Skip to main content

Main navigation

U.S. NSF Logo
NSF NCAR Logo
Contact Us
High Altitude Observatory
  • 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
  • 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)
    • Lyon-Fedder-Mobarry (LFM) code
    • MURaM Sunspot Model Output
    • TIEGCM
    • WACCM-X
    • Living With A Star Focus Team
  • Observation
    • Mauna Loa Solar Observatory
    • COSMO
    • Community Spectro-polarimetric Analysis Center
    • Fabry-Perot Interferometers
    • HAO Eclipses
    • McIntosh Synoptic Map Archive
    • NCAR Vacuum Tunnel Facility
    • Solar Maximum Mission
    • The Sun Today
    • WindCube
    • LFDI
  • 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

The McIntosh Archive; Extending a long-term dataset and its applications to solar physics research

The solar spicule forest and parallels with polymeric fluid jets excited in the laboratory

Liutex and Third Generation of Vortex Definition and Identification

Machine Learning Techniques for Predicting the Geoeffectiveness of Coronal Mass Ejections

Observations signatures of coronal heating mechanisms in active region cores

Equatorial Plasma Bubbles and Ionospheric Electrodynamics during Geomagnetic Storms

The Electrojet Zeeman Imaging Explorer (EZIE) mission

Non-thermal Parametric Studies in the Quiet-Sun of the Transition Region

Global Geomagnetic Perturbation Forecasting Using Deep Learning

Physics informed neural networks for solar magnetic field simulations

Pagination

  • Previous page ‹‹
  • Page 8
  • Next page ››
Subscribe to Colloquium

NSF NCAR

  • NSF NCAR Homepage
  • ACOM | Atmospheric Chemistry Observations & Modeling
  • CGD Laboratory
  • 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
  • Education & Training
  • For Staff
  • Government Relations & External Engagement
  • Member Institutions
  • Tech Transfer & Engagement
  • University Collaboration

Subscribe to NCAR|UCAR News

Follow NCAR|UCAR

© 2025 UCAR

  • Privacy
  • Cookies
  • Web Accessibility
  • Terms of Use
  • Copyright Issues
  • Sponsored by U.S. 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 NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. 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 U.S. National Science Foundation.