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Figure 5
Prolonged simulation of the maximal temperature growth for the 1 µm-thick slab of Si3N4 support for different parameters of heat convection and thermal radiation emissivity ∊. The solid line denotes the ambient conditions with surface emissivity coefficients, ∊SiN = 0.2, ∊PMMA = 0.9, the dot–dashed line denotes conditions with emissivity ∊SiN = 0.02, ∊PMMA = 0.09 and heat conductivity h1 = [0.21 \times \left({T - T_\infty } \right)^{5/4}] J m−2 s−1; the dashed line with diamond marks denotes conditions with heat conductivity h2 = [0.021 \times \left({T - T_\infty } \right)^{5/4}] J m−2 s−1 and ∊ = 0.002.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 18| Part 4| July 2011| Pages 580-594
https://doi.org/10.1107/S0909049511016335
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