Mauna Loa Solar Observatory (MLSO) acquires unique observations of the Sun’s atmosphere to support NCAR’s goal to address critical gaps in understanding the Sun-Earth system and to provide observations to reduce damage and disruption from space weather hazards.

SERVER MAINTENANCE, March 10 - 12: Expect intermittent outages of this website and data access.

Mauna Loa Solar Observatory is reopening in April 2026! In November 2022, MLSO was closed due to a volcanic eruption that buried parts of the access road to the Observatory. Restoration of the road is now underway and expected to be completed by early April. Following access restoration, we expect MLSO to begin K-Cor observations and CME alert services within 3–4 weeks. UCoMP observations and data services will commence shortly thereafter. See the Mauna Loa volcano eruption page.

NCAR/HAO’s Mauna Loa Solar Observatory will support the Artemis II mission by alerting NASA’s Space Radiation Analysis Group of solar Coronal Mass Ejections (CMEs) that are the root cause of radiation storms in space. MLSO measures CME velocity and direction — key parameters for determining if a CME will cause a radiation storm — on average one hour before NOAA’s operational CCOR coronagraphs on the GOES or Solar-1 satellites. This critical extra lead time enables SRAG operators and the Artemis II crew to plan mitigating actions that can protect the crew from harmful radiation in space.

Latest Images

K-Cor

pB Enhanced Intensity
 
NRGF Enhanced Intensity
 
Cropped movies: pB | NRGF
Fullres movies: pB | NRGF
NEW! K-Cor Annual Movies

UCoMP

Density
 
Enhanced Intensity
 
Doppler Velocity
 
Line Width
 
Linear Polarization
 
Version 1.0.1 FITS data now available

GONG H-alpha

Big Bear Observatory

(Mauna Loa GONG station is offline due to road closure)

● Big Bear GONG movie

● GONG H-alpha Network

Featured Events

  POS B-field map

  2024-03-30: Fast CME

More Data

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