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2014 CISM School Students photograph
January 26, 2015

The CISM Space Weather Summer School (July 13–24, 2015) is intended to give students a comprehensive immersion in the subject of space weather.

January 21, 2015

For the first time a mesoscale-resolving whole atmosphere general circulation model has been developed.

October 27, 2014

A new era starts October 26, 2014, when Scott McIntosh takes on the role of HAO Director.

MLSO Latest Images

H-alpha Disk and Limb

Currently, H-alpha images are obtained by the GONG network, operated by the National Solar Observatory .

GET GONG DATA

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.

GET CoMP DATA

K-Cor White Light Corona

Preliminary K-Cor Data is now available!

GET K-COR DATA

PSPT Blue

PSPT produces seeing-limited full-disk images in the blue continuum, red continuum, CaII K, CaII K Narrow Band Wing (NBW), and CaII K Narrow Band Core (NBC), with 0.1% pixel-to-pixel relative photometric precision.

GET PSPT DATA

PSPT Red

PSPT produces seeing-limited full-disk images in the blue continuum, red continuum, CaII K, CaII K Narrow Band Wing (NBW), and CaII K Narrow Band Core (NBC), with 0.1% pixel-to-pixel relative photometric precision.

GET PSPT DATA

PSPT Ca-K

PSPT produces seeing-limited full-disk images in the blue continuum, red continuum, CaII K, CaII K Narrow Band Wing (NBW), and CaII K Narrow Band Core (NBC), with 0.1% pixel-to-pixel relative photometric precision.

GET PSPT DATA

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