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Physics 681: Solar Physics and Instrumentation – Lecture 9 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.

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Presentation on theme: "Physics 681: Solar Physics and Instrumentation – Lecture 9 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research."— Presentation transcript:

1 Physics 681: Solar Physics and Instrumentation – Lecture 9 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research

2 September 27, 2005Center for Solar-Terrestrial Research Polarimetry  Zeeman splitting  Assume weak magnetic field (LS or Russel-Saunders coupling)  Quantum numbers: L orbital angular momentum of the electrons, S spin angular momentum, J total angular momentum, and M J magnetic quantum number  Landé factor  Displacement of the line in the presence of a magnetic field  Normal Zeeman effect or Lorentz triplet: S = S’ = 0 and ΔM J = –1, 0, +1  g* = –1, 0, +1

3 September 27, 2005Center for Solar-Terrestrial Research http://w.home.cern.ch/w/wadhwa/www/zeeman.html Normal and Anomalous Zeeman Effect http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/sodzee.html

4 September 27, 2005Center for Solar-Terrestrial Research  Solar spectral lines are broadened by micro- and macro-turbulence and by pressure  the components of a Zeeman multiplet are normally not resolved  The triplet consists of two shifted σ-components and an unshifted π- component  Longitudinal Zeeman effect: line-of-sight (LOS) || B  σ-components with circular polarization of opposite sense  Transverse Zeeman effect: LOS ̲|̲̲ B  π-component (linearly polarized ̲|̲̲ B ) and σ-components (linearly polarized || B )  Δλ B ≈ λ 2  Δλ D ≈ λ  Polarized light (propagating in the z-direction)  Stokes vector

5 September 27, 2005Center for Solar-Terrestrial Research Schlichenmaier and Collados (2002)

6 September 27, 2005Center for Solar-Terrestrial Research Bellot Rubio et al. (2004)

7 September 27, 2005Center for Solar-Terrestrial Research  Superposition of a large number of independent waves  Degree of polarization  Stokes profiles I(λ), Q(λ), U(λ), and V(λ)  Longitudinal Zeeman triplet

8 September 27, 2005Center for Solar-Terrestrial Research Unno’s Equations

9 September 27, 2005Center for Solar-Terrestrial Research Transfer of Polarized Light  Longitudinal magnetic field  Radiative transfer equations

10 September 27, 2005Center for Solar-Terrestrial Research  Transverse magnetic field  Radiative transfer equations

11 September 27, 2005Center for Solar-Terrestrial Research SOLIS


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