Studying Interstellar Turbulence Driving Scales using the Bispectrum
Studying Interstellar Turbulence Driving Scales using the Bispectrum
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We demonstrate the utility of the bispectrum, the Fourier three-point correlation function, for studying driving scales of magnetohydrodynamic (MHD) turbulence in the interstellar medium. We calculate the bispectrum by implementing a parallelized Monte Carlo direct measurement method, which we have made publicly available. In previous works, the bi...
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Studying Interstellar Turbulence Driving Scales using the Bispectrum
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TN_cdi_proquest_journals_2644202103
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2644202103
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2203.13334
