Unusual solar activity might lead to an increase in incident radiation.
A key design goal is that each original ionising event due to incident radiation produces only one avalanche.
The point at which a lens or mirror will focus parallel incident radiation.
A bolometer measures the energy of incident electromagnetic radiation.
Too low a pressure and the efficiency of interaction with incident radiation is reduced.
The temperature at any given position would depend upon the intensity of the incident radiation at that wavelength.
The pulse carries information about the energy of the original incident radiation on the scintillator.
The concavities they leave reflect incident radiation from side to side, and thus continue to grow.
Lack of nutrients, rather than low temperature or incident radiation, is the single most important factor restricting primary production.
Thus, the energy required for such a transition may be calculated if the frequency of the incident radiation is known.
