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- W2018255364 abstract "Charge exchange (CX) is a basic physical process involving the transfer of bound electrons between colliding particles. In the solar system, highly-charged solar wind ions collide with neutral particles from cometary and planetary (e.g. Mars, Earth) environments, as well as interstellar atoms sweeping through the heliosphere, and produce X-rays through radiative decay. I will present an overview of our current knowledge of the CX X-ray emission, focusing mainly on the heliospheric component which, along with CX emission from the Earth's geocorona, surrounds Earth-bound observatories and adds a variable background to all X-ray observations. Current studies combine theoretical modeling and observational analyses from Suzaku, XMM-Newton and Chandra in order to constrain this emission and its contribution to the diffuse soft X-ray background." @default.
- W2018255364 created "2016-06-24" @default.
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- W2018255364 date "2012-01-01" @default.
- W2018255364 modified "2023-09-25" @default.
- W2018255364 title "Charge exchange X-ray emission in the heliosphere and beyond" @default.
- W2018255364 doi "https://doi.org/10.1063/1.3696147" @default.
- W2018255364 hasPublicationYear "2012" @default.
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