SEMBAY, S., A. L. ALME, D. AGNOLON, T. ARNOLD, A. BEARDMORE, A. BELÉN BALADO MARGELI, C. BICKNELL, C. BOULDIN, G. BRANDUARDI-RAYMONT, Jean-Paul Bernhard BREUER (76 Brazílie, domácí), T. BUGGEY, G. BUTCHER, R. CANCHAL, J. A. CARTER, T. CRAWFORD, A. CHENEY, Y. COLLADO-VEGA, H. CONNOR, T. CRAWFORD, N. EATON, C. FELDMAN, C. FORSYTH, T. FRANTZEN, G. GALGÓCZI, J. GARCIA, G. Y. GENOV, C. GORDILLO, H-P. GRÖBELBAUER, M. GUEDEL, Y. GUO, M. HAILEY, D. HALL, R. HAMPSON, J. HASIBA, O. HETHERINGTON, A. HOLLAND, S-Y. HSIEH, M. HUBBARD, H. JESZENSZKY, M. JONES, T. KENNEDY, K. KOCH-MEHRIN, S. KÖGL, S. KRUCKER, K. D. KUNTZ, C. LAKIN, G. LAKY, O. LYLUND, A. MARTINDALE, J. MIGUEL MAS HESSE, R. NAKAMURA, K. OKSAVIK, N. ØSTGAARD, H. OTTACHER, R. OTTENSAMER, C. PAGANI, S. PARSONS, P. PATEL, J. PEARSON, G. PEIKERT, F. S. PORTER, T. POULIANTIS, G. RANDALL, B. H. QURESHI, W. RAAB, G. RANDALL, A. M. READ, N. M. ROQUE, M. E. ROSTAD, C. RUNCIMAN, S. SACHDEV, A. SAMSONOV, M. SOMAN, D. SIBECK, S. SMIT, J. SØNDERGAARD, R. SPEIGHT, S. STAVLAND, M. STELLER, TianRan SUN, J. THORNHILL, W. THOMAS, K. ULLALAND, B. WALSH, D. WALTON, C. WANG a S. YANG
Vydání
Earth and Planetary Physics, Science Press, 2024, 2096-3955
The Soft X-ray Imager (SXI) is part of the scientific payload of the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) mission. SMILE is a joint science mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS) and is due for launch in 2025. SXI is a compact X-ray telescope with a wide field-of-view (FOV) capable of encompassing large portions of Earth’s magnetosphere from the vantage point of the SMILE orbit. SXI is sensitive to the soft X-rays produced by the Solar Wind Charge eXchange (SWCX) process produced when heavy ions of solar wind origin interact with neutral particles in Earth’s exosphere. SWCX provides a mechanism for boundary detection within the magnetosphere, such as the position of Earth’s magnetopause, because the solar wind heavy ions have a very low density in regions of closed magnetic field lines. The sensitivity of the SXI is such that it can potentially track movements of the magnetopause on timescales of a few minutes and the orbit of SMILE will enable such movements to be tracked for segments lasting many hours. SXI is led by the University of Leicester in the United Kingdom (UK) with collaborating organisations on hardware, software and science support within the UK, Europe, China and the United States.
SEMBAY, S., A. L. ALME, D. AGNOLON, T. ARNOLD, A. BEARDMORE, A. BELÉN BALADO MARGELI, C. BICKNELL, C. BOULDIN, G. BRANDUARDI-RAYMONT, Jean-Paul Bernhard BREUER, T. BUGGEY, G. BUTCHER, R. CANCHAL, J. A. CARTER, T. CRAWFORD, A. CHENEY, Y. COLLADO-VEGA, H. CONNOR, T. CRAWFORD, N. EATON, C. FELDMAN, C. FORSYTH, T. FRANTZEN, G. GALGÓCZI, J. GARCIA, G. Y. GENOV, C. GORDILLO, H-P. GRÖBELBAUER, M. GUEDEL, Y. GUO, M. HAILEY, D. HALL, R. HAMPSON, J. HASIBA, O. HETHERINGTON, A. HOLLAND, S-Y. HSIEH, M. HUBBARD, H. JESZENSZKY, M. JONES, T. KENNEDY, K. KOCH-MEHRIN, S. KÖGL, S. KRUCKER, K. D. KUNTZ, C. LAKIN, G. LAKY, O. LYLUND, A. MARTINDALE, J. MIGUEL MAS HESSE, R. NAKAMURA, K. OKSAVIK, N. ØSTGAARD, H. OTTACHER, R. OTTENSAMER, C. PAGANI, S. PARSONS, P. PATEL, J. PEARSON, G. PEIKERT, F. S. PORTER, T. POULIANTIS, G. RANDALL, B. H. QURESHI, W. RAAB, G. RANDALL, A. M. READ, N. M. ROQUE, M. E. ROSTAD, C. RUNCIMAN, S. SACHDEV, A. SAMSONOV, M. SOMAN, D. SIBECK, S. SMIT, J. SØNDERGAARD, R. SPEIGHT, S. STAVLAND, M. STELLER, TianRan SUN, J. THORNHILL, W. THOMAS, K. ULLALAND, B. WALSH, D. WALTON, C. WANG a S. YANG. The Soft X-ray Imager (SXI) on the SMILE Mission. Earth and Planetary Physics. Science Press, 2024, roč. 8, č. 1, s. 5-14. ISSN 2096-3955. Dostupné z: https://dx.doi.org/10.26464/epp2023067.
