Sentence examples for burning phases from inspiring English sources

Four typical burning phases including pre-heating burning, steady burning, thin-layer burning and extinguishment were identified.

During the presupernova evolution of massive stars, from oxygen shell burning till around end of convective core silicon burning phases, the calculated neutrino cooling rates due to 54Fe are three to four times larger than the corresponding shell model rates.

A single-zone combustion process starts with a rapid premixed burning phase, followed by a slower mixing-controlled burning phase.   5.

Should heat release exceed heat loss as the temperature increases to that for hot ignition, initiation of a high temperature burning phase may be possible.

The star is thought to be around 4.5 billion years old, and at or very near the end of its main-sequence hydrogen burning phase.

Semi-permanent cultivators have developed a positive attitude towards the cultivation of groundnut and other Leguminosaea, which in a slash and burn system can help replenish nitrogen volatilized during the burning phase (Budelman and Ketelaars 1974).

It is based on a single-zone combustion modeling with a rapid premixed burning phase followed by a slower mixing-controlled burning phase.

Slightly more massive stars up to ({sim}11M_{odot}) experience an additional nuclear burning phase.

The present rapid thermodynamic simulation for the direct-injection diesel engine is based on a single-zone combustion modeling with a rapid premixed burning phase followed by a slower mixing-controlled burning phase.

In their development, the combustion process starts from a rapid premixed burning phase (represented by function f1), followed by a slower mixing-controlled burning phase (represented by function f2), with both functions empirically linked to the duration of ignition delay ( τ ˜ id Open image in new window) and the duration of combustion (Δθcomb).

Timing studies in X-rays (combined with the optical) of the stable nuclear burning phase in steady nuclear burning sources and in post-novae allow to constrain the mass accretion rate onto and the mass of the nuclear burning WD.