Our lazy Sun Barbara Sylwester Solar Physics Division

Slides:



Advertisements
Similar presentations
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,
Advertisements

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.
OUR SUN Unusually active the past 2 weeks Very beautiful.
The Sun – Describe characteristics of the Sun (S6C3PO2 high school)
Chapter 8 The Sun – Our Star.
The Sun – Our Star Chapter 7:. General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years)
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.
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.
High-latitude activity and its relationship to the mid-latitude solar activity. Elena E. Benevolenskaya & J. Todd Hoeksema Stanford University Abstract.
Helioseismic Magnetic Imager and Why We Study Helioseismology Junwei Zhao W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford,
Show 1 -- photosphere & sunspots SUN COURSE - SLIDE SHOW 3 Show 2 -- corona & solar cycle Today: SOHO.
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
Chapter 7 The Sun. Solar Prominence – photo by SOHO spacecraft from the Astronomy Picture of the Day site link.
Solar Activities and Halloween Storms Ahmed Hady Astronomy Department Cairo University, Egypt.
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.
Synoptic Solar Cycle observed by Solar Dynamics Observatory Elena Benevolenskaya Pulkovo Astronomical Observatory Saint Petersburg State University ‘Differential.
Solar Rotation Lab 3. Differential Rotation The sun lacks a fixed rotation rate Since it is composed of a gaseous plasma, the rate of rotation is fastest.
The Sun. Sun Considered a medium STAR 93,000,000 miles away from Earth 1.39 million kilometers in diameter (one million Earths can fit inside the sun.
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.
The Sun Earth Science - Mr. Gallagher. The Sun is the Earth's nearest star. Similar to most typical stars, it is a large ball of hot electrically charged.
The Sun Chapter 29 Section 29.2 and Spaceweather.
SUN COURSE - SLIDE SHOW 8 Today: Solar flares & coronal mass ejections (CME’s)
The Sun. Solar Prominence 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.
Chapter 20, Section 2 The Sun Anne Marie Scrudato’s notes borrowed by Rusty Sturken.
Chapter 9 The Sun. 9.4 The Active Sun Sunspots: appear dark because slightly cooler than surroundings:
CHAPTER 22 THE SUN and ITS SOLAR SYSTEM
The Sun and Cycle 24 David Treharne, N8HKU Ford Amateur Radio League January 12th, 2012.
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.
CLIMATE CHANGE THE GREAT DEBATE Session 7. SOLAR POWER The Sun is the primary driving force of climate and sits in the centre of the solar system that.
The Sun 1 of 200 billion stars in the Milky Way. Our primary source of energy.
Propagation Trends Dayton 2014 Solar Maximum! But the slow decline to solar minimum in 2020 is likely to begin later this year.
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
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.
The Past and Future of Climate June 2007 David Archibald Lavoisier Conference, Melbourne.
Solar Astronomy Space Science Lab 2008 Pisgah Astronomical Research Institute.
Unit 8 Chapter 29 The Sun. We used to think that our sun was a ball of fire in the sky. Looking at our sun unaided will cause blindness. The Sun’s Energy.
Units to cover: 52, 53, Observatories in Space.
The Sun Our Very Own Star Assembled By Ken Mitchell Livermore TOPScience dtd; 3/15/09 Copy this URL into your browser
Ahmed A. HADY Astronomy Department Cairo University Egypt Deep Solar Minimum of Cycle23 and its Impact and its Impact.
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.
The Sun Part 2.
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,
CSI /PHYS Solar Atmosphere Fall 2004 Lecture 04 Sep. 22, 2004 Solar Magnetic Field, Solar Cycle, and Solar Dynamo.
Bringing 93,000,000 Miles to 40,000 Feet: Space Weather & Aviation An introduction to Space Weather What is it? Where does it come from? What does it do?
Studying the Sun HOMEWORK: REVIEW (1-7,9-12,14-17) Page 414: REVIEW (1-7,9-12,14-17) using complete sentences 15 Questions using complete sentences.
Chapter 28 The Sun Section 2 Solar Activity Notes 28-2.
The sun and the moon. Questions 1. What is a moon? What planets don’t have moons? 2. How did the moon form? 3. What causes moon phases? What’s waxing.
The Sun. What do you know about the Sun? Sun Facts The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy. It is closer to Earth.
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 – Our Favorite (and Ordinary) Star
CH29: The Sun Mrs. Kummer, 2016.
Most of the sunlight we see from earth comes from continuous photosphere emissions. These emissions make up the “quiet sun”.
The Sun All images and information courtesy of SOHO consortium. SOHO is a project of international cooperation between ESA and NASA."
Introduction to Space Weather
Introduction to Space Weather
The Sun.
Sunspots Sunspots are black spots on the surface of the Sun. They were first seen thousands of years ago by Chinese and Indian astronomers. Greek observers.
Solar Activity Chapter 8 Section 3.
The Sun & It’s Solar System
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 Sun and Eclipses Notes.
The Centre of the Solar System Earth Science 11
The Sun.
SOLAR PROMINENCE.
Closing the Books on Cycle 24 J
Presentation transcript:

Our lazy Sun Barbara Sylwester Solar Physics Division Space Research Center, Wrocław

SOHO activity cycle; 171 Å, ~1.3 MK plasma

SOHO UV  1997 & 1999 changing activity

Recurrent behavior of sunspots: 140 years Butterfly diagram Sunspots are typically confined to an equatorial belt (-35 degrees south and +35 degrees north latitude). At the beginning of a new cycle, sunspots tend to form at high latitudes, but as the cycle reaches a maximum the spots form at lower latitudes. This gives rise to the ``butterfly'' pattern first discovered by Edward Maunder in 1904.

