<p><strong>Particle-induced emission of X-rays from the Europa (100-10 keV)</strong></p>
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dc |
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Title Statement |
<p><strong>Particle-induced emission of X-rays from the Europa (100-10 keV)</strong></p> |
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Added Entry - Uncontrolled Name |
BRIGHT, SMART KUNDASSERY; DEPARTMENT OF ATMOSPHERIC SCIENCES, SCHOOL OF MARINE SCIENCES, COCHIN UNIVERSITY OF SCIENCE AND TECHNOLOGY BABU, CHETHALAN ANTONY; DEPARTMENT OF ATMOSPHERIC SCIENCES, SCHOOL OF MARINE SCIENCES, COCHIN UNIVERSITY OF SCIENCE AND TECHNOLOGY COCHIN UNIVERSITY OF SCIENCE AND TECHNOLOGY |
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Uncontrolled Index Term |
SPACE PHYSICS, PLANETARY ATMOSPHERE EUROPA, JOVIAN, MAGNETOSPHERE, X-RAYS, H2O ICE |
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Summary, etc. |
We considered the interaction of H<sup>+</sup>, O<sup>+</sup> and S<sup>+</sup> ions of spectral energy range 100-10 keV with the predominant H2O ice composition of the surface of the Jovian Europa, and developed a model to quantify the ion-induced emission of X-rays from the satellite during its three encounters with Galileo mission flyby (E12, E19, E26). To achieve this, we computed the stopping power of H2O ice using SRIM code, and X-ray ionization cross sections of interaction for the ions with H2O ice using ISICS14 code. We found that the integrated fluxes of H<sup>+</sup>, O<sup>+</sup> and S<sup>+</sup> ions are seen as lower above the current sheet (E19) and enhanced through the centre of the current sheet (E12) and below the current sheet (E26). The proton-induced energy flux received at the telescope of the Chandra X-ray Observatory (ergs-cm<sup>-2</sup>-s<sup>-1</sup>) during E12 encounter is 9.49E-11, during E19 encounter is 4.79E-11, and during E26 encounter is 9.39E-11. The energy flux generated by O^+ and S^+ ions is found as trivial in comparison to the proton-induced energy flux (100-10 keV). |
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Publication, Distribution, Etc. |
Indian Journal of Radio & Space Physics (IJRSP) 2022-04-27 14:43:08 |
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Electronic Location and Access |
application/pdf http://op.niscair.res.in/index.php/IJRSP/article/view/57489 |
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Data Source Entry |
Indian Journal of Radio & Space Physics (IJRSP); ##issue.vol## 50, ##issue.no## 4 (2021): IJRSP DECEMBER 2021 |
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Language Note |
en |
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