Scientific objectives and capabilities of the Coronal Solar Magnetism Observatory

S. Tomczyk; E. Landi; J. T. Burkepile; R. Casini; E. E. DeLuca; Y. Fan; S. E. Gibson; H. Lin; S. W. McIntosh; S. C. Solomon; G. Toma; A. G. Wijn; J. Zhang

doi:10.1002/2016ja022871

Scientific objectives and capabilities of the Coronal Solar Magnetism Observatory

Journal of Geophysical Research Space Physics ◽

10.1002/2016ja022871 ◽

2016 ◽

Vol 121 (8) ◽

pp. 7470-7487 ◽

Cited By ~ 19

Author(s):

S. Tomczyk ◽

E. Landi ◽

J. T. Burkepile ◽

R. Casini ◽

E. E. DeLuca ◽

...

Keyword(s):

Solar Magnetism

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The Sun as a Magnetic Star

International Astronomical Union Colloquium ◽

10.1017/s0252921100080775 ◽

1976 ◽

Vol 32 ◽

pp. 457-463

Author(s):

John M. Wilcox ◽

Leif Svalgaard

Keyword(s):

Recent Work ◽

Rotation Axis ◽

Polar Field ◽

Magnetic Star ◽

Rotational Axis ◽

Field Variation ◽

The Sun ◽

Arbitrary Angle ◽

Solar Magnetism ◽

Oblique Rotator

SummaryThe sun as a magnetic star is described on the basis of recent work on solar magnetism. Observations at an arbitrary angle to the rotation axis would show a 22-year polar field variation and a 25-day equatorial sector variation. The sector variation would be similar to an oblique rotator with an angle of 90° between the magnetic and rotational axis.

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Solar Magnetism

Science ◽

10.1126/science.95.2462.10.s ◽

1942 ◽

Vol 95 (2462) ◽

pp. 10-10

Keyword(s):

Solar Magnetism

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The Coronal Solar Magnetism Observatory

Proceedings of the International Astronomical Union ◽

10.1017/s1743921317011334 ◽

2017 ◽

Vol 13 (S335) ◽

pp. 359-361 ◽

Cited By ~ 1

Author(s):

Michael J. Thompson ◽

Steven Tomczyk ◽

Sarah E. Gibson ◽

Scott W. McIntosh ◽

Enrico Landi

Keyword(s):

Solar Observatory ◽

Field Of View ◽

Preliminary Design ◽

Research Facility ◽

Plasma Properties ◽

Design Review ◽

Mauna Loa ◽

Solar Magnetism ◽

New Facility ◽

Inner Parts

AbstractThe 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.

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