Akebono/Suprathermal Mass Spectrometer observations of low‐energy ion outflow: Dependence on magnetic activity and solar wind conditions

By Christopher Cully, E. Donovan, A. Yau, G. G. Arkos. 2003

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Circulation of Heavy Ions and Their Dynamical Effects in the Magnetosphere: Recent Observations and Models (2014, methodology): “For O+, both the density and scale height increase with EUV input, and so a seasonal and a solar cycle effect are observed, as well as short term changes with solar activity (Yau et al. 1985; Cully et al. 2003).”
What makes a planet habitable? (2009, background): “Table 5 from the present terrestrial ionosphere during solar maximum (e.g., Moore et al. 1999; Cully et al. 2003).”
Atmospheric Escape and Evolution of Terrestrial Planets and Satellites (2008, background): “…and the exobase temperature, the observed nonthermal loss rate from the Earth-mass and size planets is much faster than Jeans escape, except for light species like H, H2 and He (e.g., Lundin and Dubinin 1992; Cully et al. 2003; Wahlund et al. 2005 and references therein; Yamauchi and Wahlund 2007).”
How Hospitable Are Space Weather Affected Habitable Zones? The Role of Ion Escape (2017, unknown): “…caused signi ﬁ cant additional iono-spheric out ﬂ ow at Earth, and this effect has been further quanti ﬁ ed by observational statistical studies ( e.g., Cully et al. 2003; Lennartsson et al. 2004 ) and numerical simulation studies ( Yu & Ridley 2009; Damiano et al. 2010; Welling & Liemohn 2014 )…”