SPAIN'S NATIONAL ASSETS

Slides:



Advertisements
Similar presentations
Automatic prediction of SEP events and the first hours of their proton fluxes with E > 10 MeV and E > 100 MeV Marlon Núñez Universidad de Málaga, Spain.
Advertisements

Cosmic Rays and Space Weather
Space Environment Center Service Start to Finish Joe Hirman SEC Lab Review July 2000.
Space Weather in CMA Xiaonong Shen Deputy Administrator China Meteorological Administration 17 May 2011 WMO Cg-XVI Side Event Global Preparedness for Space.
Space Weather User Needs Related to Solar Observations Eamonn Daly and Alexi Glover ESA Space Environments and Effects Section ESTEC, The Netherlands.
The Johns Hopkins University Applied Physics Laboratory SHINE 2005, July 11-15, 2005 Transient Shocks and Associated Energetic Particle Events Observed.
On the link between the solar energetic particles and eruptive coronal phenomena On the link between the solar energetic particles and eruptive coronal.
Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
Space Research Institute Short-term space weather forecast A.A. Petrukovich Space Research Institute, Russian Academy of Sciences with contributions from.
I. U. Observatorio del Ebro, Universitat Ramon Llull Center for Atmospheric Research, University of Massachusets Lowell IRI/COST 296 WORKSHOP; July.
ESA SSA Programme Objective:
Solar Energetic Particle Production (SEPP) Mission Primary Contacts: Robert P. Lin (UC Berkeley), John L. Kohl (Harvard-Smithsonian CfA) Primary Science.
Space Weather Forecast Models from the Center for Integrated Space Weather Modeling The Solar Wind Forecast Model Carrington Rotation 1896Carrington Rotation.
Session 1 Hot topics in Space Weather. Space weather of the past weekend.
ESA SSA SWE element status and near future plans 7th European Space Weather Week November, Brugge, Belgium Juha-Pekka Luntama Space Weather.
GEANT-4/Spenvis User Meeting November 2006 Solar Energetic Particle Modelling Activities at ESA A.Glover 1, E. Daly 1,A. Hilgers 1, SEPEM Consortium 2.
PHOEBUS* on LISA: A Proposal for Solar Physics on LISA INFN-SPAZIO/2 Riunione sulle prospettive della Fisica Astroparticellare nello spazio LNF, 16 Febbraio.
14-18 Nov 2005ESWW – SAAPS1 SAAPS Spacecraft Anomaly Analysis and Prediction System ESA Contract 11974/96/NL/JG(SC) Two year project (April 1999 – June.
1 Introduction The TOP-modelPotential applicationsConclusion The Transient Observations-based Particle Model and its potential application in radiation.
System for Radiation Environment characterization (fluxes, doses, dose equivalents at Earth, Moon and Mars) on hourly thru yearly time frame Example: Snapshots.
K9LA Vancouver 2003 Disturbances to Propagation Carl Luetzelschwab K9LA CQ DX?Where’d everybody go?
China National Report , Uppsala, Sweden China National Space Administration.
Nowcast model of low energy electrons (1-150 keV) for surface charging hazards Natalia Ganushkina Finnish Meteorological Institute, Helsinki, Finland.
29 August, 2011 Beijing, China Space science missions related to ILWS in China
Space Weather Modelling: from Science to Applications Chair: M. Dinguirard ONERA.
NMDB - the European neutron monitor database Karl-Ludwig Klein, for the NMDB consortium.
Earth-Moon-Mars Radiation Environment Model N. A. Schwadron, K. Kozarev, L. Townsend, M. Desai, M. A. Dayeh, F. Cucinotta, D. Hassler, H. Spence, M. Pourars,
Japan, ICRC 2003 Daejeon, UN/ESA/NASA/JAXA Workshop, Sept 2009 Satellite Anomalies and Space Weather By Lev Dorman for INTAS team (A. Belov, L. Dorman,,
Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO
Solar and Cosmic Ray Energetic Particle Models : Space Weather Aspects
What we can learn from the intensity-time profiles of large gradual solar energetic particle events (LGSEPEs) ? Guiming Le(1, 2,3), Yuhua Tang(3), Liang.
