Solar activity variations of the Venus thermosphere/ionosphere

By J. Fox, K. Y. Sung. 2001

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Thermal escape of carbon from the early Martian atmosphere (2009, methodology): “In order to apply the model to a CO2-dominated upper atmosphere, electron impact cross sections [Sawada et al., 1972] for both CO2 and CO were added to the GLOW model, and atomic carbon chemistry reactions from Fox and Sung [2001] were included.”
Is Proxima Centauri b Habitable? A Study of Atmospheric Loss (2017, methodology): “…to PCb values, using the EUV estimate from Ribas et al. (2016), the latter being around 33 times that received by the Earth. cRate coefficient from Fox & Sung (2001). atmosphere from Ma et al. (2013) is: [CO2]=1.0 · 10 15 · e−(z−z0)/5.5 cm−3, (1) [O] =2.0 · 1011 · e−(z−z0)/17 cm−3. where z0 = 100…”
Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere (2015, methodology): “, suprathermal electrons) that ionize these same neutral species (especially on the nightside), and (3) subsequent ion-neutral photochemical reactions [e.g., Fox, 2004; Fox and Sung, 2001; Fox and Yeager, 2009].”
Three‐dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars (2004, unknown): “H+ +O ! O+ + H 5.08 � 10 10 cm 3s 1 Fox and Sung [2001]”