radiation pressure मीनिंग इन हिंदी

अधिक: आगे

The major part of this perturbation is contributed by classical radiation pressure:
Over time, radiation pressure from the cluster will disperse the molecular cloud.
In the heaviest non-degenerate stars, radiation pressure is the dominant pressure component.
Solar radiation pressure affects bodies throughout much of the Solar System.
This is related to radiation pressure tangential to the grain's motion.
Both the lorentz force and radiation pressure only affect charged particles.
:You can read about this at Solar sail and radiation pressure.
This allows you to use conservation of momentum to calculate the radiation pressure.
:: According to solar sail, the pressure comes from radiation pressure.
:: : : There can be no radiation pressure without charges.

संज्ञा.

the minute pressure exerted on a surface normal to the direction of propagation of a wave
पर्याय: corpuscular-radiation pressure