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[null,"1.","Record Nr.",null,"UNIPARTHENOPE000011152"]
[null,null,"Autore",null,"Theel, Gustav Adolf"]
[null,null,"Titolo",null,"The world shipping scene : atlas of shipping, shipbuilding, seaports, and sea-borne trade / by Gustav Adolf Theel ; graphics under the direction of Dorothea Mattern-Authenrieth"]
[null,null,"Pubbl/distr/stampa",null,"Munich : Weststadt-Verlag, 1963"]
[null,null,"Descrizione fisica",null,"1 v. (pagin. varia) : ill. ; 30 cm"]
[null,null,"Disciplina",null,"387.5"]
[null,null,"Collocazione",null,"387.5/111"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,"2.","Record Nr.",null,"UNINA9910437979703321"]
[null,null,"Autore",null,"Balogh Andre"]
[null,null,"Titolo",null,"Physics of collisionless shocks : space plasma shock waves / / Andre Balogh, Rudolf A. Treumann"]
[null,null,"Pubbl/distr/stampa",null,"New York, : Springer, 2013"]
[null,null,"ISBN",null,"1-4614-6099-9"]
[{"$nulls":4},"1-283-94573-8"]
[null,null,"Edizione",null,"[1st ed. 2013.]"]
[null,null,"Descrizione fisica",null,"1 online resource (501 p.)"]
[null,null,"Collana",null,"ISSI scientific report series ; ; v. 12"]
[null,null,"Disciplina",null,"530.442"]
[null,null,"Soggetti",null,"Plasma waves"]
[{"$nulls":4},"Shock waves"]
[{"$nulls":4},"Space plasmas"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Note generali","Description based upon print version of record."]
[null,null,null,"Nota di bibliografia","Includes bibliographical references and index."]
[null,null,"Nota di contenuto",null,"pt. 1. Collisionless shock theory -- pt. 2. Applications : two kinds of collisionless shocks in the heliosphere."]
[null,null,null,"Sommario/riassunto","The present book provides a contemporary systematic treatment of shock waves in high-temperature collisionless plasmas as are encountered in near Earth space and in Astrophysics. It consists of two parts. Part I develops the complete theory of shocks in dilute hot plasmas under the assumption of absence of collisions among the charged particles when the interaction is mediated solely by the self-consistent electromagnetic fields. Such shocks are naturally magnetised implying that the magnetic field plays an important role in their evolution and dynamics. This part treats both subcritical shocks, which dissipate flow energy by generating anomalous resistance or viscosity, and supercritical shocks. The main emphasis is, however, on super-critical shocks where the anomalous dissipation is insufficient to retard the upstream flow. These shocks, depending on the direction of the upstream magnetic field, are distinguished as quasi-perpendicular and quasi-parallel shocks which exhibit different behaviours, reflecting particles back upstream and generating high electromagnetic wave intensities. Particle acceleration and turbulence at such shocks become possible and important. Part II treats planetary bow shocks and the famous Heliospheric Termination shock as examples of two applications of the theory developed in Part I."]