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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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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
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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
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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
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September 27, 2005Center for Solar-Terrestrial Research Schlichenmaier and Collados (2002)
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September 27, 2005Center for Solar-Terrestrial Research Bellot Rubio et al. (2004)
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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
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September 27, 2005Center for Solar-Terrestrial Research Unno’s Equations
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September 27, 2005Center for Solar-Terrestrial Research Transfer of Polarized Light Longitudinal magnetic field Radiative transfer equations
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September 27, 2005Center for Solar-Terrestrial Research Transverse magnetic field Radiative transfer equations
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September 27, 2005Center for Solar-Terrestrial Research SOLIS
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