CRRES observations indicate an abrupt increase in radiation belt fluxes corresponding to the arrival of a solar wind shock. The processes(s) which accelerate.
What is a geomagnetic storm? A very efficient exchange of energy from the solar wind into the space environment surrounding Earth; These storms result.
Thermospheric density variations due to space weather Tiera Laitinen, Juho Iipponen, Ilja Honkonen, Max van de Kamp, Ari Viljanen, Pekka Janhunen Finnish.
The CME geomagnetic forecast tool (CGFT) M. Dumbović 1, A. Devos 2, L. Rodriguez 2, B. Vršnak 1, E. Kraaikamp 2, B. Bourgoignie 2, J. Čalogović 1 1 Hvar.
Space Weather Services to Build Global Resilience Expert Meeting on Space Weather Services February 3, 2015 – UNCOPUOS STSC Assembly Goal: Foster greater.
Space Weather Service in Indonesia Clara Y. Yatini National Institute of Aeronautics and Space (LAPAN)
ISES Director’s Report Terry Onsager, April 9, 2015 Accomplishments Actions from 2014 Annual Meeting Complementary Activities Challenges.
National Oceanic and Atmospheric Administration, April 2015 Coordination Group for Meteorological Satellites - CGMS NOAA: Space Weather Overview Presented.
1 Test Particle Simulations of Solar Energetic Particle Propagation for Space Weather Mike Marsh, S. Dalla, J. Kelly & T. Laitinen University of Central.
30 April 2009 Space Weather Workshop 2009 The Challenge of Predicting the Ionosphere: Recent results from CISM. W. Jeffrey Hughes Center for Integrated.
KMA Space Weather Service Presented to CGMS-44 on Working Group SWTT.
Contact: Dr. Johannes Labrenz Extraterrestrische Physik Institut für Experimentelle und Angewandte Physik Christian Albrechts-Universität.
EGU General Assembly 2016 Contact: Dr. Johannes Labrenz
EGU General Assembly 2016 Contact: Dr. Johannes Labrenz
Driving 3D-MHD codes Using the UCSD Tomography
2016 Solar Storms with NASA/NOAA GOES-R Satellite Primed to Support Space Weather Predictive Capabilities On 20 December 2016 Earth encountered a stream.
Future SWE Missions Workshop ESA SSA/SWE State-of-Play
Solar Energetic Particle Environment Modelling: Pre-Release of the SEPEM Project Norma Crosby1, Alexi Glover2, Angels Aran2, Cédric Bonnevie3, Clive Dyer4,
ESA SSA Measurement Requirements for SWE Forecasts
The Instruments Faraday Cup CfA/U of Mich & MIT
A joint study of the University of Göttingen (1) and Astrium (2)
M.J. Rivas [1,2], C. Cid [1] RELATIONSHIP BETWEEN THE INTENSITY OF X-RAY FLARES AND THEIR EFFECTS IN THE HORIZONTAL COMPONENT OF THE.
Solar Energetic Particle Environment Modelling: Pre-Release of the SEPEM Project Norma Crosby1, Alexi Glover2, Angels Aran2, Cédric Bonnevie3, Clive Dyer4,
Utilizing Scientific Advances in Operational Systems
ARTEMIS – solar wind/ shocks
Marlon Núñez and David A. Núñez Universidad de Málaga
EGU General Assembly 2016 Contact: Dr. Johannes Labrenz
Introduction to Space Weather Interplanetary Transients
Spacecraft Anomaly Analysis and Prediction System – SAAPS
P2-SWE-X Enhanced Space Weather Monitoring System ESWW13
Earth-Moon-Mars Radiation Environment Model
Solar and Heliospheric Physics
Environmental conditions during the charging anomaly of the two geosynchronous satellites reported: TELSTAR 401 and Galaxy 15 Elena Saiz, A. Guerrero,
Introduction to Space Weather
P. Stauning: The Polar Cap (PC) Index for Space Weather Forecasts
NMDB - the European neutron monitor database
Toshiyuki Kurino, WMO Space Programme
Searching for relationships between the solar regular daily magnetic variation at mid latitude and the solar irradiance at different ionizing wavelengths.
Added-Value Users of ACE Real Time Solar Wind (RTSW) Data
Presentation transcript:

SPAIN'S NATIONAL ASSETS Consuelo Cid (consuelo.cid@uah.es) SRG-Space Weather, University of Alcalá

