Skip to main content
Progress in Earth and Planetary Science
Fig. 3 | Progress in Earth and Planetary Science

Fig. 3

From: An electrodynamics model for Data Interpretation and Numerical Analysis of ionospheric Missions and Observations (DINAMO)

Fig. 3

Behavior of the vertical plasma drifts as a function of local time for different seasons (rows) and solar flux conditions (columns). The blue curves represent results from the DINAMO model at 360 km. The green curves represent the Jicamarca ISR observations presented by Shidler et al. (2019) for altitudes of 360±40 km. The red curves correspond to vertical drifts predicted by the SF99 model

Back to article page