magnetic waves in solar coronal loops ryan orvedahl stony brook university advisor: aad van...
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Magnetic Waves in Solar Coronal Loops
Ryan OrvedahlStony Brook University
Advisor:Aad van
BallegooijenCenter for
Astrophysics
What Heats the Interior?
http://en.wikipedia.org/wiki/Sun
Core ~ 15 MKProton-proton chain
Radiative Zone ~ 5 MKRadiation diffusion
Convective Zone ~ 100 kKBulk fluid motion
What Heats the Atmosphere?Photosphere =
~5700 KSurface that we see
Chromosphere = ~ 10 kKWaves?
Corona = ~ 1-10 MKWaves?
http://solar.physics.montana.edu/YPOP/Spotlight/SunInfo/Transregion.html
Coronal Loops and Alfvén Waves
http://en.wikipedia.org/wiki/Gateway_Arch
What are coronal loops?
What are Alfvén Waves?
How do they fit into the model?
Different Temperatures of a Single Active
Region
335 Å ~ 2.5 MK 211 Å ~ 2.0 MK
171 Å ~ 0.6 MK
193 Å ~ 1.2 MK
Hinode SOT/SP InstrumentSolar Optical Telescope and SpectroPolarimeter
0.5 m optical telescope0.167” res = ~120 km
res
Zeeman EffectSplit energy levels in B
fieldSplit ~ B field strengthPolarized = how much
split
http://en.wikipedia.org/wiki/File:Zeeman_effect.svg
Step 1: Look for the WavesLoop lifetime ~10-15 min
Ideally want thin loops
Create Movie Hopefully see
transverse waves
Very small amplitudes
Program to measure changes of transverse position with sub-pixel accuracy
Select a Loop Loop
Follow max intensity over time
Plot position vs time
Ideally want a sinusoidal curve
Transverse position:
Best Examples of Alfvén WavesVelocity ~1 km/s
Step 2: Modeling a Single LoopReflection and nonlinear terms
important?Assumptions:
Neglect curvatureCircular cross section throughout
r = r(z)Constant density in cross section
ρ = ρ(z)And a few others
Calculates heating rate, QCor
photosphere
photosphere
Symmetric about apex
TR
TR
How does Qcor depend on Bphot?
van Ballegooijen et al. 2011 varied Lcor, Bcor
Fit equation for Qcor
Fine structure in m-gram various values of Bphot
Step 3: Reproduce Fine Structure?
Read Bz at z = 0
Calculate B (x, y, z) assuming a potential field
Trace ~108 field lines
Estimate Qcor using eqn3D spatial distribution
Compare to AIA Images
Above: ~75 field linesAbove: AIA Image
taken in 171 Å (~600,000 K)Right: 3D spatial
distribution of Qcor
M-gram and AIA from same date/time
Mag
net
AIA
Im
ag
es
Quantitative Comparison
Quantitative ComparisonM
ag
net
AIA
Im
ag
es
Conclusions What Next?No definitive Alfvén
wavesPossible disagreement
Found Vel ~ 1 km/sTheory ~ 30 km/s
Qcor increases with Bphot
Importance of reflection and nonlinear terms
Can reproduce fine structure
Bright loops possibly result of small loop length
Keep searching increase angular
resolutionDifferentiate between p-mode and Alfvén
waves
Incorporate: loop motions Interactions between
loops
Investigate non-potential models
Questions?
Thank you toAad van Ballegooijen
Kathy Reevesand all the REU Students
for making this both afun and productive
summer