Temporal variations of geocoronal and heliospheric X‐ray emission associated with the solar wind interaction with neutrals

By T. Cravens, I. Robertson, S. Snowden. 2001

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Energy spectra of the soft X-ray diffuse emission in fourteen fields observed with Suzaku (2009, background): “The spectrum below 1 keV could be contaminated by the SWCX induced emission from the geocorona (e.g. Cravens et al. (2001)).”
The Galaxy in Context: Structural, Kinematic, and Integrated Properties (2016, background): “There is an additional difficulty in disentangling the contribution of the Local Bubble, a supernova remnant in which the Solar System is embedded (Snowden et al. 1990), and the contribution from solar wind charge-exchange processes, which produce soft X-ray emission throughout the Solar System (Cra”
CONSTRAINING THE MILKY WAY'S HOT GAS HALO WITH O vii AND O viii EMISSION LINES (2014, background): “…X-ray emission source where neutral hydrogen and helium atoms undergo charge exchange reactions with solar wind ions in and around our solar system (Cravens et al. 2001; Snowden et al. 2004; Wargelin et al. 2004; Carter & Sembay 2008; Koutroumpa et al. 2007; Kuntz & Snowden 2008; Carter et al.…”
X-rays from solar system objects (2007, methodology): “stellar helium also gets ionized as it passes the Sun; however, due to the gravitational pull, there is gravitational focusing, giving rise to the high density helium cone in the down wind direction. Cravens et al. (2001) created a simple SWCX model to study the time-dependent behavior of X-ray emis”