlil -like model: ensembles & improved solar wind via DA Implement existing or new magnetosphere model Coupled thermo / ionosphere DA. Whole atmos UM Flares SEPs model driven by Enlil, flare detection ---------------- near real time forecast verification ---------------- Apps (eg GIC models)

Summary Met Office Space Weather services available and being developed - 24/7 forecasting as of April. Associated R&D programme shall lead to pullthrough of improved services and operational forecasts. Large challenges call for interdisciplinary collaborations which utilise the skills of partners to maximum effect.

Questions and answers

Met Office Space Weather Research & Development - Extra Slides

Other solar wind modelling solar wind persistence model WSA Enlil benchmark and quick forecast tool CME drag model ensemble quick heads up of CME arrival times for forecasters RMS error of various model predictions of solar wind speed, relative to a reference model (Owens et al, 2013)

Active Region Tracking KSWC Automatic Solar Synoptic Analyser: Magnetic classification, Flare forecasting, Coronal hole detection, Filament detection. Further development in collaboration with Trinity College Dublin. (eg Solar Monitor Active Region Tracker (SMART; Higgins et al) S. Murray