المؤلفون: C. Moissard, P. Savoini, D. Fontaine, R. Modolo

المصدر: Frontiers in Astronomy and Space Sciences, Vol 11 (2024)

مصطلحات موضوعية: interplanetary shock, magnetosheath, interplanetary sheath, magnetic cloud, hybrid PIC, global simulation, Astronomy, QB1-991, Geophysics. Cosmic physics, QC801-809

وصف الملف: electronic resource

العلاقة: https://www.frontiersin.org/articles/10.3389/fspas.2024.1330397/fullTest; https://doaj.org/toc/2296-987XTest

الوصول الحر: https://doaj.org/article/1f5e049acd224b97a263020a47235b65Test

المؤلفون: Moissard, C., Savoini, P., Fontaine, D., Modolo, Ronan

المساهمون: Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), York Plasma Institute (YPI), University of York York, UK, HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)

المصدر: ISSN: 2296-987X ; Frontiers in Astronomy and Space Sciences ; https://hal.science/hal-04442445Test ; Frontiers in Astronomy and Space Sciences, 2024, 11, pp.1330397. ⟨10.3389/fspas.2024.1330397⟩.

مصطلحات موضوعية: interplanetary shock, magnetosheath, interplanetary sheath, magnetic cloud, hybrid PIC, global simulation, [SDU]Sciences of the Universe [physics], [PHYS]Physics [physics]

العلاقة: hal-04442445; https://hal.science/hal-04442445Test; https://hal.science/hal-04442445/documentTest; https://hal.science/hal-04442445/file/fspas-11-1330397.pdfTest

الإتاحة: https://doi.org/10.3389/fspas.2024.1330397Test
https://hal.science/hal-04442445Test
https://hal.science/hal-04442445/documentTest
https://hal.science/hal-04442445/file/fspas-11-1330397.pdfTest

المؤلفون: Petukhova A. S., Petuhov I. S., Petukhov S. I., Gotovtsev I. S.

المصدر: Solar-Terrestrial Physics, Vol 9, Iss 2, Pp 94-100 (2023)

مصطلحات موضوعية: cosmic rays, coronal mass ejection, forbush decrease, solar wind, interplanetary magnetic field, shock, magnetic cloud, Astrophysics, QB460-466

وصف الملف: electronic resource

العلاقة: https://naukaru.ru/en/nauka/article/57385/viewTest; https://doaj.org/toc/2500-0535Test

الوصول الحر: https://doaj.org/article/a9981d17877f43a690a6cc949115bf0cTest

المؤلفون: Ulrich, Roger K, Riley, Pete, Tran, T

المصدر: Space weather : the international journal of research & applications. 16(11)

مصطلحات موضوعية: magnetic cloud chirality, magnetic cloud sources, solar surface sources of CMEs, southward field prediction, astro-ph.SR, Astronomical and Space Sciences

وصف الملف: application/pdf

الوصول الحر: https://escholarship.org/uc/item/4m64d1w8Test

المؤلفون: Gololobov, Petr Yu., Grigoryev, Vladislav G., Gerasimova, Sardaana K., Starodubtsev, Sergey A., Zverev, Anton S.

مصطلحات موضوعية: article, Chapter, ddc:530, ddc:600, cosmic rays, neutron monitor, anisotropy, magnetic cloud, coronal mass ejection

العلاقة: NMDB@Athens -- urn:nbn:de:gbv:8:3-2023-00486-0 -- 978-3-928794-99-2 -- 10.38072/2748-3150/v2 -- info:eu-repo/grantAgreement/EC/FP7/213007/EU/Real-Time database for high resolution Neutron Monitor measurements/NMDB; https://doi.org/10.38072/2748-3150/p29Test; https://nbn-resolving.org/urn:nbn:de:gbv:8:3-2023-00506-4Test; https://macau.uni-kiel.de/receive/macau_mods_00003828Test; https://macau.uni-kiel.de/servlets/MCRFileNodeServlet/macau_derivate_00005421/kiel-up_2748-3150_p29.pdfTest

الإتاحة: https://doi.org/10.38072/2748-3150/p2910.38072/2748-3150/v2Test
https://nbn-resolving.org/urn:nbn:de:gbv:8:3-2023-00506-4Test
https://macau.uni-kiel.de/receive/macau_mods_00003828Test
https://macau.uni-kiel.de/servlets/MCRFileNodeServlet/macau_derivate_00005421/kiel-up_2748-3150_p29.pdfTest

المؤلفون: Ala-Lahti, Matti, Pulkkinen, Tuija I., Ruohotie, Julia, Akhavan-Tafti, Mojtaba, Good, Simon W., Kilpua, Emilia K. J.

