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.

Suzdal, 2007 THE SOLAR GEOEFFECTIVE PHENOMENA: INFLUENCE ON THE SPACE ENVIRONMENT AND THE POSSIBILITY OF THEIR FORECAST V.N. Ishkov, IZMIRAN

An overview of the cycle variations in the solar corona Louise Harra UCL Department of Space and Climate Physics Mullard Space Science.

1 Hinode Coordinated Observations: Plasma Composition Photospheric composition ~ 1 in coronal hole (CH) -> fast wind Coronal composition ~1.5-3 in active.

The Solar Terrestrial Activity Report

CME Workshop Elmau, Feb , WORKING GROUP C: ENERGETIC PARTICLE OBSERVATIONS Co-Chairs: Klecker, Kunow SUMMARY FROM WORKSHOP 1 Observations Questions.

STEREO AND SPACE WEATHER Variable conditions in space that can have adverse effects on human life and society Space Weather: Variable conditions in space.

30-Day Science Plan Angelos Vourlidas, Russ Howard SECCHI Consortium Meeting IAS 8 March 2007.

HMI/AIA Science Team Meeting, HMI Science Goals Alexander Kosovichev & HMI Team.

Solar Activities and Halloween Storms Ahmed Hady Astronomy Department Cairo University, Egypt.

Photospheric Sources of Very Fast (>1100km/s) Coronal Mass Ejections Recent studies show that only very fast CMEs (> 1100 km/s) are capable of producing.

The Dangers of Solar Storms and Solar Cycles.  For every 1 million atoms of hydrogen in the entire sun  98,000 atoms of helium  850 of oxygen  360.

A Catalog of Halo Coronal Mass Ejections from SOHO N. Gopalswamy 1, S. Yashiro 2, G. Michalek 3, H. Xie 3, G. Stenborg 2, A. Vourlidas 4, R. A. Howard.

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.

Emily Linden Bear Elder. An enormous amount of energy being released Takes a matter of minutes to explode over a space Some piece of materials breaks.

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 Dangers of Solar Storms and Solar Cycles.  Radius = 696,000 km  Mass = 2E30 kg  Luminosity = 3.8E26 W  Rotation Rate  25 days at the equator.

The Sun Stellar Evolution: Low Mass Stars White Dwarfs

Heliospheric Observations during October – November 2003 Hari Om Vats Physical Research Laboratory Ahmedabad INDIA ICRC.

Synoptic Network Workshop (HAO/NCAR, April 2013) Space Weather and Synoptic Observations V J Pizzo – NOAA/SWPC.

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.

Solar Astronomy Space Science Lab 2008 Pisgah Astronomical Research Institute.

SEC Directed Research Retreat 12–13 February 2004 Science we do now GUIDELINES AND BALANCE Directed Research Retreat Feb

Joint Planning of SOT/XRT/EIS Observations Outline of 90 Day Initial Observing Plans T. Shimizu, L Culhane.

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.

17 th November, 2005STEREO/Solar-B Workshop 1 Related Solar Imaging and Near-Earth In-situ Observations of an ICME A. N. Fazakerley 1, L.K. Harra 1, J.L.

Multi-Point Observations of The Solar Corona for Space weather Acknowledgements The forecasting data was retrieved from NOAA SWPC products and SIDC PRESTO.

Agenda: Here comes the sun March 18 and 21 1.Learning Target: I can describe how sunspots are important 2.Agenda 1.Danger Solar Storm DVD and Questions.

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.

The COMESEP Space Weather Alert System Luciano Rodriguez on behalf of the COMESEP Consortium (European Commission FP7 Project )

KMA Space Weather Service Presented to CGMS-44 on Working Group SWTT.

Mid-term Periodicities of the LYRA data spectrum

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

Solar Wind Transients and SEPs

HMI Data Analysis Pipeline

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

Anemone Structure of AR NOAA and Related Geo-Effective Flares and CMEs

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,

HMI Data Analysis Pipeline

Solar Sources of Wide Coronal Mass Ejections during the Ascending Phase of Cycle 24 Sachiko Akiyama1,2, Nat Gopalswamy2, Seiji Yashiro1,2 , and Pertti.

Introduction to Space Weather

SIDC Space Weather Briefing

SIDC Space Weather Briefing

SIDC Space Weather Briefing

The Centre of the Solar System Earth Science 11

SIDC Space Weather Briefing

SIDC Space Weather Briefing

SIDC Space Weather Briefing

SIDC Space Weather Briefing

SIDC Space Weather Briefing

SIDC Space Weather Briefing

Sushanta C. Tripathy National Solar Observatory

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 25 June – 01 July 2018 Jasmina Magdalenic & SIDC forecaster team Solar Influences Data analysis Centre www.sidc.be

Summary Report Active Regions Flaring Wide CMEs NOAA AR 2715 Flaring 3 B-class flares Wide CMEs No Large Filaments eruptions Proton Events SW conditions Max solar wind speed: 660 km/s Coronal Holes Equatorial coronal hole reached central meridian on June 21 Shocks No. ICME Kp index NOAA Kp=5 & Dourbes K=5

Solar active region evolution 3

Solar active region evolution Only one sunspot group was observed on the visible side of the solar disc this week; Catania sunspot group 88 (NOAA AR 2715). 4

Solar X-ray flux and flaring 3 low B-class flares (all originating from Catania sunspot group 88, i.e. NOAA AR 2715). 27 Feb 2017: 6780 + 2007 2017 2025 G15 5 XRA 1-8A B9.3 6.3E-04 2641 28 Feb 2017: 6840 + 1142 1151 1215 G15 5 XRA 1-8A B7.7 1.0E-03 2641 5

CMEs detected by Cactus No wide CMEs reported this week. (Not a CME)

Energetic particles No particle events reported this week.

Solar wind Fast flow Fast flow???

Solar wind

Solar wind

Geomagnetism Fast solar wind

Outlook