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October 27, 2014

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

Image of the DKIST site at Haleakala, Maui
October 25, 2014

Four HAO scientists took part in the Daniel K. Inouye Solar Telescope (DKIST) Science Working Group (SWG) Meeting on Maui, Hawaii, from 23-25 October 2014.

Image of coronal mass ejection
May 9, 2014

NCAR solar physicist Scott McIntosh is raising awareness. While the current peak in the 11-year cycle of sunspot activity is on the weak side, the Sun might still produce a major storm at any point.

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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