Using coronal seismology to estimate the magnetic field strength in a realistic 
coronal model

Chen, F.; Peter, H.

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Using coronal seismology to estimate the magnetic field strength in a realistic coronal model

Chen, F., & Peter, H. (2015). Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. Talk presented at 2nd International Sino-German Symposium of Solar Physics: Multi Waveband Observations and Modeling of Solar Activity. Bad Honnef, Germany. 2015-08-31 - 2015-09-04.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0000-D207-B Version Permalink: https://hdl.handle.net/21.11116/0000-0002-0B03-F

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Creators:
Chen, F.^{1, 2}, Author
Peter, H.², Author

Affiliations:
1IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289

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Dates: Created: 2015

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Identifiers: BibTex Citekey: Chen:2015-166P

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Title: 2nd International Sino-German Symposium of Solar Physics: Multi Waveband Observations and Modeling of Solar Activity

Place of Event: Bad Honnef, Germany

Start-/End Date: 2015-08-31 - 2015-09-04

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