Podrobný výpis o publikaci

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.

Další formáty: BibTeX LaTeX RIS

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  -

Základní údaje
Originální název	The Soft X-ray Imager (SXI) on the SMILE Mission
Autoři	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.

Další údaje
Originální jazyk	angličtina
Typ výsledku	Článek v odborném periodiku
Obor	10308 Astronomy
Stát vydavatele	Čína
Utajení	není předmětem státního či obchodního tajemství
WWW	URL
Impakt faktor	Impact factor: 2.900 v roce 2022
Organizační jednotka	Přírodovědecká fakulta
Doi	http://dx.doi.org/10.26464/epp2023067
UT WoS	001170454300002
Klíčová slova anglicky	Soft X-ray Imaging; micropore optics; large area CCD
Štítky	rivok
Příznaky	Mezinárodní význam, Recenzováno
Změnil	Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 25. 3. 2024 11:52.

Anotace
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.

Anotace

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.