Noun:

সূর্যের আলোকময় বহিরাবরণ,

photospheres's Usage Examples:

There are several different computer codes available modeling stellar photospheres.

stars are larger and brighter than the Sun, with higher temperature photospheres − having effective temperatures of around 6,200 K compared to 5,772 K.

causes the spectroscopically-derived abundance of heavy elements in the photospheres of hot stars to be very much higher than solar abundance or than the.

Other stars may have hotter or cooler photospheres.

These cool temperatures allow molecules to form in their photospheres and atmospheres.

unlike Sun-like stars whose photospheres have a large number of small convection cells (solar granules), red-giant photospheres, as well as those of red.

(June 2002), "Do dusty A stars exhibit accretion signatures in their photospheres?", Astronomy and Astrophysics, 388 (3): 978–984, arXiv:astro-ph/0204449.

Both types of star have luminous and unstable photospheres at this stage of their lives and often have the spectra of supergiants.

(November 1994), "Stratification of helium in the photospheres of the helium-weak stars HD 28843 and HD 49333", Astronomy and Astrophysics.

titanium oxide is caused by the formation of perovskite grains in the photospheres of L-dwarfs.

have found that some have significantly less carbon and oxygen in their photospheres than is typical, which is evidence of their outer material having been.

spectra that are harder than expected from hot (~100,000 K) central star photospheres, possibly indicating a high frequency of binary companions to CSPNe.

to SNe Ia, but have lower maximum-light velocities, and most have hot photospheres.

"Expanding photospheres of type II supernovae and the extragalactic distance scale".

occultations also provide opportunities to study the magnetospheres and photospheres of T Tauri stars in unprecedented detail.

Synonyms:

sun; Sun; surface;

Antonyms:

stand; sit; workday; uncover;