transmission tarâgosil (#) Fr.: transmission 1) The act or process of transmitting. The fact of being transmitted. Verbal noun of → transmit. |
transmission band bând-e tarâgosil (#) Fr.: bande de transmission The frequency range above the cutoff frequency in a waveguide or transmission line. → transmission; → band. |
transmission coefficient hamgar-e tarâgosil Fr.: coefficient de transmission The ratio given by the → amplitude (or energy) of a transmitted wave divided by the amplitude (or energy) of the incident wave. → transmission; → coefficient. |
transmission grating turi-ye tarâgosili Fr.: réseau par transmission A diffraction grating that has grooves ruled onto a transparent material so that a beam of light passed through the grating is partly split into spectral orders. → transmission; → grating. |
transmission loss dastraft-e tarâgosil Fr.: perte de transmission A decrease in power in transmission from one point to another. → transmission; → loss. |
transmission system râžmân-e tarâgosil Fr.: système de transmission An assembly of elements which are capable of functioning together to transmit power or signals. → transmission; → system. |
two-photon emission gosil-e do-fotoni Fr.: émission à deux photons The simultaneous emission of two photons whose sum of energies is equal to that of a single electron transition. The energy of each individual photon of the pair is not fixed, so that the spectrum of two-photon emission is continuous from the wavelength of that transition to infinity. In practice, there is a peak in wavelength distribution of the emitted photons. Two-photon emission is studied atomic physics with application in astrophysics, as it contributes to the continuum radiation from → planetary nebulae. It was recently observed in condensed matter and specifically in → semiconductors. |
weak emission-line central star (wel) setâre-ye markazi bâ xatt-e gosili-ye nezâr Fr.: étoile centrale à faibles raies d'émission A member of a class of cntral stars of planetary nebula, → CSPN, which have weaker and narrower emission lines than → Wolf-Rayet-like CSPNe (Tylenda et al. 1993, A&AS 102, 595). |