2011
DOI: 10.2514/1.c031426
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Air Traffic Control Service Quality Perceptions of Domestic Airline Pilots in Turkey

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Cited by 6 publications
(5 citation statements)
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“…As the number of water molecules increases, the intermolecular hydrogen bonding increases, causing larger exothermic enthalpy values (DH B ), as seen in Fig. 5 73 The binding Gibbs free energies (DG B ) of the most stable binary F(W) n and ternary F(A)(W) nÀ1 (n = 1-8, 10, 12, 14, 16, 18, 20) clusters are calculated using the M06-2X/6-311++G(2d,2p) level of theory at atmospherically relevant temperatures (T) and pressures (P) (from T = 298.15 K, P = 1013.25 hPa to T = 216.65 K, P = 226.32 hPa). Eqn ( 12) and ( 13) were used to calculate the binding free energies of F(W) n and F(A)(W) nÀ1 (n = 1-8, 10, 12, 14, 16, 18, 20) clusters and the successive binding free energies (DG n ) of the F(W) n (n = 1-8) cluster respectively.…”
Section: Thermochemical Analysismentioning
confidence: 94%
“…As the number of water molecules increases, the intermolecular hydrogen bonding increases, causing larger exothermic enthalpy values (DH B ), as seen in Fig. 5 73 The binding Gibbs free energies (DG B ) of the most stable binary F(W) n and ternary F(A)(W) nÀ1 (n = 1-8, 10, 12, 14, 16, 18, 20) clusters are calculated using the M06-2X/6-311++G(2d,2p) level of theory at atmospherically relevant temperatures (T) and pressures (P) (from T = 298.15 K, P = 1013.25 hPa to T = 216.65 K, P = 226.32 hPa). Eqn ( 12) and ( 13) were used to calculate the binding free energies of F(W) n and F(A)(W) nÀ1 (n = 1-8, 10, 12, 14, 16, 18, 20) clusters and the successive binding free energies (DG n ) of the F(W) n (n = 1-8) cluster respectively.…”
Section: Thermochemical Analysismentioning
confidence: 94%
“…Wind power density (WPD) is commonly used to quantify the potential wind energy resources, and is expressed as (Manwell et al., 2010): WPD=12ρV3 $WPD=\frac{1}{2}\rho {V}^{3}$ where ρ and V are the air density (kg·m −3 ) and wind speed (m·s −1 ) at the turbine hub height, respectively, which typically ranges from 50 to 100 m. In this study, we use the wind speed at 100 m to calculate WPD, and the wind speed at 100 m is obtained from the 10 m wind speed using the power law (Cavcar, 2000; Peterson & Hennessey, 1978): VVr=ZZr17 $\frac{V}{{V}_{r}}={\left(\frac{Z}{{Z}_{r}}\right)}^{\tfrac{1}{7}}$ where V is the wind speed (m·s −1 ) at height z (m), and V r is the known wind speed at a reference height Z r (m; here refers to 10 m). Moreover, considering that ρ is a function of height Z and temperature, we estimated it following dos Santos Custódio (2009) and Sawadogo, Reboita, et al.…”
Section: Methodsmentioning
confidence: 99%
“…where ρ and V are the air density (kg•m 3 ) and wind speed (m•s 1 ) at the turbine hub height, respectively, which typically ranges from 50 to 100 m. In this study, we use the wind speed at 100 m to calculate WPD, and the wind speed at 100 m is obtained from the 10 m wind speed using the power law (Cavcar, 2000;Peterson & Hennessey, 1978):…”
Section: Wind Energy Densitymentioning
confidence: 99%
“…Maximum wave angle βmax in the limit of regular reflection as a function of preshock Mach number M1 for an air mixture (78% N2, 21% O2, and 1% Ar) in the atmosphere at different flight altitudes (0, 15, and 30 km) above sea level in the ISA model (see panel b); solid line: calorically imperfect gas with dissociation/ionization; dashed: calorically imperfect gas with frozen chemistry; dotted: calorically perfect gas. Figure 2.9 represents the maximum incidence angle β 3,max for regular shock reflections as a function of the pre-shock Mach number M 1 for three atmospheric conditions corresponding to increasing flight altitudes in the ISA model [178] [see panel (b)]. Results are presented for the three gas models defined above i), ii), and iii).…”
Section: Figure 29mentioning
confidence: 99%