Skip to main content

Main navigation

NCAR Logo

High Altitude Observatory

HAO
Contact Us
  • Home
  • About
    • HAO News
    • History of HAO
    • People
    • Visitor Program
    • Partnerships
    • Organizational Chart
    • Strategic Plan
    • External Advisory Committees
    • Internal Advisory Committees
    • Information for Staff/Visitors
    • Computer Support
  • Research
    • Research Highlights
    • Science Topics
    • Strategic Working Groups
  • Modeling
    • Assimilative Mapping of Ionospheric Electrodynamics (AMIE)
    • Coupled Magnetosphere Ionosphere Thermosphere Model (CMIT)
    • Data-Optimized Coronal Field Model (DOCFM)
    • FORWARD
    • The GLobal airglOW Model (GLOW)
    • Global Scale Wave Model (GSWM)
    • MURaM Sunspot Model Output
    • TIEGCM
    • WACCM-X
    • Living With A Star Focus Team
  • Observation
    • Community Spectro-polarimetric Analysis Center
    • COSMO
    • Fabry-Perot Interferometers
    • HAO Eclipses
    • Mauna Loa Solar Observatory
    • McIntosh Synoptic Map Archive
    • NCAR Vacuum Tunnel Facility
    • Solar Maximum Mission
    • The Sun Today
    • WindCube
  • Education
    • The Sun: A Pictorial Introduction
    • Questions and Answers About the Sun
    • Solar Physics Historical Timeline
    • Famous Solar-Stellar Scientists
    • Solar Astronomy in the Prehistoric Southwest
    • Suggested Reading
    • Additional Educational Resources
  • News & Events
    • News
    • All Upcoming Events
    • Past Events
Contact Us
Fe XIII 1074.68 nm emission over atmospheric absorption (normalized) in the He I Cryo-NIRSP wavelength range with all labeled candidate lines.
Jul 11, 2022

A Spectroscopic Survey of Infrared 1–4 μm Spectra in Regions of Prominent Solar Coronal Emission Lines of Fe XIII, Si X, and Si IX

LC Dome
Mar 7, 2022

NSF Approves Funding for COSMO Next Stage

Damon Burke and Steve Tomczyk of HAO, shown with the COSMO Phase I site survey equipment currently at the NCAR Marshall Field site just south of Boulder Colorado
Mar 7, 2022

COSMO Site and Design Advancement Updates

UCoMP mounted on MLSO spar
Mar 4, 2022

UCoMP Instrument Nearing Science Mission Phase

Domes at MLSO
Dec 17, 2021

MLSO Facility gets a new dome!

Ben Berkey (bearded, lower right) giving tour to 30 people from the International Astronomy Teaching Summit conference
Dec 17, 2021

Outreach and Observing at Mauna Loa in Hawaii

Mk4 images of the solar corona near solar maximum in Jan 2000 and solar minimum
Dec 2, 2021

End of an era: The Mauna Loa K-coronameter is decommissioned

Electrical engineer, Brandon Larson, and Technician Rob Graves install the K-cor center section onto the solar spar at the NCAR Mesa Lab in Boulder
Dec 1, 2021

A New Coronagraph for Mauna Loa

Venus in the corona
Nov 23, 2021

A Rare Transit of Venus Across the Sun

Damon Burke and Steve Tomczyk standing in front of optical equipment at Marshall Fields
Nov 22, 2021

The Marshall Field Site

Pagination

  • Page 1
  • Next page ››
Subscribe to instrumentation

NCAR

  • NCAR Homepage
  • ACOM | Atmospheric Chemistry Observations & Modeling
  • CGD | Climate & Global Dynamics
  • CISL | Computational & Information Systems
  • EdEC | Education, Engagement & Early-Career Development
  • EOL | Earth Observing Laboratory
  • HAO | High Altitude Observatory
  • MMM | Mesoscale & Microscale Meteorology
  • RAL | Research Applications Laboratory

UCAR

  • UCAR Homepage
  • Community Programs
  • Diversity & Inclusion
  • Education & Training
  • For Staff
  • Government Relations & External Engagement
  • Member Institutions
  • Tech Transfer & Engagement
  • University Collaboration

Subscribe to NCAR|UCAR News

Follow NCAR|UCAR

© 2023 UCAR

  • Privacy
  • Cookies
  • Terms of Use
  • Copyright Issues
  • Sponsored by NSF
  • Report Ethics Concern
  • Staff Login
Postal Address: P.O. Box 3000, Boulder, CO 80307-3000 • Shipping Address: 3090 Center Green Drive, Boulder, CO 80301
NSF Logo

This material is based upon work supported by the National Center for Atmospheric Research, a major facility sponsored by the National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the National Science Foundation.