Front Page

Recent News

HAO 75th Anniversary Save the Date
March 5, 2015

Announcing HAO’s 75th Anniversary celebration; a three day event scheduled for September 1-3, 2015. The theme will be “HAO: Past, Present and Future”.

2014 CISM School Students photograph
The CISM Space Weather Summer School
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.

Linking terrestrial and space weather using high-resolution WACCM
January 21, 2015

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

More news in our archive >>

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

People Profile

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.