Solar activity - proxies Red: sunspot number, reconstructed from historical observations Blue: the beryllium-10 concentration (104 atoms/(gram of ice)) as measured in annually layered ice core (Greenland) Rudolf Wolf, inventor of the modern sunspot number (1848, Zurich observatory).

400 years of sunspot observations 1749Carrington cycles Sporadic observations Regular sunspot number observations (from 1749) 1610  Among a huge number of revolutionary discoveries of Galileo Galilei was the first observations of sunspots using telescope. ( "And yet it does move"). 1640-1710  the coldest period of Little Ice Age (LIA)  the taverns for frozen ramblers have been built at the middle of Baltic Sea ; coincidence with Maunder Minimum

Sunspot number prediction (March 2006)

6 latest cycles & solar cycles prediction During the annual Space Weather Workshop held in April 2007 the Solar Cycle 24 Prediction Panel released the prediction for the next solar cycle. They expected that the new cycle will begin in late 2007 or early 2008 – about a year later than earlier predictions. Expected peak sunspot number  140 in October, 2011. Next Cycle (25) peaking in 2022 could be one of the weakest in centuries. Predictive Flux-transport Dynamo Model Mausumi Dikpati team

11 Dec. 2007 Solar Cycle 24 say: Hello ! SOHO UV-wavelength image of the Sun and a map showing positive (white) and negative (black) magnetic polarities. This region fits both criteria of new cycle: high latitude and magnetically reversed, marking it as a harbinger of a new solar cycle. Good candidate… But……the first swallow does not make a spring ….

and.…..Solar Cycle 24 official start was later 4 Jan. 2008 The large sunspot region just south of the equator is part of the waning Solar Cycle 23.

Few days later…. SOHO EIT instrument This image was taken in extreme ultraviolet: 195 Å; ~ 1.6 MK. It shows the area of the solar surface where the sunspot occured whose appearing marked the start of the new solar cycle (‘Cycle 24’) on 4 January 2008. SOHO also obsered two associated „EIT waves”, blast waves that spread out from the active regions.

First southern hemisphere spots: 4.05.2008 Solar minimum is upon us ! New solar cycle had begun definitely! EIT/SOHO; 284 Å; ~ 2MK

2008, September - Spotless Sun Left: A photo of the Sun taken Sept. 27, 2008. The face of the sun is "blank”. Right: The Sun on Sept. 27, 2001. The Sun's face is peppered with sunspots. The difference is the phase of the 11-year solar cycle. updated: Sept. 27, 2008 To find a year with more blank Sun, we have to go back to 1954 (three years before the launch of Sputnik).  2008 the „blankest year” of the Space Age

29 September 2008; 304 Å NASA's STEREO (Ahead) spacecraft observed this prominence eruption. It rose up and cascaded to the right over several hours, appearing something like a flag headed into space. The material observed is actually ionized Helium at about 60,000 K. Prominences are relatively cool clouds of gas controlled by magnetic forces.

New cycle flare activity; Oct. 2008 6 Oct. 2008 A6.4

Signs of life  …. Solar minimum behind us? A new sunspot appeared on 11 Oct. 2008, the third spot seen in many weeks. New-cycle sunspot group 1007 emerges on Halloween and marches across the face of the sun over a four-day period in early November 2008.

2 Nov. 2008; B7.2 flare

….boring Sun on 13th Jan. 2009 captured by amateur astronomer A whole year after Solar Cycle 24 was supposed to start (when the first reversed polarity sunspot pair appeared on the Sun’s surface) the Sun is blank (featureless). However we have had flares from „left over” Cycle 23 and a bit of action from Cycle 24 (A, B class flares). 2008 was a year of overlap with both cycles weakly active at the same time.

KORONAS Photon-TESIS: 20.02.2009 18:27 UT 18:28 UT Inner corona: Fe IX 171 Å; ~1 MK He II 304; ~80 000 K 18:34 UT; Outer corona: Fe IX 171 Å; ~1 MK

27 Feb. 2009; A3.2 flare

28 Feb. 2009 (8 hours period); TESIS

20 March 2009: Where have all activity gone? SOHO MDI continuum 304 Å ; T ~ 80 000 K 284 Å ; T ~ 2 MK http://sohowww.nascom.nasa.gov/data/realtime-images.html

Progression of the solar cycle http://solarcycle24.com/ http://www.nwra-az.com/spawx/ssne-year.html Data gathered by GOES satellites which monitor solar X-rays (tracking solar flares). Solar flares can also trigger geomagnetic storms which produce aurora. The daily effective sunspot numbers over the past year. Two parameters are plotted: solid line - based on analysis of ionospheric data, and dotted line based on the observed 10.7 cm solar radio flux.

HINODE XRT Present Sun; 305 Å; ~80 000 K

Why the Sun has gone quiet? Solar dynamo…… the magnetic field lines are wrapped dipole field after many rotations lines are highly twisted and bundled the rotation rate is 20 ℅ faster at the equator the resulting buoyancy lifts the bundle to the surface  something abruptly “switched off” in the inner workings of the solar dynamo ????? the Sun has slowed it’s internal dynamo to a similar level such as was seen during the Dalton Minimum ???? The truth is, solar activity never stops, "not even during solar minimum."

Conculding ….. the „new millenium solar minimum”? The Sun is now in the quietest phase of its 11 - year activity cycle. In fact, it has been unusually quiet during 2008 year. Scientists are unsure of the significance of this unusual calm. The only way to know is to wait and see. Our closest star is continually monitoring with an array of telescopes and satellites. Probably this time next year we will be inundated with sunspots…fingers crossed.