spectral energy वाक्य
उदाहरण वाक्य
मोबाइल
- All stars have a spectral energy distribution that depends on their surface temperature.
- It is that which contributes to a double-peaked spectral energy distribution.
- An adductory gesture is also identified by the change in voice spectral energy it produces.
- Each component has the same spectral energy distribution and is an image of the quasar.
- Which is just the spectral energy density for Planck's law of black body radiation.
- This is also a spectral energy density function with units of energy per unit wavelength per unit volume.
- The witch of Agnesi approximates the spectral energy distribution of spectral lines, particularly X-ray lines.
- It was first considered notable for its infrared excess and double-peaked Spectral energy distribution in the infrared.
- The double-peaked spectral energy distribution and polarization are strongly indicative of a dust shell around the star.
- From Planck's law of black-body radiation at temperature we have for the spectral energy density at frequency
- From this equation one can derive the spectral energy density as a function of frequency and as a function of wavelength:
- The Ghost Hunter is searching for William in order to obtain'spectral energy'which is only obtainable from capturing ghosts.
- The derivation yields the spectral energy distribution " u " which is the energy per unit volume per unit frequency interval:
- The exact value of the Eddington luminosity depends on the chemical composition of the gas layer and the spectral energy distribution of the emission.
- One conventional way is to define a series of " frequency bins " into which you allocate the spectral energy of the waveform being analyzed.
- Combining the spectral energy distribution with the surface brightness profile yields a smaller estimate of the radius of the inner hole, 1-10 AU.
- Radio, infrared, and space-based observations have expanded coverage of Eta Carinae across all wavelengths and revealed ongoing changes in the spectral energy distribution.
- The simplest way to measure the luminosity of a star is to observe its radiated output at all wavelengths ( the spectral energy distribution or SED ) and sum them together.
- As a consequence of Parseval's theorem, one can prove that the signal energy is always equal to the summation across all frequency components of the signal's spectral energy density.
- That colour has nothing to do with the redshift, it is due to the fact that these galaxies contain lots of young stars which have a spectral energy distribution that increases towards the ultraviolet.
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