المساهمون: Department of Physics, Space Physics Research Group, Particle Physics and Astrophysics

مصطلحات موضوعية: Coronal mass ejection, Reconnection exhaust structure, Magnetic cloud erosion, Solar-wind, Current sheets, Guide-field, Magnetospheric storms, Dayside magnetopause, Radial evolution, In-situ, 115 Astronomy, Space science

وصف الملف: application/pdf

العلاقة: Ala-Lahti , M , Pulkkinen , T I , Ruohotie , J , Akhavan-Tafti , M , Good , S W & Kilpua , E K J 2023 , ' Multipoint Observations of the Dynamics at an ICME Sheath-Ejecta Boundary ' , Astrophysical Journal , vol. 956 , no. 2 , 131 . https://doi.org/10.3847/1538-4357/acf99eTest; ORCID: /0000-0002-4489-8073/work/146908974; ORCID: /0000-0002-2999-5457/work/146909745; ORCID: /0000-0002-4921-4208/work/146910530; ORCID: /0000-0001-9574-339X/work/146910566; 85175619470; 2d7aa690-c698-4651-8fc5-83fe32f4c4a2; http://hdl.handle.net/10138/567099Test; 001086905600001

الإتاحة: http://hdl.handle.net/10138/567099Test

المؤلفون: Sanchita Pal, Benjamin J. Lynch, Simon W. Good, Erika Palmerio, Eleanna Asvestari, Jens Pomoell, Michael L. Stevens, Emilia K. J. Kilpua

المصدر: Frontiers in Astronomy and Space Sciences, Vol 9 (2022)

مصطلحات موضوعية: coronal mass ejection (CME), heliosphere, reconnection, interplanetary magnetic field, interplanetary magnetic cloud, Astronomy, QB1-991, Geophysics. Cosmic physics, QC801-809

وصف الملف: electronic resource

العلاقة: https://www.frontiersin.org/articles/10.3389/fspas.2022.903676/fullTest; https://doaj.org/toc/2296-987XTest

الوصول الحر: https://doaj.org/article/c703344f5258489fada38c05c543e89fTest

المؤلفون: Zhao, L-L, Zank, G. P., He, J. S., Telloni, D., Hu, Q., Li, G., Nakanotani, M., Adhikari, L., Kilpua, E. K. J., Horbury, T. S., O'Brien, H., Evans, Bradley, Angelini, Corrado

المساهمون: Department of Physics, Space Physics Research Group, Doctoral Programme in Particle Physics and Universe Sciences

مصطلحات موضوعية: shock waves, turbulence, waves, Sun, coronal mass ejections (CMEs), ION-CYCLOTRON WAVES, MAGNETIC CLOUD, ALFVEN WAVES, ACCELERATION, EVOLUTION, HELICITY, 114 Physical sciences, 115 Astronomy, Space science

وصف الملف: application/pdf

العلاقة: We acknowledge the partial support of the NSF EPSCoR RII-Track-1 Cooperative Agreement OIA-1655280 and a NASA award 80NSSC20K1783. D.T. is partially supported by the Italian Space Agency (ASI) under contract I/013/12/0. The Solar Orbiter magnetometer was funded by the UK Space Agency (grant ST/T001062/1).; Zhao , L-L , Zank , G P , He , J S , Telloni , D , Hu , Q , Li , G , Nakanotani , M , Adhikari , L , Kilpua , E K J , Horbury , T S , O'Brien , H , Evans , B & Angelini , C 2021 , ' Turbulence and wave transmission at an ICME-driven shock observed by the Solar Orbiter and Wind ' , Astronomy & Astrophysics , vol. 656 , 3 . https://doi.org/10.1051/0004-6361/202140450Test; ORCID: /0000-0002-4489-8073/work/106341640; c4b09e8d-3424-47e4-ae80-724527c1c7dc; http://hdl.handle.net/10138/338538Test; 000730246400004

الإتاحة: http://hdl.handle.net/10138/338538Test

المؤلفون: Pal, Sanchita

المساهمون: Space Physics Research Group, Particle Physics and Astrophysics, Department of Physics

مصطلحات موضوعية: 114 Physical sciences, Coronal mass ejection, Magnetic reconnection, Interplanetary magnetic field, Flux rope, Magnetic cloud

وصف الملف: application/pdf

العلاقة: This work is partially supported by the Center of Excellence in Space Sciences India (CESSI) that is funded by the Ministry of Human Resource Development, Government of India under the Frontier Areas of Science and Technology scheme. The author is grateful to Dr. Katsuhide Marubashi for making available the linear force free cylindrical flux rope model. The author is thankful to Prof. Dibyendu Nandy for his help in improving the quality of this work. The author thanks the referees for their helpful comments and suggestions that improve the manuscript. The author acknowledges the use of data from the SDO, SOHO, STEREO and ACE instruments. The authors declare the following financial interests/personal relationships which may be considered as potential competing interests: [The author Dr. Sanchita Pal, hereby declares that part of this work is partially supported by the Center of Excellence in Space Sciences India (CESSI) that is funded by the Ministry of Human Resource Development, Government of India under the Frontier Areas of Science and Technology scheme.]; Pal , S 2022 , ' Uncovering the process that transports magnetic helicity to coronal mass ejection flux ropes ' , Advances in Space Research , vol. 70 , no. 6 , pp. 1601-1613 . https://doi.org/10.1016/j.asr.2021.11.013Test; 85123883483; 896d242a-dc25-4063-9225-751e511a4a93; http://hdl.handle.net/10138/347629Test; 000838599300007

الإتاحة: https://doi.org/10.1016/j.asr.2021.11.013Test
http://hdl.handle.net/10138/347629Test

المؤلفون: Alexander A. Khokhlachev, Yuri I. Yermolaev, Irina G. Lodkina, Maria O. Riazantseva, Liudmila S. Rakhmanova

المصدر: Universe; Volume 8; Issue 11; Pages: 557

مصطلحات موضوعية: solar wind, interplanetary coronal mass ejection, magnetic cloud, helium abundance

وصف الملف: application/pdf

العلاقة: Solar System; https://dx.doi.org/10.3390/universe8110557Test

الإتاحة: https://doi.org/10.3390/universe8110557Test