Preliminary Design Review: PCA Integrated Radar-Tracker Application

2002 ◽  
Author(s):  
J. M. Lebak
2017 ◽  
Vol 13 (S335) ◽  
pp. 359-361 ◽  
Author(s):  
Michael J. Thompson ◽  
Steven Tomczyk ◽  
Sarah E. Gibson ◽  
Scott W. McIntosh ◽  
Enrico Landi

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.


Author(s):  
Emily A. Beckman ◽  
David J. Benson ◽  
Daniel Cataldo ◽  
Wanyi Ng

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