RUSSIAN JOURNAL OF EARTH SCIENCES, VOL. 16, ES6006, doi:10.2205/2016ES000589, 2016
$H_{\mathrm{low}} = 1.5$ $\mu$W/m$^3$ | $H_{\mathrm{norm}} = 2.0$ $\mu$W/m$^3$ | $H_{\mathrm{high}} = 2.5$ $\mu$W/m$^3$ | ||||
$La_{\mathrm{low}} = 2.0$ W/m K | 685/730 | 780/840 | 715/755 | 840/890 | 750/885 | 885/920 |
$La_{\mathrm{norm}} = 2.5$ W/m K | 630/700 | 700/770 | 665/720 | 745/810 | 700/740 | 780/840 |
$La_{\mathrm{high}} = 3.0$ W/m K | 590/670 | 615/705 | 620/690 | 670/750 | 650/710 | 710/780 |
Citation: Parphenuk O. I. (2016), Thermal regime and heat transfer during the evolution of continental collision structures, Russ. J. Earth Sci., 16, ES6006, doi:10.2205/2016ES000589.
Copyright 2016 by the Geophysical Center RAS.