Motions of the equatorial ionization anomaly crests imaged by FORMOSAT‐3/COSMIC

By C. Lin, J. Liu, T. Fang, P. Chang, H. Tsai, C. Chen, C. Hsiao. 2007

183 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/d8e802e9a4d4471d6c066b6e02e261065ed008db

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In Aerospace Engineering

1. C. Liu
2. Shin-Yi Su

In Astronomy and Astrophysics

1. C. Liu
2. Shin-Yi Su
3. S. T. Ram

In Geophysics

1. C. Liu
2. Shin-Yi Su

Citations in the corpus

• FORMOSAT-3/COSMIC observations of seasonal and longitudinal variations of equatorial ionization anomaly and its interhemispheric asymmetry during the solar minimum period (2009, methodology): “Further, it can be seen from Figure 4 that the EIA crests appear stronger in the winter (southern) hemisphere during morning to noon hours from 0700 to 1300 LT, and they appear stronger in the summer (northern) hemisphere during afternoon hours from 1400 LT. This corroborates with the observations m”
• Exploring earth's atmosphere with radio occultation: contributions to weather, climate and space weather (2011, unknown): “Figure 39 shows the vertically integrated electron content in two layers, between 100 and 500 km and 300–350 km altitude (Lin et al., 2007c).”