SwePub
Sök i LIBRIS databas

  Utökad sökning

WFRF:(Valentini F.)
 

Sökning: WFRF:(Valentini F.) > Three-dimensional m...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00006793naa a2200577 4500
001oai:DiVA.org:uu-522995
003SwePub
008240213s2023 | |||||||||||000 ||eng|
009oai:DiVA.org:kth-338495
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-5229952 URI
0247 a https://doi.org/10.1093/mnras/stad23842 DOI
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3384952 URI
040 a (SwePub)uud (SwePub)kth
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
1001 a Trotta, D.u Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England.,The Blackett Laboratory, Department of Physics, Imperial College London, London SW7 2AZ, UK4 aut
2451 0a Three-dimensional modelling of the shock-turbulence interaction
264 1b Oxford University Press,c 2023
338 a electronic2 rdacarrier
500 a QC 20231115
520 a The complex interaction between shocks and plasma turbulence is extremely important to address crucial features of energy conversion in a broad range of astrophysical systems. We study the interaction between a supercritical, perpendicular shock and pre-existing, fully developed plasma turbulence, employing a novel combination of magnetohydrodynamic and small-scale, hybrid-kinetic simulations where a shock is propagating through a turbulent medium. The variability of the shock front in the unperturbed case and for two levels of upstream fluctuations is addressed. We find that the behaviour of shock ripples, i.e. shock surface fluctuations with short (a few ion skin depths, di) wavelengths, is modified by the presence of pre-existing turbulence, which also induces strong corrugations of the shock front at larger scales. We link this complex behaviour of the shock front and the shock downstream structuring with the proton temperature anisotropies produced in the shock-turbulence system. Finally, we put our modelling effort in the context of spacecraft observations, elucidating the role of novel cross-scale, multispacecraft measurements in resolving shock front irregularities at different scales. These results are relevant for a broad range of astrophysical systems characterized by the presence of shock waves interacting with plasma turbulence.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng
653 a plasmas
653 a shock waves
653 a turbulence
7001 a Pezzi, O.u Istituto per la Scienza e Tecnologia dei Plasmi (ISTP), Consiglio Nazionale delle Ricerche, Via Amendola 122/D, I-70126 Bari, Italy4 aut
7001 a Burgess, D.u Queen Mary Univ London, Dept Phys & Astron, London E1 4NS, England.,Department of Physics and Astronomy, Queen Mary University of London, London, E1 4NS, UK4 aut
7001 a Preisser, L.u Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria.,Space Research Institute, Austrian Academy of Sciences, Graz, A-8042, Austria4 aut
7001 a Blanco-Cano, X.u Univ Nacl Autonoma Mexico, Inst Geofis, Dept Ciencias Espaciales, Ciudad Univ, Ciudad De Mexico 0451, Mexico.,Departamento de Ciencias Espaciales, Instituto de Geofísica, Universidad Nacional Aut onoma de México, Ciudad Universitaria, Ciudad de México, 0451, Mexico4 aut
7001 a Kajdic, P.u Univ Nacl Autonoma Mexico, Inst Geofis, Dept Ciencias Espaciales, Ciudad Univ, Ciudad De Mexico 0451, Mexico.,Departamento de Ciencias Espaciales, Instituto de Geofísica, Universidad Nacional Aut onoma de México, Ciudad Universitaria, Ciudad de México, 0451, Mexico4 aut
7001 a Hietala, H.u Queen Mary Univ London, Dept Phys & Astron, London E1 4NS, England.,Department of Physics and Astronomy, Queen Mary University of London, London, E1 4NS, UK4 aut
7001 a Horbury, T. S.u Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England.,The Blackett Laboratory, Department of Physics, Imperial College London, London SW7 2AZ, UK,Dipartimento di Fisica, Università della Calabria, I-87036 Rende, Italy,Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, Italy.4 aut
7001 a Vainio, R.u Univ Turku, Dept Phys & Astron, FI-20014 Turku, Finland.,Department of Physics and Astronomy, University of Turku, FI-20014 Turku, Finland4 aut
7001 a Dresing, N.u Univ Turku, Dept Phys & Astron, FI-20014 Turku, Finland.,Department of Physics and Astronomy, University of Turku, FI-20014 Turku, Finland4 aut
7001 a Retinò, A.u Univ Paris Sud, UPMC, CNRS, Ecole Polytech,LPP, F-91128 Palaiseau, France.,LPP, Ecole Polytechnique, CNRS, UPMC, Université Paris Sud, Palaiseau, F-91128, France4 aut
7001 a Marcucci, M. F.u INAF Ist Astrofis & Planetol Spaziali, I-00133 Rome, Italy.,INAF -Istituto di Astrofisica e Planetologia Spaziali, Rome, I-00133, Italy4 aut
7001 a Sorriso-Valvo, Lucau KTH,Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,CNR, Ist Sci & Tecnol Plasmi ISTP, Via Amendola 122-D, I-70126 Bari, Italy; KTH Royal Inst Technol, Sch Elect Engn & Comp Sci, Space & Plasma Phys, SE-10044 Stockholm, Sweden,Rymd- och plasmafysik,Istituto per la Scienza e Tecnologia dei Plasmi (ISTP), Consiglio Nazionale delle Ricerche, Via Amendola 122/D, I-70126 Bari, Italy; Swedish Institute of Space Physics (IRF), Ångström Laboratory, Läg erhyddsväg en 1, SE-75121 Uppsala, Sweden4 aut0 (Swepub:kth)u118wzcp
7001 a Servidio, S.u Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, Italy.4 aut
7001 a Valentini, F.u Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, Italy.,Dipartimento di Fisica, Università della Calabria, I-87036 Rende, Italy4 aut
7102 a Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England.b The Blackett Laboratory, Department of Physics, Imperial College London, London SW7 2AZ, UK4 org
7730 t Monthly notices of the Royal Astronomical Societyd : Oxford University Pressg 525:2, s. 1856-1866q 525:2<1856-1866x 0035-8711x 1365-2966
8564 u https://doi.org/10.1093/mnras/stad2384y Fulltext
8564 u https://uu.diva-portal.org/smash/get/diva2:1837326/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-522995
8564 8u https://doi.org/10.1093/mnras/stad2384
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-338495

Hitta via bibliotek

Till lärosätets databas

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Stäng

Kopiera och spara länken för att återkomma till aktuell vy