SIDC Space Weather Briefing

Slides:



Advertisements
Similar presentations
Space Environment Center Service Start to Finish Joe Hirman SEC Lab Review July 2000.
Advertisements

Space Weather User Needs Related to Solar Observations Eamonn Daly and Alexi Glover ESA Space Environments and Effects Section ESTEC, The Netherlands.
Space Weather Effects over EGNOS Performance in the North of Europe 11 th SWW, Liege, 17 th November 2014 Presenter author: Pedro Pintor Authors: R. Roldán,
PARTS V: GEOMAGNETIC INDICES Observed, estimated, and predicted daily geomagnetic AFr-indices (A- indices from Fredericksburg, VA), and daily AP-indices.
1 Grades 3 - 5: Introduction. 2 Better Observation Of The Sun And Earth Importance of Space Technology.
E. Robbrecht – SIDC- Royal Observatory of Belgium 8 March 2007 The statistical importance of narrow CMEs Open questions to be addressed by SECCHI Eva Robbrecht,
Discussion Summary: Group B –Solar Active Regions And Their Production of Flares and Coronal Mass Ejections Discussion Leaders: George Fisher Hugh Hudson.
Space Weather Forecast With HMI Magnetograms: Proposed data products Yang Liu, J. T. Hoeksema, and HMI Team.
Sung-Hong Park Space Weather Research Laboratory New Jersey Institute of Technology Study of Magnetic Helicity and Its Relationship with Solar Activities:
Agenda: Here comes the sun March 21 1.Learning Target: I can explain my Science Fair project to other Astronomers 2.Kick-off: What was the most interesting.
Announcements Observing Monday-Thursday of this week counts on the third exam. Fourth exam is Wednesday, November 17 Review will be Monday, November 15.
The Sun Our Nearest Star. The Source of the Sun’s Energy The Source of the Sun’s Energy Fusion of light elements into heavier elements. Hydrogen converts.
Locating the solar source of 13 April 2006 Magnetic Cloud K. Steed 1, C. J. Owen 1, L. K. Harra 1, L. M. Green 1, S. Dasso 2, A. P. Walsh 1, P. Démoulin.
Mark DierckxsensSpace Weather and Solar Energetic Particles1 M. Dierckxsens 1, K. Tziotziou 2, S. Dalla 3, I. Patsou 2, M. Marsh 3, N. Crosby 1, O. Malandraki.
Space Weather from Coronal Holes and High Speed Streams M. Leila Mays (NASA/GSFC and CUA) SW REDISW REDI 2014 June 2-13.
K9LA Vancouver 2003 Disturbances to Propagation Carl Luetzelschwab K9LA CQ DX?Where’d everybody go?
The Solar Wind.
CASS/UCSD - Jeju 2015 A Jets in the Heliosphere: A Solar Wind Component B.V. Jackson, H.-S. Yu, P.P. Hick, and A. Buffington, Center for Astrophysics and.
The Sun Stellar Evolution: Low Mass Stars White Dwarfs
Sunny Spells and Solar Storms: understanding space weather with LUCID.
Direct Spatial Association of an X-Ray Flare with the Eruption of a Solar Quiescent Filament Gordon D. Holman and Adi Foord (2015) Solar Seminar on July.
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.
Analysis of 3 and 8 April 2010 Coronal Mass Ejections and their Influence on the Earth Magnetic Field Marilena Mierla and SECCHI teams at ROB, USO and.
1 SPACE WEATHER SPACE WEATHER. 2 Causes of space weather Space weather is caused mainly by storms and eruptions in our volatile Sun sending potentially.
The Solar Wind. The Sun is not a quiet place. Disturbances in the Sun’s magnetic field create Sunspots.
Multi-Point Observations of The Solar Corona for Space weather Acknowledgements The forecasting data was retrieved from NOAA SWPC products and SIDC PRESTO.
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.
National Oceanic and Atmospheric Administration, April 2015 Coordination Group for Meteorological Satellites - CGMS NOAA: Space Weather Overview Presented.
The COMESEP Space Weather Alert System Luciano Rodriguez on behalf of the COMESEP Consortium (European Commission FP7 Project )
Manuela Temmer Institute of Physics, University of Graz, Austria Tutorial: Coronal holes and space weather consequences.
STCE annual meeting 7 June, 2011
Driving 3D-MHD codes Using the UCSD Tomography
ICME in the Solar Wind from STEL IPS Observations
Scientists demonstrate a new Solar Energetic Particle warning technique using K-COR ground coronagraph data A Heliophysics science publication using ESA/NASA.
Introduction to Space Weather Interplanetary Transients
SIDC Space Weather briefing
Met Office Forecaster and Customer Requirements and Rationale
Comprehensive analysis of the Geoeffective Solar Event of June 21, 2015: Effects on the Magnetosphere, Plasmasphere and Ionosphere Systems - part 1. Francesca.
The Not-So-Calm After the Storm:
Anemone Structure and Geo-Effective Flares/CMEs
Forecasting the arrival time of the CME’s shock at the Earth
D. Paronis1 , P. Jiggens3 , A. Hilgers3
Anemone Structure of AR NOAA and Related Geo-Effective Flares and CMEs
SIDC Space Weather briefing
Quantification of solar wind parameters from measurments by SOHO and DSCOVR spacecrafts during series of Interplanetary Coronal Mass Ejections in the.
. Multipoint, galactic cosmic ray observations associated with a series of interplanetary coronal mass ejections: the case study of June 2015 A. Papaioannou1,
Introduction to Space Weather
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
Grades 3 - 5: Introduction
Ju Jing, Vasyl B. Yurchyshyn, Guo Yang, Yan Xu, and Haimin Wang
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
Grades 3 - 5: Introduction
Filament/Prominence Eruption Corona Mass Ejection (CME)
Richard B. Horne British Antarctic Survey Cambridge UK
An MHD Model for the Formation of Episodic Jets
Added-Value Users of ACE Real Time Solar Wind (RTSW) Data
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
SIDC Space Weather Briefing
CORONAL MASS EJECTIONS
SIDC Space Weather Briefing
SIDC Space Weather Briefing
Presentation transcript:

