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A Rare Transit of Venus Across the Sun

Venus in the corona

The Marshall Field Site

Damon Burke and Steve Tomczyk standing in front of optical equipment at Marshall Fields

HIWIND Prepares for a New Zealand Flight in 2022

HiWind instrument during final flight preparations in Kiruna, Sweden, June, 2011

Dynamics of Late-Stage Reconnection in the 2017 September 10 Solar Flare

White light images (upper panels A and B) from HAO's KCOR instrument are shown with Fe XIII emission line polarization data (HAO's CoMP instrument) acquired one day after the initial flare was released

Mapping the magnetic field in the solar corona through magnetoseismology

Analysis results for the observation on November 3, 2016 (dataset D2)

Design of a Highly Efficient Polychromatic Full-Stokes Polarization Modulator for the CRISP Imaging Spectrometer

Example spectro-polarimetric data of Active Region 12471 in the Fe I lines at 630.2 nm

Pagination

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This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.