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Point spread function of SDO/HMI and the effects of stray light correction on the apparent properties of solar surface phenomena

MPS-Authors
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Yeo,  K. L.
IMPRS on Physical Processes in the Solar System and Beyond, 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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Feller,  A.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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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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Danilovic,  S.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104034

Krivova,  N. A.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Yeo, K. L., Feller, A., Solanki, S. K., Couvidat, S., Danilovic, S., & Krivova, N. A. (2014). Point spread function of SDO/HMI and the effects of stray light correction on the apparent properties of solar surface phenomena. Astronomy and Astrophysics, 561: A22. doi:10.1051/0004-6361/201322502.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0026-C87B-7
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