Zobrazeno 1 - 10
of 21
pro vyhledávání: '"G. B. Andrews"'
Autor:
N. Salazar, N. P. Barnes, Fran Bagenal, Matthew E. Hill, A. Harch, H. A. Elliott, S. A. Stern, M. Kusterer, Ralph L. McNutt, George Clark, David E. Kaufmann, Leslie A. Young, John R. Spencer, Peter Delamere, J. A. Kammer, Mihaly Horanyi, R. B. Decker, Stamatios M. Krimigis, L. E. Brown, P. W. Valek, G. B. Andrews, Jon Vandegriff, Donald G. Mitchell, Robert Allen, Michael E. Summers, Joseph Westlake, Kimberly Ennico, K. S. Nelson, Carey M. Lisse, David J. Smith, Peter Kollmann, Harold A. Weaver, Andrew F. Cheng, G. Romeo, M. R. Piquette, Catherine B. Olkin, S. Weidner, S. E. Jaskulek, G. R. Gladstone, E. D. Fattig
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:7413-7424
Pluto energies of a few kiloelectron volts and suprathermal ions with tens of kiloelectron volts and above. We measure this population using the Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) instrument on board the New Horizons
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:
R. Gómez-Herrero, D. Pacheco, A. Kollhoff, F. Espinosa Lara, J. L. Freiherr von Forstner, N. Dresing, D. Lario, L. Balmaceda, V. Krupar, O. E. Malandraki, A. Aran, R. Bučík, A. Klassen, K.-L. Klein, I. Cernuda, S. Eldrum, H. Reid, J. G. Mitchell, G. M. Mason, G. C. Ho, J. Rodríguez-Pacheco, R. F. Wimmer-Schweingruber, B. Heber, L. Berger, R. C. Allen, N. P. Janitzek, M. Laurenza, R. De Marco, N. Wijsen, Y. Y. Kartavykh, W. Dröge, T. S. Horbury, M. Maksimovic, C. J. Owen, A. Vecchio, X. Bonnin, O. Kruparova, D. Píša, J. Souček, P. Louarn, A. Fedorov, H. O’Brien, V. Evans, V. Angelini, P. Zucca, M. Prieto, S. Sánchez-Prieto, A. Carrasco, J. J. Blanco, P. Parra, O. Rodríguez-Polo, C. Martín, J. C. Terasa, S. Boden, S. R. Kulkarni, A. Ravanbakhsh, M. Yedla, Z. Xu, G. B. Andrews, C. E. Schlemm, H. Seifert, K. Tyagi, W. J. Lees, J. Hayes
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 656, ⟨10.1051/0004-6361/202039883⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 656, 1-8
Astronomy & Astrophysics, 656, pp. 1-8
Astronomy and Astrophysics-A&A, 2021, 656, ⟨10.1051/0004-6361/202039883⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 656, 1-8
Astronomy & Astrophysics, 656, pp. 1-8
Gómez-Herrero, R., et al.
