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
neutral density perturbation observed by CHAMP and GRACE
Dec 16, 2022

Thermospheric Density Perturbations Produced by Traveling Atmospheric Disturbances during August 2005 Storm

TIEGCM vertical ExB drift
Dec 16, 2022

The Ionospheric Connection Explorer - Prime Mission Review

ICON MIGHTI track
Dec 16, 2022

Pronounced suppression and X-pattern merging of equatorial ionization anomalies after the 2022 Tonga volcano eruption

Neutral density variations along the Starlink orbit
Nov 23, 2022

Thermospheric Neutral Density Variation during the "SpaceX" Storm: Implications from Physics-based Whole Geospace Modeling

Students and lecturers assembled together outdoors at the Embassy Suites patio area
Aug 30, 2022

2022 Space Weather Summer School

Center for Geospace Storms: Transforming the understanding and predictability of space weather
Jul 11, 2022

The Multiscale Atmosphere-Geospace Environment (MAGE) model

Erupting prominence
Apr 4, 2022

2023 UCAR/NCAR Summer Program: Heliophysics

Jack Eddy
Mar 4, 2022

3rd Eddy Cross Disciplinary Symposium 2022

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

Cover of Jack Eddy's book
Nov 22, 2021

The Sun, The Earth, and Near-Earth Space

Pagination

  • Page 1
  • Next page ››
Subscribe to space weather

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.