magnetic fields in spicules arturo lópez ariste roberto casini (hao)
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Magnetic fields in spicules
Arturo López AristeRoberto Casini (HAO)
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Broadened profiles
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Broadened profiles
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Aproach to inversion
1. Get an (empirical) description of the anomalous broadening: A convolution of Doppler-shifted profiles each one given a
weight by a gaussian distribution
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Subpixel velocity distributions
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Aproach to inversion
1. Get an (empirical) description of the anomalous broadening: A convolution of Doppler-shifted profiles each one given a
weight by a gaussian distribution
2. Investigate how much magnetic information is still available in the so-broadened profiles: Create synthetic profiles, broaden them and try to invert
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He I atomic model
2 3P0,1,2
2 3S1
3 3S1
3 3P0,1,2
3 3D1,2,3
5876 Å
7065 Å
3889 Å
10830 Å • 5 atomic terms• L-S coupling
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Scattering Geometry
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Model theory
• Quantum theory of polarized line formation (Landi Degl’Innocenti, 1983)
• Spectrally flat incident radiation (CRD)
• No collisions
• Includes level-crossing and coherence effects within each atomic term
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Synthetic broad profiles inverted
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Aproach to inversion
1. Get an (empirical) description of the anomalous broadening: A convolution of Doppler-shifted profiles each one given a
weight by a gaussian distribution
2. Investigate how much magnetic information is still available in the so-broadened profiles: Create synthetic profiles, broaden them and try to invert
3. Try with the real data and see what happens!
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Error bars are not always
just white noise
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Inversion of real data: Distribution of inferred field strengths
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Not yet done!
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The 90 degrees ambiguity
BBBQ 2cossin)1cos3(8
3 22
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A few conclusions
•Broadened profiles are well reproduced by subpixel velocity distribution (either real or arisen from projection effects)
•Magnetic field in spicules appear to be either ALIGNED or TRANSVERSAL to the visible structure
•Field strengths of up to 40 G are present. No much higher than that though.