Context. Solar Orbiter, launched in February 2020, started its cruise phase in June 2020, in coincidence with its first perihelion at 0.51 au from the Sun. The in situ instruments onboard, including the Energetic Parti
Context. Solar Orbiter, launched in February 2020, started its cruise phase in June 2020, in coincidence with its first perihelion at 0.51 au from the Sun. The in situ instruments onboard, including the Energetic Parti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b8a992322cfe68c3f52bf033a0ba01fe
https://hdl.handle.net/https://repository.ubn.ru.nl/handle/2066/243986
https://hdl.handle.net/https://repository.ubn.ru.nl/handle/2066/243986
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
Autor:
Milan Maksimovic, G. M. Mason, M. E. Wiedenbeck, S. Kolbe, Pertti Makela, A. Ravanbakhsh, N. Vilmer, C. Gordillo, L. Seimetz, Lauri Panitzsch, A. da Silva Fariña, A. Russu, R. Elftmann, Stephan Böttcher, J. R. Hayes, R. Paspirgilis, Aarón Montalvo, S. Begley, Säm Krucker, Óscar Ramón Ramos Gutiérrez, Pablo Parra, Alberto Carrasco, Eduard P. Kontar, Andrew Walsh, Sebastián Sánchez-Prieto, Stefan J. Hofmeister, Karl-Ludwig Klein, J. Tammen, E. Böhm, Olga Malandraki, B. Schuster, K. S. Nelson, F. Espinosa Lara, Jia Yu, Manuel Prieto, Arik Posner, W. Dröge, Neus Agueda, O. Gevin, I. Sánchez, Raúl Gómez-Herrero, C. Terasa, K. Tyagi, Rami Vainio, A. R. Dupont, Juan Jose Blanco, C. E. Schlemm, Angels Aran, Q. Zong, James M. Ryan, A. Kulemzin, Matthew E. Hill, David Lario, Jan Soucek, Jan Köhler, Cesar Martin, Karel Kudela, Robert F. Wimmer-Schweingruber, G. C. Ho, S. Kerem, Javier Rodriguez-Pacheco, T. I. Varela, O. Rodríguez-Polo, D. Meziat, Bernd Heber, O. Limousin, K. Wirth, V. Knierim, D. Pacheco, V. de Manuel González, H. Seifert, J. Almena, Christopher J. Owen, Yulia Kartavykh, Shrinivasrao R. Kulkarni, S. Boden, A. Martínez Hellín, J. J. Connell, S. Eldrum, Christian Drews, H. Önel, I. Cernuda, R. Castillo, Natchimuthuk Gopalswamy, S. Liang, W. J. Lees, Dennis Haggerty, M. Jüngling, Linghua Wang, W. Boogaerts, Silvia Dalla, B. Klecker, Timothy S. Horbury, M. Yedla, M. L Richards, G. B. Andrews, Jan Steinhagen, Blai Sanahuja, G. Mann
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A7. ⟨10.1051/0004-6361/201935287⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A7. ⟨10.1051/0004-6361/201935287⟩
International audience; After decades of observations of solar energetic particles from space-based observatories, relevant questions on particle injection, transport, and acceleration remain open. To address these scientific topics, accurate measure
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed454870d1ce8818b410e0bf2a5d84bc
https://hal.archives-ouvertes.fr/hal-03435908
https://hal.archives-ouvertes.fr/hal-03435908
Autor:
