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Show 1 -- photosphere & sunspots --> SUN COURSE - SLIDE SHOW 2 1. Introduction, 2. Magnetic
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SUN COURSE - SLIDE SHOW 2

Feb 11, 2016

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SUN COURSE - SLIDE SHOW 2. Show 1 -- photosphere & sunspots. -->. 1. Introduction, 2. Magnetic fields, 3. Corona. 1. INTRODUCTION: PS Age of Sun ?. If Sun consists of coal, it could generate heat/light for …. a few thousand yrs. - PowerPoint PPT Presentation
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Page 1: SUN  COURSE - SLIDE SHOW 2

Show 1 -- photosphere & sunspots -->

SUN COURSE - SLIDE SHOW 2

1. Introduction, 2. Magnetic fields, 3. Corona

Page 2: SUN  COURSE - SLIDE SHOW 2

1. INTRODUCTION: PS Age of Sun ? If Sun consists of coal, it could generate heat/light for …

a few thousand yrs Kelvin (1862) - if Sun slowly contracts (grav. Energy -> heat), it could have illuminated Earth for … 100 m yrs !

Radioactivity discovered -> Earth rocks older than this !!

Paradox resolved - new source heat discovered - nuclear fusionRadioactive dating method (eg uranium --> lead):

- measure ratio masses + rate of decay--> time since rocks have formed

Oldest rocks in s. system (Moon/meteorites) formed 4.6b yrs ago -- when Sun thought to have been born

Page 3: SUN  COURSE - SLIDE SHOW 2

PS Diffusion

QuickTime™ and aYUV420 codec decompressorare needed to see this picture.

Start with field B0(x) and watch diffuse.

Current density

Page 4: SUN  COURSE - SLIDE SHOW 2

Ionosphere --> Sun (8 light mins)

Learn basic behaviour of plasma from Sun

stars (4 light years) [At 186,000 miles per sec, 1 light year = 6 trillion

miles]

MOST of UNIVERSE is PLASMA:

Page 5: SUN  COURSE - SLIDE SHOW 2

? THOUGHT of Vector Calculus FILL with CONFIDENCE

Page 6: SUN  COURSE - SLIDE SHOW 2

Eqns of Magnetohydrodynamics PDE's for v and B as

functions of x,y,z,t

As beautiful as the Sun !! -- Nonlinear

Impossible to solve completely

So approximate in imaginative ways --

ODE's or PDE's and solve (standard techs)

--> Construct models for many dynamic phenomena on Sun

Page 7: SUN  COURSE - SLIDE SHOW 2

Temperature Structure

Page 8: SUN  COURSE - SLIDE SHOW 2

ATMOSPHERE Photosphere --> Sunspots

Galileo discovered (1610) w. telescope

-- Greeks, Chinese

? Planets, clouds, smoke, slag

Dark because cool

Surprise (1908):

site of strong magnetic field

Page 9: SUN  COURSE - SLIDE SHOW 2

White -- towards you; Black -- away from you

Regions around sunspots -- "Active Regions"

SURPRISES: -- patterns of sunspots

-- intense magnetic fields over whole Sun

2. MAGNETIC MAP ("Magnetogram")

Page 10: SUN  COURSE - SLIDE SHOW 2

Movie

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.But why the active region

patterns ?

Page 11: SUN  COURSE - SLIDE SHOW 2

In interior, plasma dominates --> moves B

Rotation shears B

Magnetic Field (B) and Plasma CoupledB exerts force on plasma -- move together

--> 2 tubes B --> Emerge:

Page 12: SUN  COURSE - SLIDE SHOW 2

Magnetic Tube Emerges

Creates pair of sunspots +/-

Opposite pattern in s. hemisphere

Page 13: SUN  COURSE - SLIDE SHOW 2

Global Magnetic Field of Sun

Spreads out --> remnant active region

Merges --> unipolar region -- one dominant polarity

Migrates to the poles --> polar field

At photosphere <|B|> ~ 3 - 20 G, but most is strong (1 kG) & vertical

(i) ACTIVE REGION FLUX

Emerges as

•sunspots (B = 3 kG, flux = 1022

Mx)

* active regions --> faculae (bright)

Page 14: SUN  COURSE - SLIDE SHOW 2

Solar Cycle Sunspots vary with period 8-15 years (average 11.1 yr) Two zones between -35o and +35o latitude

In opposite hemispheres, leading spots have opposite polarities (Hale) Leading polarity is closer to equator (Joy)

