Fifty Years Of Solar Events NOAO 50 th Anniversary Symposium.

Slides:



Advertisements
Similar presentations
CHAPTER 10: The Sun – Our Favorite (and Ordinary) Star
Advertisements

Chapter 10 Our Star A Closer Look at the Sun Our Goals for Learning Why does the Sun shine? What is the Sun’s structure?
The Sun’s Magnetic Personality Assembled by Ken Mitchell Livermore TOPScience.
Dr Matt Burleigh The Sun and the Stars. Dr Matt Burleigh The Sun and the Stars Limb darkening The surface of the sun does not have uniform brightness,
Stars and Galaxies The Sun.
Sunspots and the Scientific Method: Models. Hypothesis Driven Science Hypothesis: An educated speculation about how a particular phenomenon behaves- very.
The Sun – Describe characteristics of the Sun (S6C3PO2 high school)
An overview of the cycle variations in the solar corona Louise Harra UCL Department of Space and Climate Physics Mullard Space Science.
Our Star, the Sun Chapter Eighteen.
Chapter 8 The Sun – Our Star.
Planetary tides and solar activity Katya Georgieva
General Properties Absolute visual magnitude M V = 4.83 Central temperature = 15 million 0 K X = 0.73, Y = 0.25, Z = 0.02 Initial abundances: Age: ~ 4.52.
The Solar Cycle for seeing the sun exhibit. The Sun’s Magnetic Field The magnetic field on the sun is produced by the flow of electrically charged ions.
Scientific astrology: planetary effects on solar activity Katya Georgieva Solar-Terrestrial Influences Lab., Bulgarian Academy of Sciences In collaboration.
Solar Flares and Lunar Tides. The Sun’s Differential Rotation Since the Sun is a gaseous body rather than solid, different latitudes can rotate at different.
Guiding Questions 1.What is the source of the Sun’s energy? 2.What is the internal structure of the Sun? 3.How can we measure the properties of the Sun’s.
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
Physics 681: Solar Physics and Instrumentation – Lecture 20 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
High-latitude activity and its relationship to the mid-latitude solar activity. Elena E. Benevolenskaya & J. Todd Hoeksema Stanford University Abstract.
HMI/AIA Science Team Meeting, HMI Science Goals Alexander Kosovichev & HMI Team.
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
Influence of depth-dependent diffusivity profiles in governing the evolution of weak, large-scale magnetic fields of the sun Night Song and E.J. Zita,
Prediction on Time-Scales of Years to Decades Discussion Group A.
THE SUN 1 million km wide ball of H, He undergoing nuclear fusion. Contains 99% of the mass in the whole solar system! Would hold 1.3 million earths!
Thomas Zurbuchen University of Michigan The Structure and Sources of the Solar Wind during the Solar Cycle.
Introduction to Space Weather Jie Zhang CSI 662 / PHYS 660 Spring, 2012 Copyright © The Sun: Magnetism Feb. 09, 2012.
The Asymmetric Polar Field Reversal – Long-Term Observations from WSO J. Todd Hoeksema, Solar Observatories H.E.P.L., Stanford University SH13C-2278.
EARTH & SPACE SCIENCE Chapter 29 The Sun 29.2 Solar Activity.
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2 Doppler/ Sunspots/ Interior.
Space Weather Major sources of space weather ● Solar wind – a stream of plasma consisting of high energy charged particles released from the upper atmosphere.
Activity Cycles in Stars Dr. David H. Hathaway NASA Marshall Space Flight Center National Space Science and Technology Center.
Chapter 9 The Sun. 9.4 The Active Sun Sunspots: appear dark because slightly cooler than surroundings:
