يعرض 1 - 20 نتائج من 197 نتيجة بحث عن '"Laker, R"', وقت الاستعلام: 0.98s تنقيح النتائج
  1. 1
  2. 2
    Report
  3. 3
    Report
  4. 4
    Report
  5. 5
    Report
  6. 6
    Report
  7. 7
  8. 8
  9. 9
  10. 10
    Report
  11. 11
    Report
  12. 12
    Academic Journal

    وصف الملف: 147 - 147

    Relation: The Astrophysical Journal; @article{Trotta_2024, doi = {10.3847/1538-4357/ad187d}, url = {https://dx.doi.org/10.3847/1538-4357/ad187d}, year = {2024}, month = {feb}, publisher = {The American Astronomical Society}, volume = {962}, number = {2}, pages = {147}, author = {Domenico Trotta and Andrea Larosa and Georgios Nicolaou and Timothy S. Horbury and Lorenzo Matteini and Heli Hietala and Xochitl Blanco-Cano and Luca Franci and C. H. K Chen and Lingling Zhao and Gary P. Zank and Christina M. S. Cohen and Stuart D. Bale and Ronan Laker and Nais Fargette and Francesco Valentini and Yuri Khotyaintsev and Rungployphan Kieokaew and Nour Raouafi and Emma Davies and Rami Vainio and Nina Dresing and Emilia Kilpua and Tomas Karlsson and Christopher J. Owen and Robert F. Wimmer-Schweingruber}, title = {Properties of an Interplanetary Shock Observed at 0.07 and 0.7 au by Parker Solar Probe and Solar Orbiter}, journal = {The Astrophysical Journal}, abstract = {The Parker Solar Probe (PSP) and Solar Orbiter (SolO) missions opened a new observational window in the inner heliosphere, which is finally accessible to direct measurements. On 2022 September 5, a coronal mass ejection (CME)-driven interplanetary (IP) shock was observed as close as 0.07 au by PSP. The CME then reached SolO, which was radially well-aligned at 0.7 au, thus providing us with the opportunity to study the shock properties at different heliocentric distances. We characterize the shock, investigate its typical parameters, and compare its small-scale features at both locations. Using the PSP observations, we investigate how magnetic switchbacks and ion cyclotron waves are processed upon shock crossing. We find that switchbacks preserve their V–B correlation while compressed upon the shock passage, and that the signature of ion cyclotron waves disappears downstream of the shock. By contrast, the SolO observations reveal a very structured shock transition, with a population of shock-accelerated protons of up to about 2 MeV, showing irregularities in the shock downstream, which we correlate with solar wind structures propagating across the shock. At SolO, we also report the presence of low-energy (∼100 eV) electrons scattering due to upstream shocklets. This study elucidates how the local features of IP shocks and their environments can be very different as they propagate through the heliosphere.} }; https://qmro.qmul.ac.uk/xmlui/handle/123456789/96868

  13. 13
    Academic Journal
  14. 14
  15. 15
    Academic Journal

    المساهمون: Telloni, D, Adhikari, L, Zank, Gp, Hadid, Lz, Sanchez-Cano, B, Sorriso-Valvo, L, Zhao, Ll, Panasenco, O, Shi, C, Velli, M, Susino, R, Verscharen, D, Milillo, A, Alberti, T, Narita, Y, Verdini, A, Grimani, C, Bruno, R, D'Amicis, R, Perrone, D, Marino, R, Carbone, F, Califano, F, Malara, F, Stawarz, Je, Laker, R, Liberatore, A, Bale, Sd, Kasper, Jc, Heyner, D, de Wit, Td, Goetz, K, Harvey, Pr, Macdowall, Rj, Malaspina, Dm, Pulupa, M, Case, Aw, Korreck, Ke, Larson, D, Livi, R, Stevens, Ml, Whittlesey, P, Auster, Hu, Richter, I

    وصف الملف: STAMPA

    Relation: info:eu-repo/semantics/altIdentifier/wos/WOS:000869317700001; volume:938; issue:2; firstpage:1; lastpage:8; numberofpages:8; journal:THE ASTROPHYSICAL JOURNAL LETTERS; https://hdl.handle.net/11568/1172007; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85141745585; https://iopscience.iop.org/article/10.3847/2041-8213/ac9624/meta

  16. 16
  17. 17
    Academic Journal
  18. 18
    Academic Journal

    المساهمون: Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École polytechnique (X), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES), Centre National d'Études Spatiales Toulouse (CNES), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)

    المصدر: ISSN: 0004-6361.

    Relation: BIBCODE: 2021A&A.656A.39M

  19. 19
    Academic Journal

    المساهمون: Laboratoire de Mecanique des Fluides et d'Acoustique (LMFA), École Centrale de Lyon (ECL), Université de Lyon-Université de Lyon-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-École polytechnique (X), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)

    المصدر: ISSN: 0004-6361.

  20. 20
    Academic Journal