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The Coronal Solar Magnetism Observatory

Published online by Cambridge University Press:  24 July 2018

Michael J. Thompson ,
Steven Tomczyk ,
Sarah E. Gibson ,
Scott W. McIntosh  and
Enrico Landi
Michael J. Thompson
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, USA email: [email protected], [email protected], [email protected], [email protected]
Steven Tomczyk
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, USA email: [email protected], [email protected], [email protected], [email protected]
Sarah E. Gibson
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, USA email: [email protected], [email protected], [email protected], [email protected]
Scott W. McIntosh
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, USA email: [email protected], [email protected], [email protected], [email protected]
Enrico Landi
Affiliation:
Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109-2143, USA email: [email protected]
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Abstract

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The Coronal Solar Magnetism Observatory (CoSMO) is a proposed new facility led by the High Altitude Observatory and a consortium of partners to measure magnetic field and plasma properties in a large (one degree) field of view extending down to the inner parts of the solar corona. CoSMO is intended as a research facility that will advance the understanding and prediction of space weather. The instrumentation elements of CoSMO are: a white-light coronagraph (KCor), already operational at the Mauna Loa Solar Observatory (MLSO); the Chromosphere and Prominence Magnetometer (ChroMag), due for deployment to MLSO next year; and the CoSMO Large Coronagraph (LC) which has completed Preliminary Design Review.

Keywords

Sun: coronaSun: chromosphereSun: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 359 - 361
Copyright
Copyright © International Astronomical Union 2018 

References

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