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Solar maximum

About the Mauna Loa Solar Observatory

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Development and Validation of the Whole Atmosphere Community Climate Model with Thermosphere and Ionosphere Extension (WACCM-X)

WACCM-X simulations image
Wednesday, February 14, 2018

H.Liu et al. have improved a comprehensive numerical model, the Whole Atmosphere Community Climate Model with thermosphere and ionosphere extension (WACCM-X).

Solar Maximum Mission Information and Data on the MLSO website

Submitted by kolinski on December 22, 2014 - 12:41pm

The Solar Maximum Mission (SMM) satellite was launched in 1980 aboard a NASA Delta rocket. Among SMM's primary science objectives was the study of the dynamics of solar flares and the study of solar magnetic fields associated with the flare phenomenon. Towards this end, the High Altitude Observatory (HAO) provided a white-light coronagraph/polarimeter (C/P) to study the relationship of the corona to the flare process.

Long-Term Solar Variability

Overview and Research Goal

Solar Maximum Mission Coronagraph

This will be the SMM instrument page.

COMING SOON!

Observing the Quiet Sun: A Weak Cycle Offers Opportunity for Expanding Solar Understanding

Observing the Quiet Sun

Since the dawn of the Space Age in the 1950s, solar maxima have coincided with strong upticks in sunspot activity but the current cycle, Cycle 24, which was expected to peak in Spring of 2013, has been unusually quiet.

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The National Center for Atmospheric Research is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.