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
Alfred De Wijn and Roberto Cassini installing ViSP
Mar 15, 2023

First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP

The Sun: Myths and Magnetism
Sep 29, 2022

Watch the BBC's Interview with Philip Judge—The Sun: Myths and Magnetism

Two rows of colorful squares, 8 total, showing coronal geyser jet action
Sep 21, 2022

Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets Publication Name

The solar spectrum seen at low resolution, below the atmospheric cutoff at 3100 Angstrom
Jul 11, 2022

Optimal spectral lines for measuring chromospheric magnetic fields

CLEDB 2-line magnetic inversion algorithm flowchart. An important aspect is the delivery of multiple possible solutions for each observation at the last step. Note that the x-coordinate of the point in space, as well as nearest electron density, are returned along with B. The figure uses the notation Vobs and Vdb for observed and computed values of the amplitudes of the Stokes parameters corresponding to O3 and S3 (B = 1) in the text.
Jul 11, 2022

Efficient and Automated Inversions of Magnetically-Sensitive Forbidden Coronal Lines: CLEDB - The Coronal Line Emission DataBase Magnetic Field Inversion Algorithm

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

Jenna Samra, taken on the Gulfstream V research aircraft
Dec 17, 2021

The 2017 Total Eclipse was a Life-changing Four Minutes

Phil Judge and Roberto Cassini
Dec 17, 2021

P Judge and R Casini Advise Early Career Researchers

Images to highlight the corrugated surfaces at which the centers of UV lines are formed (close to τ = 1) in MURaM calculations of the upper solar chromosphere
Nov 18, 2021

AAS Nova Features a Recent Publication by Philip Judge

Seasonally averaged data for the CaII“S-index” and for the average magnitudes of the Strömgrenbplusy filters are shown for the star 18 Sco
Nov 18, 2021

Sun-Like Stars Shed Light on Solar Climate Forcing

Pagination

  • Page 1
  • Next page ››
Subscribe to Phil Judge

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.