G. M. Mason, C. M. S. Cohen, G. C. Ho, D. G. Mitchell, R. C. Allen, M. E. Hill, G. B. Andrews, L. Berger, S. Boden, S. Böttcher, I. Cernuda, E. R. Christian, A. C. Cummings, A. J. Davis, M. I. Desai, G. A. de Nolfo, S. Eldrum, R. Elftmann, A. Kollhoff, J. Giacalone, R. Gómez-Herrero, J. Hayes, N. P. Janitzek, C. J. Joyce, A. Korth, P. Kühl, S. R. Kulkarni, A. W. Labrador, F. Espinosa Lara, W. J. Lees, R. A. Leske, U. Mall, C. Martin, A. Martínez Hellín, W. H. Matthaeus, D. J. McComas, R. L. McNutt, R. A. Mewaldt, J. G. Mitchell, D. Pacheco, P. Parra Espada, M. Prieto, J. S. Rankin, A. Ravanbakhsh, J. Rodríguez-Pacheco, O. Rodríguez Polo, E. C. Roelof, S. Sánchez-Prieto, C. E. Schlemm, N. A. Schwadron, H. Seifert, E. C. Stone, J. R. Szalay, J. C. Terasa, K. Tyagi, J. L. Freiherr von Forstner, M. E. Wiedenbeck, R. F. Wimmer-Schweingruber, Z. G. Xu, M. Yedla
Publikováno v:
Astronomy & Astrophysics. 656:L12
Context.Following a multi-year minimum of solar activity, a solar energetic particle event on 2020 Nov. 29 was observed by multiple spacecraft covering a wide range of solar longitudes including ACE, the Solar Terrestrial Relations Observatory-A, and
Autor:
R. C. Allen, G. M. Mason, G. C. Ho, J. Rodríguez-Pacheco, R. F. Wimmer-Schweingruber, G. B. Andrews, L. Berger, S. Boden, I. Cernuda, F. Espinosa Lara, J. L. Freiherr von Forstner, R. Gómez-Herrero, J. R. Hayes, S. R. Kulkarni, W. J. Lees, C. Martin, D. Pacheco, O. R. Polo, M. Prieto, A. Ravanbakhsh, S. Sánchez-Prieto, C. E. Schlemm, H. Seifert, J. C. Terasa, K. Tyagi, Z. Xu, M. Yedla
Publikováno v:
Astronomy & Astrophysics. 656:L2
The first orbit of Solar Orbiter provided comprehensive measurements of six corotating interaction regions (CIRs) within 1 au. Five of these CIRs were also observed by ACE at 1 au, allowing for comparisons of the suprathermal ion intensities and spec
Autor:
R. C. Allen, I. Cernuda, D. Pacheco, L. Berger, Z. G. Xu, J. L. Freiherr von Forstner, J. Rodríguez-Pacheco, R. F. Wimmer-Schweingruber, G. C. Ho, G. M. Mason, S. K. Vines, Y. Khotyaintsev, T. Horbury, M. Maksimovic, L. Z. Hadid, M. Volwerk, A. P. Dimmock, L. Sorriso-Valvo, K. Stergiopoulou, G. B. Andrews, V. Angelini, S. D. Bale, S. Boden, S. I. Böttcher, T. Chust, S. Eldrum, P. P. Espada, F. Espinosa Lara, V. Evans, R. Gómez-Herrero, J. R. Hayes, A. M. Hellín, A. Kollhoff, V. Krasnoselskikh, M. Kretzschmar, P. Kühl, S. R. Kulkarni, W. J. Lees, E. Lorfèvre, C. Martin, H. O’Brien, D. Plettemeier, O. R. Polo, M. Prieto, A. Ravanbakhsh, S. Sánchez-Prieto, C. E. Schlemm, H. Seifert, J. Souček, M. Steller, Š. Štverák, J. C. Terasa, P. Trávníček, K. Tyagi, A. Vaivads, A. Vecchio, M. Yedla
Publikováno v:
Astronomy & Astrophysics, 656, pp. 1-11
Astronomy & Astrophysics, 656, 1-11
Astronomy & astrophysics
656 (2021): A7-1–A7-11. doi:10.1051/0004-6361/202140803
info:cnr-pdr/source/autori:Allen R.C.; Cernuda I.; Pacheco D.; Berger L.; Xu Z.G.; Freiherr Von Forstner J.L.; Rodriguez-Pacheco J.; Wimmer-Schweingruber R.F.; Ho G.C.; Mason G.M.; Vines S.K.; Khotyaintsev Y.; Horbury T.; Maksimovic M.; Hadid L.Z.; Volwerk M.; Dimmock A.P.; Sorriso-Valvo L.; Stergiopoulou K.; Andrews G.B.; Angelini V.; Bale S.D.; Boden S.; Bottcher S.I.; Chust T.; Eldrum S.; Espada P.P.; Espinosa Lara F.; Evans V.; Gomez-Herrero R.; Hayes J.R.; Hellin A.M.; Kollhoff A.; Krasnoselskikh V.; Kretzschmar M.; Kuhl P.; Kulkarni S.R.; Lees W.J.; Lorfevre E.; Martin C.; O'brien H.; Plettemeier D.; Polo O.R.; Prieto M.; Ravanbakhsh A.; Sanchez-Prieto S.; Schlemm C.E.; Seifert H.; Soucek J.; Steller M.; Stverak S.; Terasa J.C.; Travnicek P.; Tyagi K.; Vaivads A.; Vecchio A.; Yedla M./titolo:Energetic ions in the Venusian system: Insights from the first Solar Orbiter flyby/doi:10.1051%2F0004-6361%2F202140803/rivista:Astronomy & astrophysics (Print)/anno:2021/pagina_da:A7-1/pagina_a:A7-11/intervallo_pagine:A7-1–A7-11/volume:656
