Sentence examples for on wavelength for from inspiring English sources

Measurements were performed on a spectrophotometer UV-5800 PC. Figure 8 shows dependences of the absorption coefficient on wavelength for samples 3 and 6.

Open image in new window Fig. 5 Dependence of extinction coefficient (k) on wavelength for samples 2 and 3 Open image in new window Fig. 6 Dependence of absorption coefficient on wavelength for samples 2 and 3 Open image in new window Fig. 7 Plot of (αhν 2 versus photon energy (hν) for annealed Cu2O films.

(a) Dependence of the coupling lengths on wavelength for different separations and (b) electric field |E| transfer process in two AHPMW waveguides for wavelengths of 1.45 and 1.65 μm.

Fluorescence and potentiometric measurements showed the change in response behavior depending on wavelength of the light used for illumination.

A band-pass filter with a wavelength range of 520 560 nm and a long-pass filter with cut-on wavelength at 590 nm (for emitted light) were employed to visualize the Texas Red® molecules.

An optimal design of an optical fiber surface plasmon resonance (SPR) sensor based on wavelength modulation for hydrogen (H2) concentration detection is presented in this paper.

A Precision Long Pass filter NT62-9844) (Edmund Optics, York, UK) with rejection range of 200 539 nm, transmission region of 560 1650 nm, and cut-on wavelength at 550 nm was used for the camera lens.

c Quantum efficiency depends on the wavelength for the APD that includes the micro-structured and unstructured regions.

The refraction angle is dependent on the wavelength for a normal incident light, which is obtained from θ t = θ r = arcsin sinθ i −2π/k 0 Γ).

In the inset of Fig. 5a, dark I-V dependence of DLC:Ag/p-Si heterojunction in broader voltages range is presented Fig. 6 The dependence of the open circuit voltage (a) and short circuit current (b) on excitation wavelength for DLC:Ag/n-Si and DLC:Ag/p-Si heterostructures.

Analogues of the VRE may be predicted based on the wavelength for the peak photon-flux at the planetary surface if the incident stellar spectrum and the planetary atmospheric parameters are well known (Kiang et al., 2007a, 2007b).