TIEGCM

Data-Driven Ensemble Modeling of Equatorial Ionospheric Electrodynamics

Graphic depicting root-mean-square difference of the plasma drift
Thursday, February 4, 2021

A Case Study During a Minor Storm Period Under Solar Minimum Conditions: The dayside equatorial ionospheric electrodynamics exhibits strong variability driven simultaneously by highly changeable external forcings that originate from the Sun, magnetosphere, and lower atmosphere.

Modeling Diurnal Variation Magnetic Fields for Mantle Induction Studies

Graphic image of the magnetic Bx component
Thursday, January 28, 2021

Accurate models of the spatial structure of ionospheric magnetic fields in the daily variation (DV) band (periods of approximately a few hours to a day) would enable use of magneto-variational methods for three-dimensional imaging of upper mantle and transition zone electrical conductivity.

Planetary wave (PW) generation in the thermosphere driven by the PW-modulated tidal spectrum

Graphic image of Q6DW zonal wind amplitudes
Thursday, July 16, 2020

The National Center for Atmospheric Research thermosphere-ionosphere-electrodynamics general circulation model (TIE-GCM) is used to conduct numerical experiments that isolate and elucidate a substantial modication of the quasi-6-day wave (Q6DW) above 110 km due to presence of the planetary wave (

Tingting Yu

Tingting Yu is a scientific visitor in the High Altitude Observatory of the National Center for Atmospheric Research hosted by Dr. Wenbin Wang. She is a Ph.D. student in the Institute of Geology and Geophysics, Chinese Academy of Sciences.

Haonan Wu

Haonan Wu is a visiting scientist in the High Altitude Observatory (HAO) at the National Center for Atmospheric Research (NCAR). Haonan graduated from the University of Science and Technology of China and obtained his BS degree in Space Physics in 2017. He joined Clemson University in Fall 2017.

Xuguang Cai

Xugang Cai is a postdoctoral fellow II in the High Altitude Observatory at NCAR. He is working on the investigation of the thermosphere and ionosphere by GOLD satellite and numerical models (TIEGCM).

New 2018 HIWIND Thermospheric Wind Observations

Graphs depicting 2018 HIWIND Thermospheric Wind Observations
Thursday, June 13, 2019

Daytime thermospheric winds observed by the balloon-borne instrument HIWIND (High altitude Interferometer WIND experiment) during two flights in June 2011 and 2018 from Kiruna (68°N, 20°E), along with simultaneous EISCAT (European Incoherent SCATter radar) ion drift data, are analyzed.

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