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4 results on '"A. Belén Balado Margeli"'

1. The Soft X-ray Imager (SXI) on the SMILE Mission

Author

S. Sembay, A. L. Alme, D. Agnolon, T. Arnold, A. Beardmore, A. Belén Balado Margeli, C. Bicknell, C. Bouldin, G. Branduardi-Raymont, T. Crawford, J. P. Breuer, T. Buggey, G. Butcher, R. Canchal, J. A. Carter, A. Cheney, Y. Collado-Vega, H. Connor, 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. W. J. 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, B. H. Qureshi, W. Raab, G. Randall, A. M. Read, N. M. 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, and S. Yang

Subjects
soft x-ray imaging, micropore optics, large area ccd, Science, Geophysics. Cosmic physics, QC801-809, Environmental sciences, GE1-350
Abstract

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.

Published
2024
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2. Alignment and integration of the first PLATO camera

Author

Coyle, Laura E., Matsuura, Shuji, Perrin, Marshall D., Royer, P., Baeke, A., Terrasa, G., Huygen, R., Regibo, S., Farinato, J., Magrin, D., Mazzoli, A., Pajas, M., Vandenbussche, B., Hermans, A., Millou, G., Vassallo, D., Belén Balado Margeli, A., Clermont, L., Cottinelli, A., Ferrari, L., Gorius, N., Laauwen, W., Levillain, Y., Novi, A., Pagano, I., Pertenais, M., Ramos Zapata, G., Salatti, M., and Van Kempen, T. A.

Published
2022
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3. Alignment and integration of the first PLATO camera.

Author

Royer, P., Baeke, A., Terrasa, G., Huygen, R., Regibo, S., Farinato, J., Magrin, D., Mazzoli, A., Pajas, M., Vandenbussche, B., Hermans, A., Millou, G., Vassallo, D., Belén Balado Margeli, A., Clermont, L., Cottinelli, A., Ferrari, L., Gorius, N., Laauwen, W., and Levillain, Y.

Published
2022
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4. The Soft X-ray Imager (SXI) on the SMILE Mission

Author

Sembay, S., Alme, A.L., Agnolon, D., Arnold, T., Beardmore, A., Belén Balado Margeli, A., Bicknell, C., Bouldin, C., Branduardi-Raymont, G., Breuer, J.P., Buggey, T., Butcher, G., Canchal, R., Carter, J.A., Crawford, T., Cheney, A., Collado-Vega, Y., Connor, H., 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., Lakin1, 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., Read, A.M., Roque, N.M.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., Sembay, S., Alme, A.L., Agnolon, D., Arnold, T., Beardmore, A., Belén Balado Margeli, A., Bicknell, C., Bouldin, C., Branduardi-Raymont, G., Breuer, J.P., Buggey, T., Butcher, G., Canchal, R., Carter, J.A., Crawford, T., Cheney, A., Collado-Vega, Y., Connor, H., 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., Lakin1, 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., Read, A.M., Roque, N.M.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., and Yang, S.

Abstract

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.

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