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First results of Chinese particle instruments in the Double Star Program
J. B. Cao, Z. X. Liu, C. X. Yan, C. L. Cai, Z. Y. Li, G. W. Zhu, S. R. Wang, H. Zhao, J. B. Liang, Q. Y. Ren, Y. Y. Zai, H. R'Eme, I. Dandouras, C. Aoustin, P. Escoubet, A. Fazakerley, S. Mckenna-Lawlor, M. Dunlop

First results of Chinese particle instruments in the Double Star Program

Science & Mathematics Published 2005 Verification Pending

Overview & Synopsis

Double Star Program (DSP) aims to investigate the trigger mechanism and physical models of geomagnetic storms and substorms. The DSP involves two satellites: the equatorial satellite of DSP (TC-1 in China) and the polar satellite of DSP (TC-2 in China). On board the two satellites of TC-1 and TC-2, there are four kinds of particle instruments developed by the Center for Space Science and Applied Research (CSSAR), namely: the High Energy Electron Detector (HEED, TC-1, 2), the High Energy Proton Detector (HEPD, TC-1, 2), the High Energy Heavy Ion Detector (HID, TC-1, 2) and the Low Energy Ion Detector (LEID, TC-2). HEED, HEPD and HID were developed and calibrated in China. The LEID was developed in China and calibrated in France. This paper introduces the scientific objectives and characteristics of each instrument, their status and some preliminary results.

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Document Information

Document Title First results of Chinese particle instruments in the Double Star Program
Author / Organization J. B. Cao, Z. X. Liu, C. X. Yan, C. L. Cai, Z. Y. Li, G. W. Zhu, S. R. Wang, H. Zhao, J. B. Liang, Q. Y. Ren, Y. Y. Zai, H. R'Eme, I. Dandouras, C. Aoustin, P. Escoubet, A. Fazakerley, S. Mckenna-Lawlor, M. Dunlop
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2005
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-141302
Original Source Link Visit Source Page on hal.science »