Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Dimitrios Millas"'
Autor:
Dimitrios Millas, Maria Elena Innocenti, Brecht Laperre, Joachim Raeder, Stefaan Poedts, Giovanni Lapenta
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 7 (2020)
Solar activity, ranging from the background solar wind to energetic coronal mass ejections (CMEs), is the main driver of the conditions in the interplanetary space and in the terrestrial space environment, known as space weather. A better understandi
Externí odkaz:
https://doaj.org/article/5c866f2a81424debb748438dc877f361
Publikováno v:
Galaxies, Vol 5, Iss 4, p 79 (2017)
Relativistic jets from active galactic nuclei (AGN) often display a non-uniform structure and are, under certain conditions, susceptible to a number of instabilities. An interesting example is the development of non-axisymmetric, Rayleigh-Taylor type
Externí odkaz:
https://doaj.org/article/d55d75728f934f619035f436c79d9adc
The Jovian magnetosphere can undergo significant changes in its size due to varying external (e.g. solar activity) or internal (e.g. hot plasma pressure) conditions. Simulations have shown that the difference in the dayside stand-off distance between
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af9c81075b8111c34f55eb12b53f953a
https://doi.org/10.5194/egusphere-egu23-15246
https://doi.org/10.5194/egusphere-egu23-15246
Autor:
Nicolas Wijsen, Alan Thomson, A. Kouloumvakos, Konstantin Herbst, Andrea Lani, Rami Vainio, Bernd Heber, Rui F. Pinto, Jens Pomoell, Alexandr Afanasiev, C. Verbeke, Blandine Gorce, Joachim Raeder, Aurélie Marchaudon, Andrey Kochanov, Ellen Clarke, Alexis Rouilard, Petra Vanlommel, Tinatin Baratashvili, P.-L. Blelly, Brecht Laperre, Maria Elena Innocenti, Angels Aran, Evangelia Samara, Luciano Rodriguez, Giovanni Lapenta, Jan Depauw, Stefaan Poedts, I. Plotnikov, Ronald Van der Linden, Emilia Kilpua, Emmanuel Chané, Blai Sanahuja, Dimitrios Millas, Ranadeep Sarkar, Josep M. Paredes, Camilla Scolini
Publikováno v:
Journal of Space Weather and Space Climate
Journal of Space Weather and Space Climate, 2020, 10, ⟨10.1051/swsc/2020055⟩
Journal of Space Weather and Space Climate, Vol 10, p 57 (2020)
Dipòsit Digital de la UB
Universidad de Barcelona
Journal of Space Weather and Space Climate, EDP sciences, 2020, 10, ⟨10.1051/swsc/2020055⟩
Journal of Space Weather and Space Climate, 2020, 10, ⟨10.1051/swsc/2020055⟩
Journal of Space Weather and Space Climate, Vol 10, p 57 (2020)
Dipòsit Digital de la UB
Universidad de Barcelona
Journal of Space Weather and Space Climate, EDP sciences, 2020, 10, ⟨10.1051/swsc/2020055⟩
Aims: This paper presents a H2020 project aimed at developing an advanced space weather forecasting tool, combining the MagnetoHydroDynamic (MHD) solar wind and coronal mass ejection (CME) evolution modelling with solar energetic particle (SEP) trans
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abe425668857efa1933339f939cbc4be
https://lirias.kuleuven.be/handle/123456789/662732
https://lirias.kuleuven.be/handle/123456789/662732
Publikováno v:
Proceedings of the International Astronomical Union. 14:257-259
Supernovae and astrophysical jets are two of the most energetic and intriguing objects in the universe. We examine an interesting scenario that involves the interaction of these two extreme phenomena, motivated by observations of the W50-SS433 system
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783030141271
Supernovae and astrophysical jets are two of the most energetic and intriguing objects in the universe. An interaction between these two extreme phenomena is believed to be present in the case of the W50-SS433 system: a jet launched from the microqua
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::90a074e1b6a1a2276bf0134f4806d6f3
https://doi.org/10.1007/978-3-030-14128-8_11
https://doi.org/10.1007/978-3-030-14128-8_11
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 470, pp.592. 〈10.1093/mnras/stx1288〉
Mon.Not.Roy.Astron.Soc., 2017, 470, pp.592. ⟨10.1093/mnras/stx1288⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470, pp.592. ⟨10.1093/mnras/stx1288⟩
Mon.Not.Roy.Astron.Soc., 2017, 470, pp.592. 〈10.1093/mnras/stx1288〉
Mon.Not.Roy.Astron.Soc., 2017, 470, pp.592. ⟨10.1093/mnras/stx1288⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470, pp.592. ⟨10.1093/mnras/stx1288⟩
Several observations of astrophysical jets show evidence of a structure in the direction perpendicular to the jet axis, leading to the development of "spine & sheath" models of jets. Most studies focus on a two-component jet consisting of a highly re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2fd42382225db1e6bb61abca0d3873aa
http://arxiv.org/abs/1706.06912
http://arxiv.org/abs/1706.06912
Publikováno v:
Galaxies; Volume 5; Issue 4; Pages: 79
Galaxies, Vol 5, Iss 4, p 79 (2017)
Galaxies, Vol 5, Iss 4, p 79 (2017)
© 2017 by the authors. Relativistic jets from active galactic nuclei (AGN) often display a non-uniform structure and are, under certain conditions, susceptible to a number of instabilities. An interesting example is the development of non-axisymmetr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f91386b0263fb116db2c6c634520d99f
https://lirias.kuleuven.be/handle/123456789/606110
https://lirias.kuleuven.be/handle/123456789/606110