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Measuring the magnetic vector with the He I 10830 Å line: A rich new world

MPS-Authors
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Solanki,  S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Lagg,  A.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Aznar Cuadrado,  R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Wiegelmann,  T.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Woch,  J.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Sasso,  C.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Krupp,  N.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Solanki, S. K., Lagg, A., Aznar Cuadrado, R., Orozco, D., Collados, M., Wiegelmann, T., et al. (2006). Measuring the magnetic vector with the He I 10830 Å line: A rich new world. In R. Casini, & B. W. Lites (Eds.), Solar Polarization 4 (pp. 431-436).


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-FCB0-2
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