• विकिरण ताप • विकिरण-ताप | |
radiation: प्रकाश प्रभा | |
temperature: हालत टेम्परेचर | |
radiation temperature मीनिंग इन हिंदी
radiation temperature उदाहरण वाक्य
उदाहरण वाक्य
अधिक: आगे- Slight deviations in the radiation temperatures revealed the cosmic ripples around which matter presumably gravitated, eventually leading to stars and galaxies.
- The infrared radiometer showed that the 8.4 ?m and 10.4 ?m radiation temperatures were in agreement with radiation temperatures obtained from Earth-based measurements.
- The infrared radiometer showed that the 8.4 ?m and 10.4 ?m radiation temperatures were in agreement with radiation temperatures obtained from Earth-based measurements.
- The 8.4 ?m and 10.4 ?m showed equal radiation temperatures, indicating that the limb darkening effect would appear to come from a cloud structure rather than the atmosphere.
- Other experimenters, using instruments boosted up to 120, 000 feet by balloons detected variations to within 100 millionths of a degree in the cosmic microwave background radiation temperature.
- Because it can see the effective radiation temperature of an object as well as what that object is radiating towards, it can help locate sources of thermal leaks and overheated regions as well.
- For a hypothetical proton lifetime of 10 37 years, Adams and Laughlin calculate that proton decay will raise the solar-mass white dwarf to approximately 0.06 K . Although cold, this is thought to be hotter than the cosmic background radiation temperature 10 37 years in the future ., �IVB.
- Rapid evaporative cooling of the skin would create frost, particularly in the mouth, but this does not represent a significant hazard ( relative to ebullism, etc . ) : the effective black-body radiation temperature throughout most of space is conduction; so the main temperature regulation concern is excess naturally generated body heat.
- As the temperature of a black hole is determined by the black body radiation temperature of the radiation that comes from it, it is possible to determine that the temperature of any observable black holes ( as opposed to theorised sub-atomic ones ) would be extremely close to absolute zero ( ~ . 00000001-. 00000000000000000001K ).
- For the density of the observable universe of about 4.6?0 " 28 kg / m 3 and given the known abundance of the chemical elements, the corresponding maximal radiation energy density of 9.2?0 " 31 kg / m 3, i . e . temperature 3.2 K ( matching the value observed for the optical radiation temperature by Arthur Eddington ).