Sentence examples for reflection of the solar from inspiring English sources

As the Sun's motion in its orbit around the Galaxy is estimated to be approximately 250 km/sec in this direction, the value V of −288 km/sec is primarily just a reflection of the solar orbital motion.

The observed third ring (red cross) in Fig. 5 is found at velocity space near this prediction for all cases, and therefore, the third ring distribution is well explained by the secondary specular reflection of the solar wind ions.

Although the present study is not statistically strong, the data support common occurrence of multiple specular reflection of the solar wind at the bow shock, and hence support the explanation by the abundance of cold ions at the Martian bow shock as the reason for the speciality of Mars, i.e., not reported at the Earth or Venus (Yamauchi et al., 2011).

In all seven cases, the velocity components of the energy-bunched structure are consistent with multiple specular reflections of the solar wind at the bow shock up to at least two reflections.

Yamauchi et al. (2011) further showed that the third ring distribution at energy higher than the second ring distribution in the 12 July 2005 event agrees with second reflection of the reflected solar wind ions at the bow shock, as shown in Fig. 1(c).

Then, by simulating the reflection of these solar distributions off a set of non-ideal mirrored surfaces, accounting for non-specular reflection and mirror shape errors, the combined effect of sunshape and mirror properties on the solar image is obtained.

The photocurrent density (J ph), total current density (J tot), total loss percentage (P loss), loss current density (J loss), reflection loss (R), and parasitic absorption loss were calculated by integrating the absorption and reflection spectrum of the solar cell [15, 32].

A ray-tracing model was developed to simulate the reflection of the direct solar radiation on the CPC reflectors at different angles of incidence and compute the absorbed solar radiation distribution on the absorber surface.

The first type of event, with no apparent upward-going flux enhancement (30% of observations), does in fact display features broadly consistent with adiabatic reflection of the incoming solar wind distribution.

To investigate the effective reflection of the Si nanostructures on the solar cell performance under the solar radiation spectrum (i.e., the terrestrial air mass 1.5 global (AM 1.5G) [20]), we calculated the SWR, as given in the following equation [21]: SWR = ∫ R λ N photon dλ ∫ N photon dλ, where R is the reflectance and Nphoton is the photon number of AM 1.5G per unit area per unit wavelength.

The reflection of solar radiation from the edges could also increase the insolation enough to burn the card of Campbell Stokes sunshine recorder.