magnetic fields in spicules arturo lópez ariste roberto casini (hao)

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Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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Page 1: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Magnetic fields in spicules

Arturo López AristeRoberto Casini (HAO)

Page 2: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)
Page 3: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)
Page 4: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)
Page 5: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Broadened profiles

Page 6: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Broadened profiles

Page 7: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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

Page 8: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Subpixel velocity distributions

Page 9: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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

Page 10: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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

Page 11: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Scattering Geometry

Page 12: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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

Page 13: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Synthetic broad profiles inverted

Page 14: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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!

Page 15: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)
Page 16: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Error bars are not always

just white noise

Page 17: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Inversion of real data: Distribution of inferred field strengths

Page 18: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

Not yet done!

Page 19: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

The 90 degrees ambiguity

BBBQ 2cossin)1cos3(8

3 22

Page 20: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)
Page 21: Magnetic fields in spicules Arturo López Ariste Roberto Casini (HAO)

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.