Solar – Terrestrial Physics and Dept. d’Astronomia i Meteorologia Facultat de Física Solar – Terrestrial Physics and Space Weather Group (STP/SWG) Contact: Dr. Blai Sanahuja Phone: 34-934021131 e-mail: Blai.Sanahuja@ub.edu web: www.am.ub.es/~blai

Solar-Interplanetary energetic particle events ● Space observations and data analysis - Solar wind plasma, interplanetary magnetic field, energetic particles, related solar activity. - WIND, ACE, SOHO, ISEE-3, Ulysses, IMPs, GOES, HELIOS, etc. ● Modeling energetic (gradual protons, impulsive electrons) events - Particle transport in interplanetary space: Numerical resolution and Monte Carlo applications - 2D magnetohydrodinamic modeling of interplanetary (ICME) shocks ● Space Weather applications - The tool SOLPENCO (Solar Particle Engineering Code) Provide the capability to quantitatively and rapidly predict upstream particle fluxes and fluences generated by shocks. - Under development: SOLPENCO2 code within ESA’s SEPEM Project

Univ. of Málaga asset: UMA SEP Forecaster Characteristics of the UMA SEP forecaster: Real-time prediction of the onset and intensity of the prompt component (first hours) of well-connected SEPs (wcSEPs). Based on the estimation of the magnetic connectivity, which is deduced by correlating X-ray and Proton data at 1 AU. Real-time source: 5 min. data from the available GOES satellites. Servers downloading 5 min. forecasts: SEIS (2007), ESWP (nov. 2009) Evaluation (solar cycles 22 and 23): Probability of wcSEP prediction: 84% Missed wcSEP rate: 16% False alarm rate: 45% Max. warning time: 6:10 hours Intensity RMSError: 0.58 (log. scale) UMA SEP forecaster output: http://spaceweather.uma.es/forecastpanel.htm A forecast of a well-connected SEP

Space Research Group Space Weather C. Cid, E. Saiz, Y . Cerrato and J. Aguado Contact: consuelo.cid@uah.es http://www2.uah.es/srg_spaceweather/

Solar wind plasma and interplanetary magnetic field Data analysis: Solar wind plasma and interplanetary magnetic field Geomagnetic indices Solar activity related Physic-based modelling: Magnetic clouds (ICMEs) Terrestrial surface response to solar wind transients and recovery to quiet state Products and Applications: UAH Space Weather Monitor http://www2.uah.es/srg_spaceweather/forecasting.html

Ebro Observatory Assets D. Altadill, E. Blanch, J. M. Torta and J. J. Curto Observatorio del Ebro Universitat Ramon Llull - CSIC Roquetes, Spain

Ebro Observatory (40.8 N, 0.5 E) Instruments Data Activities - Vector magnetometer stations. - Ionospheric radio sounding station (DGS256 UML). Data - Geomagnetic field elements, Local magnetic indices and Geomagnetic rapid variations. - Real-time Ionograms, Ionospheric Characteristics and Density profiles. - Post-processed Ionospheric Data. Activities - Local magnetic field monitoring, Modeling of Sq and Sfe currents, SSC and Geomagnetic Storms. - Local ionospheric monitoring, Modeling of Ionospheric climatology and Solar driven disturbances.

INTA potential SSA Assets Long Ionosphere monitoring expertise and capabilities – INTA ‘El Arenosillo’ ground station Small Satellite platforms for Space Weather monitoring: OPTOS (3 kg), Nanosat (18 Kg) and MicroSat (40-60 Kg) Development of Radiation Effects Monitors for Housekeeping purposes Long Expertise in space payload development for scientific purposes. Space Weather Operational Tools for satellite operations support. SESS, SEISOP projects

SEISOP Space Environment Information System for Operations Delivery of a set of Space Weather services & products Capabilities: Ingestion, processing, classification and storage of Space Weather data from a variety of external /internal sources Space Weather data and satellite effects monitoring Space Weather data nowcasting & forecasting Satellite operators specific products and tools Multimission, site-independent, distributed Fully customizable through metadata Data policy & governance compatible with SSA Provides easy-to-use interface for usage from external entities Products: Space Weather data, metadata & satellite effects, including nowcasting, forecasting, monitoring, reporting & web access Space Weather events & alarms