Noun:

सूर्याचे तेजस्वी बाह्य आवरण,

photospheric's Usage Examples:

stars are defined as a group by the existence of rotationally broadened photospheric spectral lines in combination with very narrow absorption lines.

astronomers working in the near-infrared announced that the more accurate photospheric measurement was 43.

helio-latitude, as the speed of the photospheric footpoint is reduced.

lines in the star"s spectrum, but these are likely caused by regions of photospheric activity rather than being a barium star.

Its spectrum is described as having a non-photospheric continuum and silicon absorption lines, indicative of high mass loss.

and James, S: Solar chromospheric spicules from the leakage of photospheric oscillations and flows In: Nature.

radius, even when future observations will likely refine the Sun"s actual photospheric radius (which is currently only known to about an accuracy of ±100–200 km).

main-sequence star, having a Sun-like stellar classification of G2 V and a photospheric temperature only slightly higher than the sun.

the near-infrared spectrum of 2MASS J0348−6022 to various published photospheric models and derived multiple best-fit solutions for its effective temperature.

sunlight scattering off free electrons; Doppler broadening of the reflected photospheric absorption lines spreads them so greatly as to completely obscure them.

form in filament channels above divisions between regions of opposite photospheric magnetic polarity called polarity inversion lines (PIL), polarity reversal.

solar telescope with a main mirror diameter of 50 cm A chromospheric and photospheric AFR-2 telescope with dimensions of 20/13 cm, used for solar service The.

HD 12545 had a warm spot (350 K above photospheric temperature; the white area in the picture) Xu Zhen-Tao (1980).