Mauna Loa Solar Observatory - MLSO

COronal Multi-channel Polarimeter

The CoMP instrument (see Tomczyk, et al. 2008) can observe the coronal magnetic field with a full FOV in the low corona (~1.03 to 1.5 Rsun), as well as obtain information about the plasma density and motion. Like Solar-C, CoMP records the intensity and the linear and circular polarization (Stokes I,Q,U,V) of the forbidden lines of Fe XIII at 1074.7 nm and also at 1079.8 nm.

Solar Maximum Mission Coronagraph

This will be the SMM instrument page.

COMING SOON!

COSMO K-Coronagraph (K-Cor)

K-Cor on the Spar

K-Cor on the MLSO spar

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MLSO Users' Committee

The Mauna Loa Solar Observatory (MLSO) is a facility of the National Center for Atmospheric Research (NCAR) and is operated by the High Altitude Observatory (HAO). It provides observations of the solar photosphere, chromosphere and corona in order to understand the Sun’s continuous release of plasma and energy into interplanetary space and the impacts at Earth. HAO is committed to providing the community with critically important, high-quality solar observations.

MLSO Publications (by author)

Order by: Author | Year

1116 publications, 57 abstracts, and 260 citations as of 2021-02-12.

It is hoped that this listing will be of use to the scientific community. The current list is incomplete. If you are aware of any

MLSO Instruments

MLSO Data and Movies

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