The Coronal Solar Magnetism Observatory
Abstract
Measurements of coronal and chromospheric magnetic fields are arguably the most important observables required for advances in our understanding of the processes responsible for coronal heating, coronal dynamics and the generation of space weather that affects communications, GPS systems, space flight, and power transmission. The Coronal Solar Magnetism Observatory (COSMO) is a proposed ground-based suite of instruments designed for routine study of coronal and chromospheric magnetic fields and their environment, and to understand the formation of coronal mass ejections (CME) and their relation to other forms of solar activity. This new facility will be operated by the High Altitude Observatory of the National Center for Atmospheric Research (HAO/NCAR) in support of the solar and heliospheric community. It will replace the current NCAR Mauna Loa Solar Observatory (http://mlso.hao.ucar.edu). COSMO will enhance the value of existing and new observatories on the ground (SOLIS, BBO NST, Gregor, ATST, EST, Chinese Giant Solar Telescope, NLST, FASR) and in space (SOHO, GOES, Hinode, STEREO, SDO, IRIS, Solar-C, Solar Probe+, Solar Orbiter) by providing unique and crucial observations of the global coronal and chromospheric magnetic field and its evolution.
- Publication:
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Solar Heliospheric and INterplanetary Environment (SHINE 2013)
- Pub Date:
- June 2013
- Bibcode:
- 2013shin.confE..54T