Sentence examples for opacity regions from inspiring English sources

Surprisingly, many wispy or string-like features similar to cirrus clouds on Earth are also seen on the nightside at low and midlatitudes which correspond to low opacity regions, indicating higher radiances from the atmosphere due to warmer temperatures.

Origins of such sharp opacity regions are not easy to explain dynamically without invoking "different air masses" as was suggested to explain the VeGa balloon dynamical results (Blamont et al. 1986), but then the challenge is explaining the origins of different air masses.

At the frequencies in question, the magnetosphere as a whole is an opacity region for FMS.

To the left of x S, there is an opacity region expanding to −∞ in the x direction.

If the wave source is to the right of the transition layer, then, using an asymptotic representation of (14) in the opacity region at, we find C1 =0.

One is the Alfven resonance point, x A, defined by equality Ω2 X A ) = 0, located in the opacity region in the interval (x01, x02).

Since the magneto-sphere is an opacity region for the fast magnetosonic waves with m ≫ 1, their amplitude in the magnetosphere decreases exponentially, on a small scale, with distance from the region of its generation.

Note the energy absorption of the incident wave does not exceed 50% in the neighbourhood of the Alfven resonance surface located deep within the opacity region (x01, x02) (Leonovich et al., 2010).

If the wave source is to the left of the resonance surface (in the opacity region x < x s (ξs < 0)), then in the SMS wave transparency region, ξs > 0, expanding ad infinitum, the solution of (9) must describe a wave escaping from the resonance surface.

If the parameters of the wave under consideration are such (the first condition (11)) that the incident wave "leaks" through the barrier of opacity region (x01, x02) into the SMS-wave transparency region (x s, x01), then the energy of the wave penetrating through this barrier is absorbed completely in the neighbourhood of the resonance surface.

Here we shall use the model spectrum function constructed in Leonovich and Mishin (1999) (24 where C is a constant determined by the average oscillation amplitude, and Φ (k t, ω) is a step function determining the upper and lower limits of the spectrum, as well as the wave range for which the solar wind is an opacity region.