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.
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
ESS 7 Lectures 3, 4,and 5 October 1, 3, and 6, 2008 The Sun.
Inner Workings of the Sun (87). Sun is mostly hydrogen and helium gas (plasma). Core (15,000,000 ° C): –Fuels the sun, where the fusing of Hydrogen 
Modern Solar Mysteries Dr. David H. Hathaway NASA/MSFC National Space Science and Technology Center Dr. David H. Hathaway NASA/MSFC National Space Science.
OUR SUN THE CLOSEST STAR. Composition of the Sun The Sun is composed of at least 80 of the elements found on Earth. Sun is mostly composed of 91.2% Hydrogen,
The Sun- Solar Activity. Damage to communications & power systems.
The Sun.
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 Rise of Solar Cycle 24: Magnetic Fields from the Dynamo through the Photosphere and Corona and Connecting to the Heliosphere Part 1: Interior and Photosphere.
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
Recent Progress in Understanding The Sun’s Magnetic Dynamo David H. Hathaway NASA/MSFC National Space Science and Technology Center 2004 April 28 University.
1. active prominences - solar prominences that change in a matter of hours.
Dr Dash will be on travel for the next two weeks (off to Africa). We will have a guest lecturer and Justin will be available to answer questions. Homework.
Chapter 10 Our Star A Closer Look at the Sun Our goals for learning: Why does the Sun shine? What is the Sun’s structure?
The Magnetic Sun. What is the Sun? The Sun is a Star, but seen close-up. The Stars are other Suns but very far away.
Andrés Muñoz-Jaramillo Harvard-Smithsonian Center for Astrophysics
Lesson 2.  At the center of our solar system is the Sun which is a typical medium sized star.  Composed mainly of Hydrogen (73% by mass), 23% helium.
Our Sun.
The Sun. The Sun’s Size and Composition The Sun is roughly 100 times larger than Earth in diameter, and 300,000 times larger in mass. It is a gaseous.
What factors make the Sun a star, not a planet?
Reading Unit 31, 32, 51. The Sun The Sun is a huge ball of gas at the center of the solar system –1 million Earths would fit inside it! –Releases the.
Geomagnetism Part II: The Earth’s Magnetic Field
Most of the sunlight we see from earth comes from continuous photosphere emissions. These emissions make up the “quiet sun”.
What the Long-Term Sunspot Record Tells Us About Space Climate David H. Hathaway NASA/MSFC National Space Science and Technology Center Huntsville, AL,
Solar Magnetism: Solar Cycle Solar Dynamo Coronal Magnetic Field CSI 662 / ASTR 769 Lect. 03, February 6 Spring 2007 References: NASA/MSFC Solar Physics.
CSI /PHYS Solar Atmosphere Fall 2004 Lecture 04 Sep. 22, 2004 Solar Magnetic Field, Solar Cycle, and Solar Dynamo.
Axel Brandenburg & Jörn Warnecke NorditaStockholm  loop emergence –Buoyant rise –Many scale heights –Twist needed Dynamo –bi-helical field Emergence.
The Sun. Sun Fact Sheet The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy. Diameter: 1,390,000 km (Earth 12,742 km or nearly.
The Sun Essential Question: What are the properties of the Sun?
Sun Notes.
Introduction to Space Weather
The Sun: close-up of a spectral class G main sequence star
Section 2: Solar Activity
Solar Activity Chapter 8 Section 3.
WHAT DO YOU THINK? How does the mass of the Sun compare with that of the rest of the Solar System? Are there stars nearer the Earth than the Sun is? What.
The Centre of the Solar System Earth Science 11
The Sun – Our Favorite Star
Presentation transcript:

