跳到主要內容部分
NCAR is Sponsored by the National Science Foundation
DASH Search
  • 首頁
  • 資源
  • Collections
  • 關於
  1. 首頁
  2. 組織
  3. opensky
  4. Investigation of the...
  • 資源
  • 動態牆
  • Gravatar admin 建立了資料集 Investigation of the interhemispheric asymmetry in reverse convection near solstice during northward interplanetary magnetic field conditions using MHD simulations
    5 個月前

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

  • 關於 DASH Search
  • CKAN API
  • 登入

Powered by CKAN

ckan
Using 882f16b6d from branch HEAD.
Last updated 2026-06-10 13:55:09.
ckanext-dsetsearch
Using 8a55c47 from branch main.
Last updated 2026-06-10 13:55:10.
© 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.