Solar-terrestrial connections – any future? We enter global minimum – maybe Maunder minimum? (Yuri Stogkov) In science it is of greatest importance to.

Slides:



Advertisements
Similar presentations
Investigation of daily variations of cosmic ray fluxes in the beginning of 24 th solar activity cycle Ashot Chilingarian, Bagrat Mailyan IHY-ISWI Regional.
Advertisements

Sunspots and the Scientific Method: Models. Hypothesis Driven Science Hypothesis: An educated speculation about how a particular phenomenon behaves- very.
An overview of the cycle variations in the solar corona Louise Harra UCL Department of Space and Climate Physics Mullard Space Science.
The Sun Structure of the Sun & Solar Activity. Parts of the Sun Core: enormous pressure & high temperatures cause the fusion of hydrogen into helium.
Structure of the Sun & Solar Activity
29 April 2011Viereck: Space Weather Workshop 2011 The Recent Solar Minimum: How Low Was It? What Were The Consequences? Rodney Viereck NOAA Space Weather.
Propagation Index and Short Wave Communications Rodney Wolfe N3XG.
EXPLORING THE SUN’S MAGNETIC INFLUENCE April 23, 2015 LT: I can model how certain forces are able to act on an object from a distance Please get a post.
General Findings Concerning the Magnetospheric Realm ILWS - 11 Science Workshop, Beijing, China, Aug-Sep 2011.
The Effects of Geomagnetic Storms on Power Systems Mary Holleboom Justin Voogt ENGR W82 January 22, 2002.
CH – Solar Activity CH MARQUES. Terms to know…  Sunspot  Prominence  Granules  solar flare  coronal mass ejection  aurora.
1 Grades 3 - 5: Introduction. 2 Better Observation Of The Sun And Earth Importance of Space Technology.
PROGRESS IN SPACE WEATHER PREDICTIONS AND APPLICATIONS ZEYNEP KOCABAŞ METU AEE 2005.
Periodicities of the Solar Wind, Global Electron Power, and Other Indices in 2005 in HSS Barbara A. Emery (NCAR), Ian G. Richardson (GSFC), David S. Evans.
The “cone model” was originally developed by Zhao et al. ~10 (?) years ago in order to interpret the times of arrival of ICME ejecta following SOHO LASCO.
Physics 681: Solar Physics and Instrumentation – Lecture 25 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
f has a saddle point at (1,1) 2.f has a local minimum at.
NEW SOLAR MINIMUM AND THE MINI-ICE AGE OF THE 21 st CENTURY Ph.D. Víctor Manuel Velasco Herrera Institute of Geophysics, UNAM, México The Sun sows again.
Belle Tamir, Sharet High School Nitzan Atia, Tchernichovsky High School Netanya, Israel.
The active Sun. The magnetic Sun White lightMagnetic field.
The Active Sun. Sunspots Umbra Penumbra Granulation.
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.
Fundamental properties of the Sun. Last time Described the Sun’s size (diameter), mass, chemical composition, and temperature Today, additional features.
This is the graph of y = sin xo
Space Weather Major sources of space weather ● Solar wind – a stream of plasma consisting of high energy charged particles released from the upper atmosphere.
Statistical Analysis of Solar Geomagnetic Storm Occurrences By: Seth Sivak.
Chapter 9 The Sun. 9.4 The Active Sun Sunspots: appear dark because slightly cooler than surroundings:
Ham Fair K9LA Solar Cycle 23 and Early Predictions for Solar Cycle 24 Carl Luetzelschwab K9LA.
The Sun ROBOTS Summer Solar Structure Core - the center of the Sun where nuclear fusion releases a large amount of heat energy and converts hydrogen.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 1 Announcements: Spring Break: next week!! Exam #2: Thursday,
Space Weather from Coronal Holes and High Speed Streams M. Leila Mays (NASA/GSFC and CUA) SW REDISW REDI 2014 June 2-13.
The SUN!.
