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HiWIND team, Kiruna, Sweden
June 29, 2018

Finally, after repeated postponements due to unfavorable weather conditions, HiWind launched from Esrange Space Center, Kiruna, Sweden, on Sunday, 24 June. The HiWIND team arrived early May 2018. During May, they assembled the gondola and mounted numerous specialized instrumentation in preparation for a June launch.

Hanli Liu-CEDAR Prize Lecture
June 28, 2018

Hanli Liu gave the CEDAR Prize Lecture on Thursday, June 28th, at the CEDAR Summer Workshop in Santa Fe, New Mexico. The Prize Lecture was awarded in recognition of the work accomplished on the Whole Atmosphere Community Climate Model–eXtended (WACCM-X) and the paper describing it that was recently published in the Journal of Advances in Modeling of Earth Systems.

Publication Highlights

MLSO total eclipse, 1980 February 16, India
June 18, 2018

BC Low elaborates on the extraordinary sixty years of progress made to space observation of the Sun, solar wind, planets and their magnetospheres. He notes that space platforms complementing ground-based observatories have transformed solar physics.

The time evolution of height-dependent (a) electron density, (b) ionization rate, (c) Pedersen conductivity, and (d) Hall conductivity at MLT = 6 and magnetic latitude of 60
June 18, 2018

Stan Solomon et al, dicuss a new modeling capability that self-consistently couples physics-based magnetospheric 18 electron precipitation with its impact on the ionosphere, representing a significant improvement over previous models.

Change in WACCMX simulated total electron content (TEC) during a geomagnetic
June 18, 2018

Nicholas Pedatella notes that geomagnetic storms are an important driver of variability in Earth’s ionosphere, and can have significant societal impacts through the ionosphere’s impact on communications and navigation systems (e.g., GPS).

MLSO Latest Images

CoMP Coronal Intensity

The COronal Multi-channel Polarimeter (CoMP) observes the Fe-XIII emission line at 1074.7 nm to measure the coronal magnetic field and obtain plasma density and motion in the low corona from ~1.03 to 1.5 solar radii.


K-Cor White Light Corona

Designed to study the formation and dynamics of coronal mass ejections and the evolution of the density structure of the low corona, K-Cor records the polarization brightness (pB).


K-Cor (radially graded filter)

K-Cor image with a normalized radially graded filter (nrgf) to maximize image contrast, especially in the outer field.

These data are ideal for measuring positions of coronal structures such as CMEs and helmet streamers.

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