spectral energy वाक्य
उदाहरण वाक्य
मोबाइल
- 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.
- 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.
- 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.
- 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.
- 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.
- "' 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.
- 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.
- 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.
- 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.
- 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.
- Addressing fluctuating partially coherent light emitters with a tailored spectral energy distribution in the optical range, this establishes the link between stochastic electrodynamics and coherence theory; henceforth putting forward a way to optically create and control both such zero-point fields as well as Lifshitz forces of thermal fluctuations.
- Temperature estimates for the star range from around 18, 000K to well over 30, 000K . The hotter temperatures found from fitting the spectral energy distribution ( SED ) are consistent with the calculated luminosity of an LBV in the quiescent stage, but the spectrum is that of a cooler star.
- The spectral density of the vacuum field is fixed by the form of the radiation reaction field, or vice versa : because the radiation reaction field varies with the third derivative of, the spectral energy density of the vacuum field must be proportional to the third power of in order for to hold.
- This technique " comprises variable distribution of the spectral energy, synthesis of the global sound sources, micro-and macro-form as sound-process, four simultaneous layers of perception and of speed, and spectral scordaturae, i . e . rows of unequal intervals corresponding to harmonic scales ".
- Dividing E _ s ( f ) by " Z " o, the characteristic impedance of free space ( in ohms ), the dimensions become joule-seconds per meter 2 or, equivalently, joules per meter 2 per hertz, which is dimensionally correct in SI units for spectral energy density.
- The hotspots that are usually seen in FRII sources are interpreted as being the visible manifestations of shocks formed when the fast, and therefore supersonic, jet ( the speed of sound cannot exceed c / " 3 ) abruptly terminates at the end of the source, and their spectral energy distributions are consistent with this picture.
- Therefore, BPSK-modulated signals such as C / A GPS codes have most of their spectral energy concentrated around the carrier frequency, while BOC-modulated signals ( used in Galileo system ) have low energy around the carrier frequency and two main spectral lobes further away from the carrier ( thus, the name of split-spectrum ).
- The visual appearance depends on the spectral energy distribution of an object's light, the red-or blueshift is a secondary effect to the visual appearance, which is not uniquely " red " or " blue " ( it is defined as a shift of the spectrum towards longer ( " redder " ) or shorter ( " bluer " ) wavelengths ) .-- talk ) 11 : 59, 16 August 2012 ( UTC)
- For example, if " x " ( " t " ) represents the magnitude of the electric field component ( in volts per meter ) of an optical signal propagating through free space, then the dimensions of " X " ( " f " ) would become volt�seconds per meter and E _ s ( f ) would represent the signal's spectral energy density ( in volts 2 �second 2 per meter 2 ) as a function of frequency " f " ( in hertz ).
- The background field is introduced as a Lorentz force in the ( classical ) Abraham-Lorentz-Dirac equation ( see : Abraham Lorentz Dirac force ), where the classical statistics of the electric and magnetic fields and quadratic combinations thereof are chosen to match the vacuum expectation values of the equivalent operators in QED . The field is generally represented as a discrete sum of cut off, the total field has an infinite energy density, with a spectral energy density ( per unit frequency per unit volume ) [ 2h / c 3 ] f 3 where h is Planck's constant.
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