The most consistent outcomes from such experiments are that brightness or spectral energy distribution, and the " bite ", or rate and synchronicity and rise time, of the attack are important factors.
22.
The power spectral density ( PSD ) then refers to the spectral energy distribution that would be found per unit time, since the total energy of such a signal over all time would generally be infinite.
23.
For conditions of thermodynamic equilibrium, together the number densities n _ 2 and n _ 1, the Einstein coefficients, and the spectral energy density provide sufficient information to determine the absorption and emission rates.
24.
Since slower tumbling displaces the spectral energy at high tumbling frequencies to lower frequencies, the relatively low beat frequency will experience a monotonically increasing amount of energy as \ tau _ c increases, decreasing relaxation time.
25.
This interaction is dependent on the spectral energy distribution ( SED ) of the EBL . Therefore, it is necessary to know the SED of the EBL in order to study intrinsic properties of the emission in the VHE sources.
26.
"' Noise shaping "'is a filtering process that shapes the spectral energy of quantisation error, typically to either de-emphasise frequencies to which the ear is most sensitive or separate the signal and noise bands completely.
27.
A frequency ( or spectral energy ) emitted in a transition from " n " 1 to " n " 2 therefore represents the photon energy emitted or absorbed when an electron makes a jump from orbital 1 to orbital 2.
28.
Non-tidal factors, such as extreme stellar variation, spectral energy distributions shifted to the infrared relative to the Sun, and small circumstellar habitable zones due to low light output, further reduce the prospects for life in red-dwarf systems.
29.
Using this expression for the total energy of an atom ( or ion ) as a function of the shielding constants and effective quantum numbers, Slater was able to compose rules such that spectral energies calculated agree reasonably well with experimental values for a wide range of atoms.
30.
This involved the development of several key technical innovations to better determine the galaxies spectral energy distributions, especially the world's first optical fibre multi-object spectrograph on the AAT, which simultaneously gathered high quality spectra for large numbers of these faint galaxies in distant clusters.
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