SIDC Space Weather Briefing 26 May 2019 - 02 June 2019 Judith de Patoul & the SIDC forecaster team

Summary Report Solar activity from 2019-05-26 12:00 UT to 2019-06-02 12:00 UT Active regions The Sun was spotless Flaring # B-class flare: 1 # C-class flare: 0 # M-class flare: 0 # X-class flare: 0 Filaments No filament eruption CMEs No CME observed Proton Events No proton Event Solar wind and geomagnetic conditions from 2019-05-26 12:00 UT to 2019-06-02 12:00 UT Coronal Holes Few small patches of equatorial coronal hole ICME One shock like event on May 26, 2019, at 21:25 UT SW Conditions Fast solar wind speed: max 566 km/s on May 29 K-indices max K-index (Dourbes): 3.0 max Kp-index (NOAA): 4.0 All Quiet Alert: All quiet from May 30.

Solar Activity

Solar active region - start of the week SDO/HMI White Light 2019-05-26 SDO/HMI Magnetogram 2019-05-26

Solar active region - middle of the week SDO/HMI White Light 2019-05-29 SDO/HMI Magnetogram 2019-05-29

Solar active region - end of the week SDO/HMI White Light 2019-06-02 SDO/HMI Magnetogram 2019-06-02

Solar active region & Coronal hole SDO/AIA 19.3 nm 2019-05-26 SDO/AIA 19.3 nm 2019-06-02

Solar F10.7cm radio flux

Flaring activity Probabilities (%) and occurrences (#) of B/C/M/X-flares issued at 12:30 and over the next 24h: Issue date 2019-05-26 2019-05-27 2019-05-28 2019-05-29 2019-05-30 2019-05-31 2019-06-01 2019-06-02 Probability ---|01|01|01 Observed 00|00|00|00 01|00|00|00

Coronal Mass Ejection

Solar proton flux

Solar Wind and Geomagnetic Activity

Solar wind parameters (DSCOVR data)

Coronal Mass Ejection Last space weather briefing: 19 May 2019 - 26 May 2019 Jennifer O’Hara & the SIDC forecaster team

Solar wind parameters (DSCOVR data)

Geomagnetic activity (K-indexes)

Outlook

Outlook: Solar activity

Outlook: Solar wind

Outlook: Solar wind

Outlook: Solar wind

Outlook: Geomagnetic activity

SIDC Space Weather Briefing See you at our next briefing! Or visit us at www.sidc.be