The Relations Between Solar Wind Variations and the North Atlantic Oscillation Rasheed Al-Nuaimi and Kais Al-Jumily Department of Atmospheric Sciences.
The Sun- Solar Activity. Damage to communications & power systems.
Propagation Trends Dayton 2014 Solar Maximum! But the slow decline to solar minimum in 2020 is likely to begin later this year.
Geoeffectiveness of Solar and Interplanetary Events Yuri I. Yermolaev, Michail Yu. Yermolaev, Georgy N. Zastenker, Anatoli A. Petrukovich, Lev M. Zelenyi.
Recent ‘Unprecedented’ Weak Solar Wind: A solar glitch or a harbinger for the next Maunder minimum? Conveners: Joan Feynman* and Janet Luhmann When: Wednesday.
THE SUN. The Sun The sun has a diameter of 900,000 miles (>100 Earths could fit across it) >1 million Earths could fit inside it. The sun is composed.
The Sun: a star close up. The Sun in a stellar context: a spectral class G main sequence star.
Heliospheric Observations during October – November 2003 Hari Om Vats Physical Research Laboratory Ahmedabad INDIA ICRC.
Solar Astronomy Space Science Lab 2008 Pisgah Astronomical Research Institute.
1 Grades 6-8: Introduction. 2 Aerospace Technology Space Science Human Exploration And Development Of Space Earth Science Main Areas Of Research.
Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during.
Statistical Analysis of Geomagnetic Storm Occurrences By: Seth Sivak.
Ahmed A. HADY Astronomy Department Cairo University Egypt Deep Solar Minimum of Cycle23 and its Impact and its Impact.
What is a geomagnetic storm? A very efficient exchange of energy from the solar wind into the space environment surrounding Earth; These storms result.
CSI /PHYS Solar Atmosphere Fall 2004 Lecture 04 Sep. 22, 2004 Solar Magnetic Field, Solar Cycle, and Solar Dynamo.
 Caused by the magnetic field of the sun  Charged particles spiral along magnetic field lines We draw magnetic field lines (red) to represent invisible.
1.  When we look at the Sun (NEVER EVER look directly at the Sun) we often see that there’s more to it than just a ball of hot gas.  Sunspots  Prominences.
THE SUN The star we see by day.
The Decline to Solar Minimum 2014 through about 2020
Variable Sun-Earth energy coupling: dependence on solar cycle strength
Solar Activity and Space Weather
The Sun: close-up of a spectral class G main sequence star
The Earth The Earth.
MDI Global Field & Solar Wind
Quadratic Functions.
The Sun Chapter 17.
Section 2: Solar Activity
The Sun as We See It Lecture 9
Solar Activity Chapter 8 Section 3.
Chapter 9 The Sun.
EDLC(Embedded system Development Life Cycle ).
NEW SOLAR MINIMUM AND THE MINI-ICE AGE OF THE 21 st CENTURY
Grades 3 - 5: Introduction
X y y = x2 - 3x Solutions of y = x2 - 3x y x –1 5 –2 –3 6 y = x2-3x.
Grades 9-12: Introduction
Grades 3 - 5: Introduction
Extreme Space Weather as an Emerging Risk
By: CAEDEN , CORnbud , DYLAN
Presentation transcript:

Solar-terrestrial connections – any future? We enter global minimum – maybe Maunder minimum? (Yuri Stogkov) In science it is of greatest importance to choose right direction very early – CRD start TGE research from 2008! How to proceed with our networks – SEVAN and ASEC for solar physics? Minimum of solar wind – maximum of particles! Present CRD results on the Solar-terrestrial physics in the best way. Look for possible new papers! Work with SEVAN hosts, think about new physics!

Progress of the 24-th cycle: maximum in 2013?

The cycle 24 will probably mark the end of the Modern Maximum

Upcoming Solar Cycle 24 will be similar to the cycle that peaked in 1928 

Kp=4 Geomagnetic storms due to strong winds from coronal holls

Improve presentation of the 24-th solar cycle: What is going on on sun?