Skip to main content
NCAR is Sponsored by the National Science Foundation
DASH Search
  • ホーム
  • リソース
  • Collections
  • About
  1. ホーム
  2. 組織
  3. NCAR
  4. Impact of subsurface...
  • リソース
  • アクティビティストリーム
  • Gravatar admin created the データセット Impact of subsurface convective flows on the formation of sunspot magnetic field and energy build-up
    3 か月前

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
  • Education & Training
  • For Staff
  • Government Relations & External Engagement
  • Member Institutions
  • Tech Transfer & Engagement
  • University Collaboration

DASH Search

    Questions? Contact datahelp@ucar.edu

  • About DASH Search
  • CKAN API
  • ログイン

Powered by CKAN

ckan
Using 9714f3d87 from branch HEAD.
Last updated 2026-01-21 15:59:10.
ckanext-dsetsearch
Using 08b1b29 from branch main.
Last updated 2026-01-21 15:59:10.
© 2024 UCAR Privacy Cookies Accessibility Terms of use Copyright issues Sponsored by NSF Report ethics concern
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.