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Autor:
Abhishek Kumar, Franck Plunian, Rodion Stepanov, Andrei Teimurazov, Valerij Titov, Satyajit Barman, Mahendra K. Verma
Publikováno v:
2017 Ivannikov ISPRAS Open Conference (ISPRAS).
Magnetohydrodynamic (MHD) turbulence is an intrinsic part of astrophysical phenomena, which plays a crucial role is the generation of cosmic magnetic fields. The two-scale dynamo concept suggests that the small scale interactions are demanded to driv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::49b3aae29cda63133442dbf5b66fa83b
https://doi.org/10.1109/ispras.2017.00022
https://doi.org/10.1109/ispras.2017.00022
