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Development of Laboratory Experimental System to Clarify Solar Wind Charge Exchange Mechanism with TES Microcalorimeter

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Abstract

Significant fraction of the cosmic diffuse soft X-ray emission (0.1–1 keV) is caused by the Solar Wind Charge eXchange (SWCX) process between the solar wind ion (Cq+, Nq+, Oq+ etc.) and the interplanetary neutral matter. It is difficult to identify spectral features of SWCX with the spectral resolution of existing X-ray astronomy satellites. We are developing a laboratory experimental system with transition edge sensor (TES) X-ray microcalorimeters, in order to clarify the SWCX mechanism. This experiment is designed to measure Charge eXchange (CX) X-rays using Electron Cyclotron Resonance Ion Source (ECRIS) that generates multi-charged ions. Emission lines (OVIII: 2p→1s; 654 eV) by CX between O8+ and neutral He atom is aimed to be measured with energy resolution better than 10 eV. The TES microcalorimeter is cooled by a double-stage adiabatic demagnetization refrigerator (DADR), however, our TES microcalorimeter are not working potentially due to magnetic field contamination. This paper reports our experimental system, present results, and future prospects.

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Correspondence to T. Enoki.

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Enoki, T., Ishisaki, Y., Akamatsu, H. et al. Development of Laboratory Experimental System to Clarify Solar Wind Charge Exchange Mechanism with TES Microcalorimeter. J Low Temp Phys 167, 771–776 (2012). https://doi.org/10.1007/s10909-012-0486-x

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  • DOI: https://doi.org/10.1007/s10909-012-0486-x

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