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Helio-seismology in Helio-seismology in 20min 20min Introduction Introduction Solar Structure Solar Structure Physics Involved Physics Involved Observing Networks Observing Networks Current Results Current Results Summary Summary David Brands David Brands Stafford and District Stafford and District Astro. Soc Astro. Soc.

Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

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Page 1: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Helio-seismology in 20minHelio-seismology in 20minIntroductionIntroduction

Solar StructureSolar StructurePhysics InvolvedPhysics Involved

Observing NetworksObserving NetworksCurrent ResultsCurrent Results

SummarySummary

David BrandsDavid Brands

Stafford and District Astro. SocStafford and District Astro. Soc.

Page 2: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

What is Helio-Seismology?What is Helio-Seismology?

• ““Helios” of the sun (all Greek)Helios” of the sun (all Greek)

• ““Seismos” earthquakeSeismos” earthquake

• ““Logos” knowledgeLogos” knowledge

• Mis-labled because there is almost no Mis-labled because there is almost no shear activity (s wave), only p waves (like shear activity (s wave), only p waves (like sound)sound)

• ““Study of solar p waves to determine Study of solar p waves to determine structure and activity of the sun.”structure and activity of the sun.”

Page 3: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Earthquake PropogationEarthquake Propogation

• P wavesP waves– PressurePressure– FastFast

• S wavesS waves– ShearShear– SlowSlow

Page 4: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

• Particle displacement parallel to wave Particle displacement parallel to wave direction direction

• The particles do not move with the wave; The particles do not move with the wave; simply oscillate back and forthsimply oscillate back and forth

• Wave is seen as the motion of the Wave is seen as the motion of the compressed region (ie, a pressure wave)compressed region (ie, a pressure wave)

Pressure “P” Pressure “P” Longitudinal Longitudinal wavewave

Page 5: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

• Particle displacement perpendicular to Particle displacement perpendicular to wave direction wave direction

• Particles do not move with the wave; they Particles do not move with the wave; they simply oscillate up and downsimply oscillate up and down

• Wave is seen as the motion of the crests Wave is seen as the motion of the crests and troughsand troughs

Shear “S” Shear “S” Transverse Transverse wavewave

Page 6: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Water Water Waves Waves

• Example of waves that involve a Example of waves that involve a combination of both longitudinal and combination of both longitudinal and transverse motions. transverse motions.

• Particles travel in Particles travel in clockwise circlesclockwise circles. The . The radius of the circles decreases as the radius of the circles decreases as the depth into the water increases. depth into the water increases.

• See two particles in See two particles in blueblue to show that to show that each particle travels in a clockwise circle each particle travels in a clockwise circle as the wave passes. as the wave passes.

Page 7: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Rayleigh Rayleigh surface waves surface waves • In a solidIn a solid• Elliptical pathsElliptical paths

• Rayleigh waves different from water waves in Rayleigh waves different from water waves in one important way.one important way.

• Water wave all particles travel in clockwise Water wave all particles travel in clockwise circles, but in Raleigh solids:circles, but in Raleigh solids:

• Surface particles Surface particles counter-clockwisecounter-clockwise ellipse ellipse• Particles at depth Particles at depth clockwiseclockwise ellispes. ellispes.

Page 8: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

HelioseismologyHelioseismology

• Sun – almost no “s” waves, mainly “p”Sun – almost no “s” waves, mainly “p”

• Disturbances generated in convection Disturbances generated in convection zone, near photosphere surfacezone, near photosphere surface

• Propagate to surfacePropagate to surface

• Study of surface effects reveals interiorStudy of surface effects reveals interior

• Resonances make the sun “ring” like a bellResonances make the sun “ring” like a bell

Page 9: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Internal Structure of SunInternal Structure of Sun

