KNOWN: Simple expression to account for the effect of pressure on the nucleate boiling convection coefficient in water.
FIND: Compare predictions of this expression with the Rohsenow correlation for specified Δ \mathrm T_{\mathrm e} and pressures (2 and 5 bar) applied to a horizontal plate.
ASSUMPTIONS: (1) Steady-state conditions, (2) Nucleate pool boiling, (3) \mathrm C_{\mathrm{s,f}} = 0.013, n = 1.
PROPERTIES: Table A-6, Saturated water (2 bar): \rho_{\ell} = 942.7 kg/m³, \mathrm c_{\mathrm p,\ell} = 4244.3 J/kg·K, \mu_{\ell} = 230.7 × 10^{-6} N·s/m², \mathrm{Pr}_{\ell} = 1.43, \mathrm h_{\mathrm{fg}} = 2203 kJ/kg, σ = 54.97 × 10^{-3} N/m, \rho_{\mathrm v} = 1.1082 kg/m³; Saturated water (5 bar): \rho_{\ell} = 914.7 kg/m³, \mathrm c_{\mathrm p,\ell} = 4316 J/kg·K, \mu_{\ell} = 179 × 10^{-6} N·s/m², \mathrm{Pr}_{\ell} = 1.13, \mathrm h_{\mathrm{fg}} = 2107.8 kJ/kg, σ = 48.4 × 10^{-3} N/m, \rho_{\mathrm v} = 2.629 kg/m³.
ANALYSIS: The simple expression by Jakob [51] accounting for pressure effects is
h = C \left(\Delta T _{ e }\right)^{ n }\left( p / p _{ a }\right)^{0.4} (1)
where \mathrm p~\text{and}~\mathrm p_{\mathrm a} are the system and standard atmospheric pressures. For a horizontal plate, C = 5.56 and n = 3 for the range 15 < \mathrm q_{\mathrm s}^{\prime\prime} < 235 kW/m². For Δ \mathrm T_{\mathrm e} = 10°C,
p = 2 bar h =5.56(10)^3(2 bar / 1.0133 bar )^{0.4}=7,298 W / m ^2 \cdot K , \quad q _{ s }^{\prime \prime}=73 kW / m ^2
p = 5 bar h =5.56(10)^3(5 bar / 1.0133 bar )^{0.4}=10,529 W / m ^2 \cdot K , \quad q _{ s }^{\prime \prime}=105 kW / m ^2
where \mathrm q_{\mathrm s}^{\prime\prime} = \mathrm h\Delta\mathrm T_{\mathrm e}. The Rohsenow correlation, Eq. 10.5, with \mathrm C_{\mathrm{s,f}} = 0.013 and n = 1, is of the form
q _{ s }^{\prime \prime}=\mu_{\ell} h _{ fg }\left[\frac{ g \left(\rho_{\ell}~-~\rho_{ v }\right)}{\sigma}\right]^{1 / 2}\left[\frac{ c _{ p , \ell} \Delta T _{ e }}{ C _{ s , f } h _{ fg } \operatorname{Pr}_{\ell}^{ n }}\right]^3. (2)
p = 2 bar: q _{ s }^{\prime \prime}=230.7 \times 10^{-6} \frac{ N \cdot s }{ m ^2} \times 2203 \times 10^3 \frac{ J }{ kg }\left[\frac{9.8 \frac{ m }{ s ^2}(942.7 ~- ~1.1082) \frac{ kg }{ m ^3}}{54.97~ \times ~10^{-3} N / m }\right]^{1 / 2} \times\left[\frac{4244.3 J / kg \cdot K~ \times~ 10 K }{0.013 ~\times~ 2203 ~\times~ 10^3 \frac{ J }{ kg }~ \times ~1.43^1}\right]^3
q _{ s }^{\prime \prime}=232 kW / m ^2
p = 4 bar: q _{ s }^{\prime \prime}=439 kW / m ^2.
COMMENTS: For ease of comparison, the results with \mathrm p_{\mathrm a} = 1.0133 bar are:
Note that the range of \mathrm q_{\mathrm s}^{\prime\prime} is within the limits of the Simple correlation. The comparison is poor and therefore the correlation is not to be recommended. By manipulation of the Rohsenow results, find that the (\mathrm p/\mathrm p_{\mathrm o})^{\mathrm m} dependence provides m ≈ 0.75, compared to the exponent of 0.4 in the Simple correlation.
\mathrm q_{\mathrm s}^{\prime\prime} (kW/m²) | |||
Correlation/p (bar) | 1 | 2 | 4 |
Simple | 56 | 73 | 105 |
Rohsenow | 135 | 232 | 439 |