Observations

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

MLSO Publications

1024 References, 33 abstracts, and 133 citations as of January, 2017.

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 publications relating to Mauna Loa data which are NOT posted on this listing, please send the reference information via e-mail to:

MLSO Instruments

MLSO Data and Movies

Welcome to Boulder Solar Alliance (BSA)

Boulder is fortunate to have one of the greatest concentrations of solar physics institutes in the world. To encourage communication among researchers from these institutes, we have formed the BSA with representation from:

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