Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Konrad Steinvall"'
On 28th of August 2018 at 5:30 UT, MMS and Cluster were located in the magnetotail at about 16 earth radii (RE). They both suddenly crossed plasma interfaces. Located near the post midnight sector, Cluster transitioned from a cold plasma sheet to a h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e06a735d54534cc749a86c098a4b3a41
https://doi.org/10.5194/egusphere-egu23-12580
https://doi.org/10.5194/egusphere-egu23-12580
Autor:
Eva Krämer, Maria Hamrin, Herbert Gunell, Tomas Karlsson, Konrad Steinvall, Oleksandr Goncharov, Mats André
The magnetosheath is a region downstream of the bow shock filled with turbulent, decelerated solar wind plasma which is flowing earthwards. This solar wind flow sometimes shows signatures of localized structures with enhanced dynamic pressure, so cal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfd794057c7ced6b2f912730bf8cf072
https://doi.org/10.5194/egusphere-egu23-550
https://doi.org/10.5194/egusphere-egu23-550
Broadband waves near and below the lower-hybrid frequency have been observed at the magnetopause for a long time. In recent years NASA's multi-spacecraft mission Magnetospheric Multiscale (MMS) has enabled the waves to be analysed in much greater det
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::69c447759a40af6d8189f2adac6564fd
https://doi.org/10.5194/egusphere-egu22-4134
https://doi.org/10.5194/egusphere-egu22-4134
High frequency electrostatic oscillations are one of the most fundamental players in energy conversion in collisionless plasmas. Whether at collisionless shocks, turbulence energy cascades or reconnection, small scale Debye length processes are at th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1af35c5b279425c44528b5310c9a0f74
https://doi.org/10.5194/egusphere-egu22-5068
https://doi.org/10.5194/egusphere-egu22-5068
Autor:
Erika Palmerio, Christina O. Lee, M. Leila Mays, Janet G. Luhmann, David Lario, Beatriz Sánchez‐Cano, Ian G. Richardson, Rami Vainio, Michael L. Stevens, Christina M. S. Cohen, Konrad Steinvall, Christian Möstl, Andreas J. Weiss, Teresa Nieves‐Chinchilla, Yan Li, Davin E. Larson, Daniel Heyner, Stuart D. Bale, Antoinette B. Galvin, Mats Holmström, Yuri V. Khotyaintsev, Milan Maksimovic, Igor G. Mitrofanov
Predictions of coronal mass ejections (CMEs) and solar energetic particles (SEPs) are a central issue in space weather forecasting. In recent years, interest in space weather predictions has expanded to include impacts at other planets beyond Earth a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cc3cfb96bed5ef4889ff568d6d3131c
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-474450
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-474450
When analyzing plasma waves, a key parameter to determine is the phase velocity. It enables us to, for example, compute wavelengths, wave potentials, and determine the energy of resonant particles. The phase velocity of a wave, observed by a single s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a80c68c9000502916b0bfb9722eef1df
http://arxiv.org/abs/2111.10288
http://arxiv.org/abs/2111.10288
Autor:
Stuart D. Bale, Robert J. Strangeway, Yuri V. Khotyaintsev, R. Wang, Christopher T. Russell, F. S. Mozer, I. V. Kuzichev, A. V. Artemyev, Ivan Y. Vasko, Konrad Steinvall, Robert E. Ergun, Barbara L. Giles, P. A. Lindqvist
Publikováno v:
Journal of Geophysical Research: Space Physics. 126
We present a statistical analysis of more than two thousand bipolar electrostatic solitary waves (ESW) collected from ten quasi-perpendicular Earth's bow shock crossings by Magnetospheric Multiscale spacecraft. We developed and implemented a correcti
Autor:
Stuart D. Bale, Michael L. Stevens, Phyllis Whittlesey, Peter R. Harvey, Christopher J. Owen, Philippe Louarn, Stefano Livi, Francesco Carbone, Ester Antonucci, Rossana De Marco, L. D. Woodham, Helen O'Brien, V. Angelini, Marco Romoli, Lingling Zhao, Marc Pulupa, Robert J. MacDowall, Thierry Dudok de Wit, Anthony W. Case, Olga Panasenco, Davin Larson, Vincent Evans, Chen Shi, Laxman Adhikari, R. Laker, Luca Sorriso-Valvo, Raffaella D'Amicis, Roberto Livi, Daniele Telloni, Denise Perrone, Anna Tenerani, Konrad Steinvall, David M. Malaspina, Masaru Nakanotani, Vamsee Krishna Jagarlamudi, Keith Goetz, Kelly E. Korreck, Justin C. Kasper, Marco Velli, Roberto Bruno, Haoming Liang, Timothy S. Horbury, Raffaele Marino, Gary P. Zank