Astronomy & Astrophysics, 656, 1-11
Astronomy & astrophysics
656 (2021): A7-1–A7-11. doi:10.1051/0004-6361/202140803
info:cnr-pdr/source/autori:Allen R.C.; Cernuda I.; Pacheco D.; Berger L.; Xu Z.G.; Freiherr Von Forstner J.L.; Rodriguez-Pacheco J.; Wimmer-Schweingruber R.F.; Ho G.C.; Mason G.M.; Vines S.K.; Khotyaintsev Y.; Horbury T.; Maksimovic M.; Hadid L.Z.; Volwerk M.; Dimmock A.P.; Sorriso-Valvo L.; Stergiopoulou K.; Andrews G.B.; Angelini V.; Bale S.D.; Boden S.; Bottcher S.I.; Chust T.; Eldrum S.; Espada P.P.; Espinosa Lara F.; Evans V.; Gomez-Herrero R.; Hayes J.R.; Hellin A.M.; Kollhoff A.; Krasnoselskikh V.; Kretzschmar M.; Kuhl P.; Kulkarni S.R.; Lees W.J.; Lorfevre E.; Martin C.; O'brien H.; Plettemeier D.; Polo O.R.; Prieto M.; Ravanbakhsh A.; Sanchez-Prieto S.; Schlemm C.E.; Seifert H.; Soucek J.; Steller M.; Stverak S.; Terasa J.C.; Travnicek P.; Tyagi K.; Vaivads A.; Vecchio A.; Yedla M./titolo:Energetic ions in the Venusian system: Insights from the first Solar Orbiter flyby/doi:10.1051%2F0004-6361%2F202140803/rivista:Astronomy & astrophysics (Print)/anno:2021/pagina_da:A7-1/pagina_a:A7-11/intervallo_pagine:A7-1–A7-11/volume:656
The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the sys
Autor:
G. M. Mason, G. C. Ho, R. C. Allen, J. Rodríguez-Pacheco, R. F. Wimmer-Schweingruber, R. Bučík, R. Gómez-Herrero, D. Lario, J. L. F. von Forstner, G. B. Andrews, L. Berger, I. Cernuda, F. Espinosa Lara, W. J. Lees, C. Martin, D. Pacheco, M. Prieto, S. Sánchez-Prieto, J. R. Hayes, C. E. Schlemm, H. Seifert, K. Tyagi
Publikováno v:
Astronomy & Astrophysics. 656:L1
We report observations of five impulsive solar energetic particle (SEP) events observed inside 1 au during the first perihelion pass of the Solar Orbiter mission, which was launched in February 2020. These small events were all reasonably associated
Autor:
J. Wm. Parker, R. A. Mewaldt, J. R. Spencer, Carey M. Lisse, Kelsi N. Singer, G. B. Andrews, Cathy Olkin, E. Bernardoni, H. Throop, L. E. Brown, Peter Kollmann, Andrew J. Steffl, Stamatios M. Krimigis, G. R. Gladstone, George Clark, K. S. Nelson, Mihaly Horanyi, Ralph L. McNutt, Harold A. Weaver, Fran Bagenal, H. A. Elliott, Michael E. Summers, G. Romeo, A. J. Verbiscer, N. Salazar, S. A. Stern, S. E. Jaskulek, R. A. Leske, Ivan Linscott, Matthew E. Hill, Robert Allen, M. B. Kusterer, Jon Vandegriff, R. B. Decker, John D. Richardson, Leslie A. Young
Publikováno v:
The Astrophysical Journal. 905:69
We augment the heliospheric network of galactic cosmic ray (GCR) monitors using 2012–2017 penetrating radiation measurements from the New Horizons (NH) Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI), obtaining intensities of