@article{2359558, author = {Sembay, S. and Alme, A. L. and Agnolon, D. and Arnold, T. and Beardmore, A. and Belén Balado Margeli, A. and Bicknell, C. and Bouldin, C. and BranduardiandRaymont, G. and Breuer, JeanandPaul Bernhard and Buggey, T. and Butcher, G. and Canchal, R. and Carter, J. A. and Crawford, T. and Cheney, A. and ColladoandVega, Y. and Connor, H. and Crawford, T. and Eaton, N. and Feldman, C. and Forsyth, C. and Frantzen, T. and Galgóczi, G. and Garcia, J. and Genov, G. Y. and Gordillo, C. and Gröbelbauer, HandP. and Guedel, M. and Guo, Y. and Hailey, M. and Hall, D. and Hampson, R. and Hasiba, J. and Hetherington, O. and Holland, A. and Hsieh, SandY. and Hubbard, M. and Jeszenszky, H. and Jones, M. and Kennedy, T. and KochandMehrin, K. and Kögl, S. and Krucker, S. and Kuntz, K. D. and Lakin, C. and Laky, G. and Lylund, O. and Martindale, A. and Miguel Mas Hesse, J. and Nakamura, R. and Oksavik, K. and Østgaard, N. and Ottacher, H. and Ottensamer, R. and Pagani, C. and Parsons, S. and Patel, P. and Pearson, J. and Peikert, G. and Porter, F. S. and Pouliantis, T. and Randall, G. and Qureshi, B. H. and Raab, W. and Randall, G. and Read, A. M. and Roque, N. M. and Rostad, M. E. and Runciman, C. and Sachdev, S. and Samsonov, A. and Soman, M. and Sibeck, D. and Smit, S. and Søndergaard, J. and Speight, R. and Stavland, S. and Steller, M. and Sun, TianRan and Thornhill, J. and Thomas, W. and Ullaland, K. and Walsh, B. and Walton, D. and Wang, C. and Yang, S.}, article_number = {1}, doi = {http://dx.doi.org/10.26464/epp2023067}, keywords = {Soft X-ray Imaging; micropore optics; large area CCD}, language = {eng}, issn = {2096-3955}, journal = {Earth and Planetary Physics}, title = {The Soft X-ray Imager (SXI) on the SMILE Mission}, url = {http://dx.doi.org/10.26464/epp2023067}, volume = {8}, year = {2024} }
TY - JOUR ID - 2359558 AU - Sembay, S. - Alme, A. L. - Agnolon, D. - Arnold, T. - Beardmore, A. - Belén Balado Margeli, A. - Bicknell, C. - Bouldin, C. - Branduardi-Raymont, G. - Breuer, Jean-Paul Bernhard - Buggey, T. - Butcher, G. - Canchal, R. - Carter, J. A. - Crawford, T. - Cheney, A. - Collado-Vega, Y. - Connor, H. - Crawford, T. - Eaton, N. - Feldman, C. - Forsyth, C. - Frantzen, T. - Galgóczi, G. - Garcia, J. - Genov, G. Y. - Gordillo, C. - Gröbelbauer, H-P. - Guedel, M. - Guo, Y. - Hailey, M. - Hall, D. - Hampson, R. - Hasiba, J. - Hetherington, O. - Holland, A. - Hsieh, S-Y. - Hubbard, M. - Jeszenszky, H. - Jones, M. - Kennedy, T. - Koch-Mehrin, K. - Kögl, S. - Krucker, S. - Kuntz, K. D. - Lakin, C. - Laky, G. - Lylund, O. - Martindale, A. - Miguel Mas Hesse, J. - Nakamura, R. - Oksavik, K. - Østgaard, N. - Ottacher, H. - Ottensamer, R. - Pagani, C. - Parsons, S. - Patel, P. - Pearson, J. - Peikert, G. - Porter, F. S. - Pouliantis, T. - Randall, G. - Qureshi, B. H. - Raab, W. - Randall, G. - Read, A. M. - Roque, N. M. - Rostad, M. E. - Runciman, C. - Sachdev, S. - Samsonov, A. - Soman, M. - Sibeck, D. - Smit, S. - Søndergaard, J. - Speight, R. - Stavland, S. - Steller, M. - Sun, TianRan - Thornhill, J. - Thomas, W. - Ullaland, K. - Walsh, B. - Walton, D. - Wang, C. - Yang, S. PY - 2024 TI - The Soft X-ray Imager (SXI) on the SMILE Mission JF - Earth and Planetary Physics VL - 8 IS - 1 SP - 5-14 EP - 5-14 PB - Science Press SN - 20963955 KW - Soft X-ray Imaging KW - micropore optics KW - large area CCD UR - http://dx.doi.org/10.26464/epp2023067 N2 - The Soft X-ray Imager (SXI) is part of the scientific payload of the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) mission. SMILE is a joint science mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS) and is due for launch in 2025. SXI is a compact X-ray telescope with a wide field-of-view (FOV) capable of encompassing large portions of Earth’s magnetosphere from the vantage point of the SMILE orbit. SXI is sensitive to the soft X-rays produced by the Solar Wind Charge eXchange (SWCX) process produced when heavy ions of solar wind origin interact with neutral particles in Earth’s exosphere. SWCX provides a mechanism for boundary detection within the magnetosphere, such as the position of Earth’s magnetopause, because the solar wind heavy ions have a very low density in regions of closed magnetic field lines. The sensitivity of the SXI is such that it can potentially track movements of the magnetopause on timescales of a few minutes and the orbit of SMILE will enable such movements to be tracked for segments lasting many hours. SXI is led by the University of Leicester in the United Kingdom (UK) with collaborating organisations on hardware, software and science support within the UK, Europe, China and the United States. ER -
SEMBAY, S., A. L. ALME, D. AGNOLON, T. ARNOLD, A. BEARDMORE, A. BELÉN BALADO MARGELI, C. BICKNELL, C. BOULDIN, G. BRANDUARDI-RAYMONT, Jean-Paul Bernhard BREUER, T. BUGGEY, G. BUTCHER, R. CANCHAL, J. A. CARTER, T. CRAWFORD, A. CHENEY, Y. COLLADO-VEGA, H. CONNOR, T. CRAWFORD, N. EATON, C. FELDMAN, C. FORSYTH, T. FRANTZEN, G. GALGÓCZI, J. GARCIA, G. Y. GENOV, C. GORDILLO, H-P. GRÖBELBAUER, M. GUEDEL, Y. GUO, M. HAILEY, D. HALL, R. HAMPSON, J. HASIBA, O. HETHERINGTON, A. HOLLAND, S-Y. HSIEH, M. HUBBARD, H. JESZENSZKY, M. JONES, T. KENNEDY, K. KOCH-MEHRIN, S. KÖGL, S. KRUCKER, K. D. KUNTZ, C. LAKIN, G. LAKY, O. LYLUND, A. MARTINDALE, J. MIGUEL MAS HESSE, R. NAKAMURA, K. OKSAVIK, N. ØSTGAARD, H. OTTACHER, R. OTTENSAMER, C. PAGANI, S. PARSONS, P. PATEL, J. PEARSON, G. PEIKERT, F. S. PORTER, T. POULIANTIS, G. RANDALL, B. H. QURESHI, W. RAAB, G. RANDALL, A. M. READ, N. M. ROQUE, M. E. ROSTAD, C. RUNCIMAN, S. SACHDEV, A. SAMSONOV, M. SOMAN, D. SIBECK, S. SMIT, J. SØNDERGAARD, R. SPEIGHT, S. STAVLAND, M. STELLER, TianRan SUN, J. THORNHILL, W. THOMAS, K. ULLALAND, B. WALSH, D. WALTON, C. WANG a S. YANG. The Soft X-ray Imager (SXI) on the SMILE Mission. \textit{Earth and Planetary Physics}. Science Press, 2024, roč.~8, č.~1, s.~5-14. ISSN~2096-3955. Dostupné z: https://dx.doi.org/10.26464/epp2023067.