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.

PARTS V: GEOMAGNETIC INDICES Observed, estimated, and predicted daily geomagnetic AFr-indices (A- indices from Fredericksburg, VA), and daily AP-indices.

Reviewing the Summer School Solar Labs Nicholas Gross.

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.

PROGRESS IN SPACE WEATHER PREDICTIONS AND APPLICATIONS ZEYNEP KOCABAŞ METU AEE 2005.

Sung-Hong Park Space Weather Research Laboratory New Jersey Institute of Technology Study of Magnetic Helicity and Its Relationship with Solar Activities:

NOAA Space Environment Center The Status of Solar Cycle 23 Joe Kunches Chief, Space Weather Operations NOAA Space Environment Center Boulder, Colorado.

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.

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.

Weather Briefing for The 2013 Presidential Inauguration NOAA / National Weather Service Baltimore/Washington Weather Forecast Office January 21,

K9LA Vancouver 2003 Disturbances to Propagation Carl Luetzelschwab K9LA CQ DX?Where’d everybody go?

National Aeronautics and Space Administration NASA Goddard Space Flight Center Software Engineering Division Overview of Significant SWx Events.

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.

Sunny Spells and Solar Storms: understanding space weather with LUCID.

Improving Space Weather Forecasts Using Coronagraph Data S.P. Plunkett 1, A. Vourlidas 1, D.R. McMullin 2, K. Battams 3, R.C. Colaninno 4 1 Naval Research.

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.

What is a geomagnetic storm? A very efficient exchange of energy from the solar wind into the space environment surrounding Earth; These storms result.

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.

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.

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.

Detecting, forecasting and modeling of the 2002/04/17 halo CME Heliophysics Summer School 1.

Driving 3D-MHD codes Using the UCSD Tomography

Space Weather in situ measurements perspective

Chengming Tan National Astronomical Observatories

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:

CDS Images at Different Spectral Lines - Temperatures

Forecasting the arrival time of the CME’s shock at the Earth

Solar and Heliospheric Physics

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,

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

Károly Kecskeméty KFKI RMKI Budapest, Hungary

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)

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

SIDC Space Weather Briefing

CORONAL MASS EJECTIONS

SIDC Space Weather Briefing

SIDC Space Weather Briefing

Presentation transcript:

SIDC Space Weather Briefing 17 March 2019 - 24 March 2019 Luciano Rodriguez & the SIDC forecaster team

Summary Report Solar activity from 2019-03-17 12:00 UT to 2019-03-24 12:00 UT Active regions NOAA ARs 2735 and 2736 Flaring 13 C-class flares (2736) CMEs 1 with an Earth directed component Proton Events None Solar wind and geomagnetic conditions from 2019-03-17 12:00 UT to 2019-03-24 12:00 UT Coronal Holes 1 small, positive polarity ICME Only a shock arrived SW Conditions Slow solar wind (V < 450 km/s) K-indices max K-index (Dourbes): 3.0 max Kp-index (NOAA): 3 All Quiet Alert: Off

Solar Activity

Solar active region - start of the week SDO/HMI White Light 2019-03-17 SDO/HMI Magnetogram 2019-03-17

Solar active region - middle of the week SDO/HMI White Light 2019-03-20 SDO/HMI Magnetogram 2019-03-20 2736 2735

Solar active region - end of the week SDO/HMI White Light 2019-03-24 SDO/HMI Magnetogram 2019-03-24 2736 2735

Solar active region & Coronal hole SDO/AIA 19.3 nm 2019-03-17 SDO/AIA 19.3 nm 2019-03-24 +, HSS arrived on March 19 -, HSS expected on March 26

Solar F10.7cm radio flux

Solar X-Ray and UV flux

Flaring activity Probabilities (%) and occurrences (#) of B/C/M/X-flares issued at 12:30 and over the next 24h: Issue date 2019-03-17 2019-03-18 2019-03-19 2019-03-20 2019-03-21 2019-03-22 2019-03-23 2019-03-24 Probability ---|01|01|01 ---|05|01|01 ---|10|01|01 ---|75|15|01 ---|70|15|01 ---|80|20|05 ---|50|05|01 ---|45|05|01 Observed 00|00|00|00 04|00|00|00 03|00|00|00 18|03|00|00 22|09|00|00 35|01|00|00 25|00|00|00 10|00|00|00

Coronal Mass Ejection SWAP

Coronal Mass Ejection COR2A LASCO - AIA

Solar proton flux

Solar Wind and Geomagnetic Activity

Solar wind parameters (DSCOVR data)

Solar wind parameters

Solar wind parameters & K-index (DSCOVR/Dourbes)

Geomagnetic activity (K-indexes)

Outlook

Outlook: Solar activity

Outlook: Solar wind

Outlook: Geomagnetic activity

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