A long pass filter (Schott OG-530, Edmund Optics, Barrington, USA) with an edge wavelength at 530 nm and an OD ≥ 5 at the excitation wavelength was placed behind the entrance of the spectrograph to eliminate any laser light guided through the fiber.
With a weakened anchor, a quarter wavelength was placed on its length (F is low) and the inner layer of roof rocks determined the measured data.
In near-field scanning optical microscopy, a light source or detector with dimensions less than the wavelength is placed in close proximity (λ/50) to a sample to generate images with resolution better than the diffraction limit.
With a tensioned anchor, it was determined that at the free length of the anchor, half of the wavelength was placed (F is high) and the outer layer of roof rocks determined the measured data.
The chambers were filled to the top with buffer, and worms synchronized for size (900±40 µm in length, 650±40 µm wavelength) were placed in the structures and tested for motility.
Some radio telescopes, particularly those designed for operation at very short wavelengths, are placed in protective enclosures called radomes that can nearly eliminate the effect of both wind loading and temperature differences throughout the structure.
The electric field distributions in the case of more wavelengths are placed in Additional file 1.
Experimental nets had UV LEDs (peak wavelength 396 nm) placed every 5 m on the floatlines.
Three to five stimuli (10 s apart, 0.5 s long) were presented after 2 min adaptation in the dark laboratory, from the blue component of LEDs, (Kingbright, KAF-5060PBESEEVGC, maximum emission wavelength 465 nm) placed ∼6 cm in front of the fly.
An ultra-broadband absorber of light is proposed by using periodic array of ultra-thin metallic ribbons on top of a lossless quarter-wavelength dielectric spacer placed on a metallic reflector.
