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I. OUR OWN SUN

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Atmosphere: Photosphere, Chromosphere, ... 3. Photosphere. Temperature ... Photosphere -- Sunspots. Harriot discovered (1610) w. telescope. Dark because ... – PowerPoint PPT presentation

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Title: I. OUR OWN SUN


1
I. OUR OWN SUN
(Space Climate School, Saariselka, March,
2009) Eric Priest (St Andrews)
2
1. Why Study the Sun ?
1. Of great scientific interest in own
right
2. Influence on Earth
3. Important for Astronomy
-- fundamental cosmic processes
4. Many misconceptions..
Many basic properties still mystery (astrony) -
interior, dynamo, corona, wind, flares
So Sun is 1 of liveliest branches of space
physics/astronomy
3
Another Theme
Many surprises caused by magnetic field (B)
Sun is NOT a normal gas
Sun is in 4th state of matter ("PLASMA")
behaves differently from normal gas
B and plasma -- coupled (intimate, subtle)
B exerts force on plasma -- stores energy
4
2. The SUN
Vital Statistics
? Chemical composition
Radius
Age --
5
Overall Structure
Interior Core Convection zone (gt 0.7 R0)
Atmosphere Photosphere, Chromosphere, Corona
6
3. Photosphere
Temperature 6000 K
Covered with turbulent convection cells
Granulation (1 Mm) Supergranulation (15
- 30 Mm)
7
In close-up points, flowers, ribbons (created
by magnetic fields)
8
SUNSPOTS
Photosphere --gt Sunspots
Harriot discovered (1610) w. telescope
Dark because cool But why cool ?
9
New Model (Thomas Weiss)
Mixture Dark filaments- (low)
Bright filaments- (high)
10
Map of Photospheric Magnetic Field
White -- towards you Black -- away from you
Regions around sunspots -- bipolar "Active
Regions"
11
SURPRISES --
1. Intense magnetic fields over whole Sun
B carried to edges of convection cells
2. Patterns of sunspots/act. regs -- large flux
tube --gt dynamo
12
Old Picture Atmosphere - static, T(r)
13
But - atmosphere is inhomogeneous
Many temperatures in same region
14
4. Chromosphere is dynamic (2D Simulation)
Hansteen Carlsson
Corona
Chromo- sphere
Photo- sphere (light/ dense)
15
Dynamic nature s. atmosphere Swedish Solar
Telescope
Quiet active region H-alpha 0.1 arcsec
Continually-changing threads
16
5. CORONA
("crown") -- See at ECLIPSE of Sun
Along open structures -- fast solar wind
SURPRISE (1940) -- Temperature is million degrees
Students in St Andrews imaginative
Heating caused by magnetic field
Structure outlines magnetic field
17
Total Eclipse - March 29, 2006 - Motion of
Moons shadow
18
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19
Over 1.5 hours
Light level decreases,
Cooler,
Shadows sharpen
20
In last 10 minutes
Light level and temperature decrease more quickly
Wind
Start to see planets
Just before totality (when Moon covers Sun) --
Baily beads Red chromosphere Prominences
Corona - glowing against jet black disc !
21
2nd Contact
Just before totality
Magnetic tubes prominences
22
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23
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24
CORONA
Normally need eclipse to see -- Glare of surface
Observe direct with EUV/X-ray telescope
As T increases (furnace), object becomes bluer
25
Picture with X-ray telescope
Coronal holes -- loops -- bright points
Bright --gt Denser
26
Hinode X-ray Telescope (2006--..)
27
6. SOHO (Solar Heliospheric Observatory)
Launched 1995. Orbiting Sun at point in phase
with Earth
Observing Sun continuously for 1st time (ESA/NASA)
--gt 1st comprehensive view of Sun
MANY NEW SURPRISES
28
QN. -- ? Earth Influenced by Solar Variability
Number of Sunspots Oscillates w. 11-year Cycle
29
Solar Cycle
Sunspots - two zones between -35o and 35o
latitude
Leading spots have opposite polarities in 2
hemispheres Hale Leading polarity is closer to
equator Joy
Magnetic field reverses every 11 years
30
Solar cycle (ii)
Sunspot minm -- no spots -- polar fields
Spots emerge at high latitudes w. opposite
polarity later at lower latitudes
90 active region flux cancels --10 migrates
-- following flux reaches poles reduces
reverses polar field-- new minm
Global coronal magnetic field goes thro complex
set of 17 topologies (Maclean Priest,
2007)
Polar Fields maximum extent at s. minimum
change polarity 1-2 years after s. maximum
31
Whole atmosphere varies with cycle
Max Min
Chromosphere
Corona (Intensity Changes by 100)
Schematic --gt eq. streamers/polar holes
32
Solar wind velocity polar plot, ULYSSES
Sunspot minimum 1994-95
Red inward field Blue outward field
33
SURPRISE (1976)
Realised NO sunspots in most of 17th centy
"Maunder Minimum" -- Little Ice Age
So B on Sun affects climate of Earth !! But
mechanism not known !
34
SOHO --gt Total Emission (t) 1996-2000
Emission varies by 0.2 -- passage
sunspots Increase by 0.1 from sunspot min to max
Much too small to produce global warming
?? Real ?? cause
35
Solar cycle variations further back to
1980 from several spacecraft irradiance
1400 from 10Be in ice cores 30, 000 yrs BP from
14C in tree rings (J Beer)
36
CONCLUSIONS
  • Solar Physics - golden age - observations
  • Magnetic theory playing a key role
  • Sense of vitality will continue
  • amazing observations from space
  • (SOHO, TRACE, RHESSI,
  • Hinode, Stereo,
  • SDO, Orbiter)

- bright new young students
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