condensation temperature

To talk about condensation temperature and subcooling under these conditions is not entirely possible.

In planetary science, any material that has a relatively high equilibrium condensation temperature is called refractory.

Volatile elements - are chemical elements that have low boiling and condensation temperatures.

But even above the condensation temperature, the collisions must be somewhat inelastic as the gas does begin to behave nonideally.

This temperature is close to the condensation temperature of troilite (FeS).

Fluorine condenses to a bright yellow liquid at 188 C ( 307 F), which is near the condensation temperatures of oxygen and nitrogen.

They are almost completely oxidized and contain the most low condensation temperature elements ("volatile" elements) and the largest amount of organic compounds.

The top trace again illustrates the condensation temperature of various compositions, and again, above the top trace the mixture must be entirely vapor phase.

The concentration of the product acid depends on the HO/SO ratio in the catalytically converted gases and on the condensation temperature.

The main disadvantages are that it cannot operate continuously and cannot effectively pump hydrogen, helium and neon, all gases with lower condensation temperature than liquid nitrogen.

The condensation temperatures are the temperatures at which 50% of the element will be be in the form of a solid (rock) under a pressure of 10 bar.

The value of superheated steam in these applications is its ability to release tremendous quantities of internal energy yet remain above the condensation temperature of water vapor; at the pressures at which reaction turbines and reciprocating piston engines operate.

Since the pressure increase of the vapor also generates an increase in the condensation temperature, the same vapor can serve as the heating medium for its "mother" liquid or solution being concentrated, from which the vapor was generated to begin with.

The rationale for the 20 radii formation is that the carbon condensation temperature is 1,500 K, while the photospheric dust model was formulated by the 20 radii models failure to explain the fast decline of the RCBs' light curves just before reaching minimum.