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2021, 912 (2), pp.L21. ⟨10.3847/2041-8213/abf7d1⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2021, 912 (2), pp.L21. ⟨10.3847/2041-8213/ABF7D1⟩
The astrophysical journal. Letters
912 (2021): L21-1–L21-8. doi:10.3847/2041-8213/abf7d1
info:cnr-pdr/source/autori:Telloni, Daniele; Sorriso-Valvo, Luca; Woodham, Lloyd D.; Panasenco, Olga; Velli, Marco; Carbone, Francesco; Zank, Gary P.; Bruno, Roberto; Perrone, Denise; Nakanotani, Masaru; Shi, Chen; D'Amicis, Raffaella; De Marco, Rossana; Jagarlamudi, Vamsee K.; Steinvall, Konrad; Marino, Raffaele; Adhikari, Laxman; Zhao, Lingling; Liang, Haoming; Tenerani, Anna; Laker, Ronan; Horbury, Timothy S.; Bale, Stuart D.; Pulupa, Marc; Malaspina, David M.; Macdowall, Robert J.; Goetz, Keith; De Wit, Thierry Dudok; Harvey, Peter R.; Kasper, Justin C.; Korreck, Kelly E.; Larson, Davin; Case, Anthony W.; Stevens, Michael L.; Whittlesey, Phyllis; Livi, Roberto; Owen, Christopher J.; Livi, Stefano; Louarn, Philippe; Antonucci, Ester; Romoli, Marco; O'Brien, Helen; Evans, Vincent; Angelini, Virginia/titolo:Evolution of Solar Wind Turbulence from 0.1 to 1 au during the First Parker Solar Probe-Solar Orbiter Radial Alignment/doi:10.3847%2F2041-8213%2Fabf7d1/rivista:The astrophysical journal. Letters (Print)/anno:2021/pagina_da:L21-1/pagina_a:L21-8/intervallo_pagine:L21-1–L21-8/volume:912
The Astrophysical journal letters, Bristol : IOP Publishing, 2021, 912 (2), ⟨10.3847/2041-8213/abf7d1⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2021, 912 (2), pp.L21. ⟨10.3847/2041-8213/abf7d1⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2021, 912 (2), pp.L21. ⟨10.3847/2041-8213/ABF7D1⟩
The astrophysical journal. Letters
912 (2021): L21-1–L21-8. doi:10.3847/2041-8213/abf7d1
info:cnr-pdr/source/autori:Telloni, Daniele; Sorriso-Valvo, Luca; Woodham, Lloyd D.; Panasenco, Olga; Velli, Marco; Carbone, Francesco; Zank, Gary P.; Bruno, Roberto; Perrone, Denise; Nakanotani, Masaru; Shi, Chen; D'Amicis, Raffaella; De Marco, Rossana; Jagarlamudi, Vamsee K.; Steinvall, Konrad; Marino, Raffaele; Adhikari, Laxman; Zhao, Lingling; Liang, Haoming; Tenerani, Anna; Laker, Ronan; Horbury, Timothy S.; Bale, Stuart D.; Pulupa, Marc; Malaspina, David M.; Macdowall, Robert J.; Goetz, Keith; De Wit, Thierry Dudok; Harvey, Peter R.; Kasper, Justin C.; Korreck, Kelly E.; Larson, Davin; Case, Anthony W.; Stevens, Michael L.; Whittlesey, Phyllis; Livi, Roberto; Owen, Christopher J.; Livi, Stefano; Louarn, Philippe; Antonucci, Ester; Romoli, Marco; O'Brien, Helen; Evans, Vincent; Angelini, Virginia/titolo:Evolution of Solar Wind Turbulence from 0.1 to 1 au during the First Parker Solar Probe-Solar Orbiter Radial Alignment/doi:10.3847%2F2041-8213%2Fabf7d1/rivista:The astrophysical journal. Letters (Print)/anno:2021/pagina_da:L21-1/pagina_a:L21-8/intervallo_pagine:L21-1–L21-8/volume:912
The Astrophysical journal letters, Bristol : IOP Publishing, 2021, 912 (2), ⟨10.3847/2041-8213/abf7d1⟩
The first radial alignment between Parker Solar Probe and Solar Orbiter spacecraft is used to investigate the evolution of solar wind turbulence in the inner heliosphere. Assuming ballistic propagation, two 1.5 hr intervals are tentatively identified
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1eeeb85da3ee404fe49367dfb5c1d557
http://hdl.handle.net/10044/1/89346
http://hdl.handle.net/10044/1/89346
Autor:
Daniel B. Graham, Andris Vaivads, Yuri V. Khotyaintsev, Christopher T. Russell, Mats André, Konrad Steinvall
Publikováno v:
Geophysical Research Letters. 48
We report Magnetospheric Multiscale observations of large amplitude, parallel, electrostatic, proton plasma frequency waves on the magnetospheric side of the reconnecting magnetopause. The waves ar...
Autor:
Yuri V. Khotyaintsev, Christopher J. Owen, Andris Vaivads, Philippe Louarn, Giulia Cozzani, A. Fedorov, Konrad Steinvall
Solar wind current sheets have been extensively studied at 1 AU. The recent advent of Parker Solar Probe and Solar Orbiter (SolO) has enabled us to study these structures at a range of heliocentric distances.We present SolO observations of current sh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c06ebeffa8d4febfb2ad4035f2019526
https://doi.org/10.5194/egusphere-egu21-10630
https://doi.org/10.5194/egusphere-egu21-10630