Zobrazeno 1 - 2
of 2
pro vyhledávání: '"M. K. Yedla"'
Autor:
R. F. Wimmer-Schweingruber, N. P. Janitzek, D. Pacheco, I. Cernuda, F. Espinosa Lara, R. Gómez-Herrero, G. M. Mason, R. C. Allen, Z. G. Xu, F. Carcaboso, A. Kollhoff, P. Kühl, J. L. Freiherr von Forstner, L. Berger, J. Rodriguez-Pacheco, G. C. Ho, G. B. Andrews, V. Angelini, A. Aran, S. Boden, S. I. Böttcher, A. Carrasco, N. Dresing, S. Eldrum, R. Elftmann, V. Evans, O. Gevin, J. Hayes, B. Heber, T. S. Horbury, S. R. Kulkarni, D. Lario, W. J. Lees, O. Limousin, O. E. Malandraki, C. Martín, H. O’Brien, M. Prieto Mateo, A. Ravanbakhsh, O. Rodriguez-Polo, S. Sánchez Prieto, C. E. Schlemm, H. Seifert, J. C. Terasa, K. Tyagi, R. Vainio, A. Walsh, M. K. Yedla
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics
instname
Astronomy & Astrophysics
Wimmer-Schweingruber, R. F., et al.
[Context] Solar Orbiter strives to unveil how the Sun controls and shapes the heliosphere and fills it with energetic particle radiation. To this end, its Energetic Particle Detector (EPD) has now been in oper
[Context] Solar Orbiter strives to unveil how the Sun controls and shapes the heliosphere and fills it with energetic particle radiation. To this end, its Energetic Particle Detector (EPD) has now been in oper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9541b1eb450f505d352c6ee77621427a
http://hdl.handle.net/10261/263185
http://hdl.handle.net/10261/263185
Autor:
A. Aran, D. Pacheco, M. Laurenza, N. Wijsen, D. Lario, S. Benella, I. G. Richardson, E. Samara, J. L. Freiherr von Forstner, B. Sanahuja, L. Rodriguez, L. Balmaceda, F. Espinosa Lara, R. Gómez-Herrero, K. Steinvall, A. Vecchio, V. Krupar, S. Poedts, R. C. Allen, G. B. Andrews, V. Angelini, L. Berger, D. Berghmans, S. Boden, S. I. Böttcher, F. Carcaboso, I. Cernuda, R. De Marco, S. Eldrum, V. Evans, A. Fedorov, J. Hayes, G. C. Ho, T. S. Horbury, N. P. Janitzek, Yu. V. Khotyaintsev, A. Kollhoff, P. Kühl, S. R. Kulkarni, W. J. Lees, P. Louarn, J. Magdalenic, M. Maksimovic, O. Malandraki, A. Martínez, G. M. Mason, C. Martín, H. O’Brien, C. Owen, P. Parra, M. Prieto Mateo, A. Ravanbakhsh, J. Rodriguez-Pacheco, O. Rodriguez Polo, S. Sánchez Prieto, C. E. Schlemm, H. Seifert, J. C. Terasa, K. Tyagi, C. Verbeeck, R. F. Wimmer-Schweingruber, Z. G. Xu, M. K. Yedla, A. N. Zhukov
Publikováno v:
Astronomy & Astrophysics, 656, pp. 1-8
Astronomy & Astrophysics, 656, 1-8
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 656, ⟨10.1051/0004-6361/202140966⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 656, 1-8
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 656, ⟨10.1051/0004-6361/202140966⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Aran, A., et al.
[Context] In mid-June 2020, the Solar Orbiter (SolO) mission reached its first perihelion at 0.51 au and started its cruise phase, with most of the in situ instruments operating continuously. [Aims] We present the in situ partic
[Context] In mid-June 2020, the Solar Orbiter (SolO) mission reached its first perihelion at 0.51 au and started its cruise phase, with most of the in situ instruments operating continuously. [Aims] We present the in situ partic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08f28d6af6a34b1576e38761d5279c47