{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2022,3,31]],"date-time":"2022-03-31T03:35:08Z","timestamp":1648697708764},"reference-count":8,"publisher":"Cambridge University Press (CUP)","issue":"H15","license":[{"start":{"date-parts":[[2010,10,21]],"date-time":"2010-10-21T00:00:00Z","timestamp":1287619200000},"content-version":"unspecified","delay-in-days":354,"URL":"https:\/\/www.cambridge.org\/core\/terms"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Proc. IAU"],"published-print":{"date-parts":[[2009,11]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>High-resolution non-ideal magnetohydrodynamical simulations of the turbulent magnetized ISM, powered by supernovae types Ia and II at Galactic rate, including self-gravity and non-equilibriuim ionization (NEI), taking into account the time evolution of the ionization structure of H, He, C, N, O, Ne, Mg, Si, S and Fe, were carried out. These runs cover a wide range (from kpc to sub-parsec) of scales, providing resolution independent information on the injection scale, extended self-similarity and the fractal dmension of the most dissipative structures.<\/jats:p>","DOI":"10.1017\/s1743921310010318","type":"journal-article","created":{"date-parts":[[2010,10,21]],"date-time":"2010-10-21T09:52:51Z","timestamp":1287654771000},"page":"468-469","source":"Crossref","is-referenced-by-count":1,"title":["NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension"],"prefix":"10.1017","volume":"5","author":[{"given":"Miguel A.","family":"de Avillez","sequence":"first","affiliation":[]},{"given":"Dieter","family":"Breitschwerdt","sequence":"additional","affiliation":[]}],"member":"56","published-online":{"date-parts":[[2010,10,21]]},"reference":[{"key":"S1743921310010318_ref2","doi-asserted-by":"publisher","DOI":"10.1086\/521222"},{"key":"S1743921310010318_ref6","doi-asserted-by":"publisher","DOI":"10.1086\/152151"},{"key":"S1743921310010318_ref7","first-page":"301","volume":"30","author":"Kolmogorov","year":"1941","journal-title":"C.R. Acad. Sci. URSS"},{"key":"S1743921310010318_ref3","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevE.48.R29"},{"key":"S1743921310010318_ref1","first-page":"25","volume":"336","author":"Asplund","year":"2005","journal-title":"ASP Conf. Ser."},{"key":"S1743921310010318_ref4","doi-asserted-by":"publisher","DOI":"10.1086\/339403"},{"key":"S1743921310010318_ref5","first-page":"650","volume":"347","author":"Breitschwerdt","year":"1999","journal-title":"AandA"},{"key":"S1743921310010318_ref8","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.72.336"}],"container-title":["Proceedings of the International Astronomical Union"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.cambridge.org\/core\/services\/aop-cambridge-core\/content\/view\/S1743921310010318","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2019,4,30]],"date-time":"2019-04-30T10:29:18Z","timestamp":1556620158000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.cambridge.org\/core\/product\/identifier\/S1743921310010318\/type\/journal_article"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2009,11]]},"references-count":8,"journal-issue":{"issue":"H15","published-print":{"date-parts":[[2009,11]]}},"alternative-id":["S1743921310010318"],"URL":"https:\/\/doi.org\/10.1017\/s1743921310010318","relation":{},"ISSN":["1743-9213","1743-9221"],"issn-type":[{"value":"1743-9213","type":"print"},{"value":"1743-9221","type":"electronic"}],"subject":[],"published":{"date-parts":[[2009,11]]}}}