Fifty Years Of Solar Events NOAO 50 th Anniversary Symposium

The Sun is never still Conditions change on time scales from to seconds, spanning 23 orders of magnitude On the long end, secular evolution of the internal solar structure On the short end, explosive magnetic reconnection in flares In between, many different phenomena

Source of solar variability For time scales shorter than 10 4 years, main cause of variability is the magnetic field on the surface This field is generated inside the Sun by plasma motions The most familiar phenomenon is the solar activity cycle Number of sunspots increases & decreases with a period of 9 to 13 years Dominant solar polarity flips with every sunspot cycle, so the polarity cycle is 18 to 26 years

The active Sun High number of sunspots Many flares emitting energetic particles, X-rays,  - rays, etc. Increased frequency of coronal mass ejections (CMEs) Slightly higher irradiance (0.1%) Rather higher irradiance in UV (20%), X-rays Reduced galactic cosmic ray flux Increased unsigned global magnetic field strength

What happened in the last fifty years?

Highlights of cycles Coincident with the birth of the space age, IGY Activity in cycle 19 was highest since Maunder Minimum Largest solar flare in modern era on November 4, 2003 (X17) Power grid failure March 13, 1989 in Quebec from solar activity Deep solar minimum just now ending

The surface magnetic field through the cycle

The solar x-ray flux through the cycle

Halloween 2003 on the Sun

The Sun spits up a lot

Effect of the Sun on the Earth (Not to scale)

The geomagnetic storm of March 13, 1989 Quebec went dark at 7:45 UT

The current minimum is unusual Longer than average Most spotless days (so far) since cycle 15 Lowest global solar wind pressure of the space age Solar magnetic field 36% weaker than last minimum Lowest irradiance yet measured Lowest sustained 10.7-cm radio flux since 1947 Unusually high tilt of dipole field No classical quiescent equatorial streamer belt Very high cosmic ray flux Odd behavior of p-mode frequencies But it seems to be over…. What happened?

What causes the solar cycle? Flux-Transport Dynamo theory: – Differential rotation winds up the internal poloidal (N- S) magnetic field into a toroidal (E-W) field – As the field is wound up, its strength increases, and it becomes buoyant – The field breaks through the surface, reconnects in the corona, and returns to a poloidal configuration – Meridional plasma flows move the field from equator to pole at the surface and pole to equator deeper down

Fig. 2. Schematic of solar flux-transport dynamo processes. Red inner sphere represents the Sun’s radiative core and blue mesh the solar surface. In between is the solar convection zone where dynamo resides. (a) Shearing of poloidal field by the Sun’s differential rotation near convection zone bottom. The Sun rotates faster at the equator than the pole. (b) Toroidal field produced due to this shearing by differential rotation. (c) When toroidal field is strong enough, buoyant loops rise to the surface, twisting as they rise due to rotational influence. Sunspots (two black dots) are formed from these loops. (d, e, f) Additional flux emerges (d, e) and spreads (f) in latitude and longitude from decaying spots. (g) Meridional flow (yellow circulation with arrows) carries surface magnetic flux poleward, causing polar fields to reverse. (h) Some of this flux is then transported downward to the bottom and towards the equator. These poloidal fields have sign opposite to those at the beginning of the sequence, in frame (a). (i) This reversed poloidal flux is then sheared again near the bottom by the differential rotation to produce the new toroidal field opposite in sign to that shown in (b).

Internal flows cause the cycle Differential rotation winds the field up Helioseismology revealed the internal pattern of rotation and discovered the tachocline Meridional (N-S) flow moves the field in latitude – a key ingredient for FTD Speed of deep meridional flow sets period and strength of cycle Helioseismology trying to measure the deep meridional flow, but it is difficult But there is also something missing from the FTD picture – the zonal (E-W) flows

Solar cycle timing from the “torsional oscillation” Slow migration of flow towards equator coincided with extended minimum. Predicted that when flow reached  22°, then solar activity would increase. It did. (R. Howe)

Another intriguing thing… The rotation rate at the solar tachocline varied (maybe periodically) in the first part of cycle 23, but stopped. Is this related to the deep minimum preceding cycle 24?

The Sun and the Earth Solar activity affects the Earth and terrestrial society – GPS – Telecommunications – Space hardware & astronauts – Power grids – Polar airline flights Thus considerable interest in predicting “Space Weather”

Flows below active regions AR AR 10069

Flare forecasts from subsurface vorticity Active regions with both strong subsurface vorticity (twisting motions) and high surface magnetic field are almost certain to produce many energetic flares The vorticity changes rapidly before a flare occurs, starting as many as three days in advance of the flare. The predictive capability is twice that of current methods, and likely can be improved A Reinard, J. Henthorn, R. Komm

Physical scenario Convective rolls or “smoke rings” twist the flux tube Need detailed models of the process

NOAO’s contribution Solar events are also terrestrial events As society becomes more dependent on technology, the understanding of solar activity becomes more important NOAO, through NSO, has played a vital role in this understanding ATST, SOLIS and GONG will continue to be in the forefront of the science