ProvenProven

ByBy

HelioHelio

SeizmologySeizmology

2.2M Deg C

170K km 500K km1.6%

170000 Yr

10 Days50Km5mins/0.003 Hz

15.6M Deg C700K km

5000 Deg C

9000 Deg C

2.2M Deg C

0.5 MY

Page 10: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Solar Flare causing QuakeSolar Flare causing Quake

Page 11: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Mathematical models of oscillationsMathematical models of oscillations

•Mirage – light bent by hot airMirage – light bent by hot air

Actually hotter air easier / faster pathActually hotter air easier / faster path

•Sound bent in resonance cavities,Sound bent in resonance cavities,

Temp gradients, adiabatic regionsTemp gradients, adiabatic regions

N no. nodes radially outward

M no. nodes around the equator

L no. nodes around the azimuth

L 20

M 17IN

OUT

Page 12: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Vibration Nodes ExampleVibration Nodes Example

1st Harm1st Harm

2nd harm2nd harm

3rd Harm3rd Harm

4th Harm4th Harm

Page 13: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Mathematical models of oscillationsMathematical models of oscillations

•Mirage – light bent by hot airMirage – light bent by hot air

Actually hotter air easier / faster pathActually hotter air easier / faster path

•Sound bent in resonance cavities,Sound bent in resonance cavities,

Temp gradients, adiabatic regionsTemp gradients, adiabatic regions

N no. nodes radially outward

M no. nodes around the equator

L no. nodes around the azimuth

L 20

M 17IN

OUT

Page 14: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Sounds of the sunSounds of the sun

• Wideband filterWideband filter

• All sounds speeded up 42,000 times to All sounds speeded up 42,000 times to become audiblebecome audible

• 0.003 Hz 0.003 Hz

• Human detection starts at 25HzHuman detection starts at 25Hz

Page 15: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Bison NetworkBison Network((Birmingham Solar Oscillations Network)Birmingham Solar Oscillations Network)

Six-station networkSix-station network– Resonant Scattering SpectrometersResonant Scattering Spectrometers

Page 16: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Gong NetworkGong Network

• Global Oscillation Network Group Global Oscillation Network Group

• Similar to BisonSimilar to Bison

• GONG is:GONG is:– a six-station networka six-station network– extremely sensitive velocity imagersextremely sensitive velocity imagers– located around the Earth located around the Earth – obtain nearly continuous observations of the obtain nearly continuous observations of the

Sun's oscillations. Sun's oscillations.

Page 17: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Gong Instruments (1994)Gong Instruments (1994)

• InterferometerInterferometer

• 6 unit trial6 unit trial

• Before shippingBefore shipping

Page 18: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Data: Schematic MovieData: Schematic Movie

Page 19: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Gong Far Side MappingGong Far Side Mapping

• P wave mappingP wave mapping

• Uses interior modelUses interior model

Page 20: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Network ResultsNetwork Results

• Global results:Global results:– Confirmed / improved model of sun interiorConfirmed / improved model of sun interior– Eliminated model errors in “missing nuetrino”Eliminated model errors in “missing nuetrino”– Maps activity and sunspots on “far” sideMaps activity and sunspots on “far” side– Found “jet stream” in convection layersFound “jet stream” in convection layers– Calculated sun age – agrees with meteoritesCalculated sun age – agrees with meteorites

Page 21: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Helio-SeismologyHelio-Seismology

• Conclusions:Conclusions:– P wave analysis, some S wave, good modelsP wave analysis, some S wave, good models– global detector networksglobal detector networks– Internal structure revealed / refinedInternal structure revealed / refined– ““see” spots and activity on far sidesee” spots and activity on far side– Now looking at nearby stars for similar insightNow looking at nearby stars for similar insight

Page 22: Helio-seismology in 20min Introduction Solar Structure Physics Involved Observing Networks Observing Networks Current Results Summary David Brands Stafford

Helio-seismologyHelio-seismologyin 20 Minutesin 20 Minutes

Questions?Questions?

David BrandsDavid Brands

Stafford and District Astro. SocStafford and District Astro. Soc.