Page 15: SUN  COURSE - SLIDE SHOW 2

New spots emerge at start of cycle at high latitudes w. opposite polarity

As cycle progresses, spots form at lower latitudes (Sporer)

Polar Fields: * maximum extent at s. minimum * change polarity 1-2 years after s. maximum

Page 16: SUN  COURSE - SLIDE SHOW 2

No sunspots varies - 11-year

cycle

Also cycle in X-rays

And in shape of corona:

Page 17: SUN  COURSE - SLIDE SHOW 2

(ii) Quiet Sun - Network mixed polarity -- at edge of supergranule cells -- covers Sun at s. minimum

ephemeral active regions (1019 Mx) -- emerge & migrate to boundary

--> network fragments (F = 2x1018 Mx, B = 1 kG) -- at edges of cells

internetwork fragments (F = 6x1016 Mx, B = 10-100 G ?) -- inside cells

Page 18: SUN  COURSE - SLIDE SHOW 2

Chromosphere

Page 19: SUN  COURSE - SLIDE SHOW 2

("crown") -- See at ECLIPSE of Sun

Faint open structures -- Bright closed structuresSURPRISE (1868) -- Light from new element "Helium"SURPRISE (1940) -- Temperature is million degrees !!!!

3. CORONA

Page 20: SUN  COURSE - SLIDE SHOW 2

QuickTime™ and aYUV420 codec decompressorare needed to see this picture.

ECLIPSE

Page 21: SUN  COURSE - SLIDE SHOW 2

T = Million --> Corona is NOT a normal gas !!!3 states of matter ...

B here -- unaware -- no effectB in plasma -- coupled (intimate, subtle)CORONA is in 4th state ("PLASMA")

PLASMA behaves differently from normal gas:Corona created by B (heat, structure) --

open/closed (iron filings round bar magnet)

Another ECLIPSE

Page 22: SUN  COURSE - SLIDE SHOW 2
Page 23: SUN  COURSE - SLIDE SHOW 2
Page 24: SUN  COURSE - SLIDE SHOW 2

How Bright is Corona/Full Moon ?

Base corona (C0) = 10-5 x Photosphere

Corona at 1 Ro = 10-8 x Photosphere

Full Moon = 2 x 10-6 x Photosphere = 0.2 Co

Sunspot: Umbra = 0.2 Photosphere

Penumbra = 0.75 Photosphere

Lang: Moon = 0.1 x Sunspot ??

So Moon = 10-5 Sunspot

Page 25: SUN  COURSE - SLIDE SHOW 2

Normally need eclipse to see -- Glare of surface

Observe direct with X-ray telescope

As T increases (furnace), object becomes bluer

CORONA:

Page 26: SUN  COURSE - SLIDE SHOW 2

Skylab (1973-1974)

Page 27: SUN  COURSE - SLIDE SHOW 2

Coronal holes -- loops -- bright points Bright --> Denser

Picture with X-ray telescope:

Page 28: SUN  COURSE - SLIDE SHOW 2

A magnetic

world

Yohkoh

Page 29: SUN  COURSE - SLIDE SHOW 2

Eclipse seen by Yohkoh

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

Page 30: SUN  COURSE - SLIDE SHOW 2

Movie

QuickTime™ and aVideo decompressor

are needed to see this picture.

Page 31: SUN  COURSE - SLIDE SHOW 2

QuickTime™ and aYUV420 codec decompressorare needed to see this picture.

From Photosphere to Corona

Page 32: SUN  COURSE - SLIDE SHOW 2

Movie + photosphere

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

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Original Skylab Images

Latest images from new satellite:

Page 34: SUN  COURSE - SLIDE SHOW 2

TRACE (Active region)

Page 35: SUN  COURSE - SLIDE SHOW 2

Active region at limb

Page 36: SUN  COURSE - SLIDE SHOW 2

of Magnetic Loops in Corona (TRACE)

B strong

Dominates plasma

Close-up

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along Magnetic Loops

Conjuring trick --

plasma appearing by magic ?

QuickTime™ and aVideo decompressorare needed to see this picture.

Plasma Motions

Page 39: SUN  COURSE - SLIDE SHOW 2

TRACE - zoom

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

Page 40: SUN  COURSE - SLIDE SHOW 2

TRACE - flux emerge

QuickTime™ and aVideo decompressor

are needed to see this picture.

Page 41: SUN  COURSE - SLIDE SHOW 2

To Finish