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similarity hamânandi (#) Fr.: similarité The state of being similar; likeness; resemblance. |
similarity transformation tarâdiseš-e hamânandi Fr.: transformation de similarité 1) A transformation that preserves angles and changes all distances in the same ratio. → similarity; → transformation. |
simultaneity hamzamâni (#) Fr.: simultanéité The property of events occurring → simultaneously. Noun from → simultaneous; → -ity. |
singularity takini (#) Fr.: singularité 1) Math.: A point at which a given mathematical object is not defined. |
solar activity žirandegi-ye xoršid Fr.: activité solaire The general term for all forms of short-lived phenomena on the Sun, including → solar flares, → sunspots, → prominences, etc., indicating that the Sun is an active star. |
solar activity cycle carxe-ye žirandegi-ye xoršid Fr.: cycle d'activité solaire Same as the → solar cycle. → solar activity; → cycle. |
solar luminosity tâbandegi-ye xoršid (#) Fr.: luminosité solaire The total → radiant energy, in all wavelengths, emitted by the Sun in all directions. It is 3.828 × 1026 W or 3.828 × 1033 erg sec-1 (International Astronomical Union, Resolution B3, 14 August 2015, Honolulu, USA). This is the luminosity unit conventionally used to give the luminosities of stars. See also: → solar constant. When the Earth first formed, 4.56 billion years ago, the Sun radiated 30% less energy than it does today, thus giving rise to the so-called → faint early Sun paradox. Ever since then, its power has increased by 7% every billion years (I. Ribas, 2009, arXiv:0911.4872). → solar; → luminosity. |
solar metallicity felezigi-ye xoršidi Fr.: métallicité solaire The proportion of the solar matter made up of → chemical elements heavier than → helium. It is denoted by Z, which represents the sum of all elements heavier than → helium, in mass fraction. The most recent determination of the solar Z gives a value of 0.0134 (Asplund et al. 2009, ARAA 47, 481), corresponding to the present-day photospheric composition. → solar; → metallicity. |
solar velocity tondâ-ye xoršid, ~ xoršidi Fr.: vitesse solaire The rate of change of the Sun's position with respect to the local standard of rest toward the → solar apex. |
solidity dafzegi Fr.: solidité The state, property, or quality of being solid. Solidness. |
sound intensity dartanuyi-ye sedâ Fr.: intensité de son The average → sound power passing through a unit area perpendicular to the direction that the sound is traveling. It is usually expressed in watts per square meter. |
sound intensity level tarâz-e dartanuyi-ye sedâ Fr.: niveau de l'intensité de son The expression of sound intensity in decibel units. The sound intensity level (LI), in decibels, is computed as: LI = 10 log (I/I0), where I is the measured sound intensity and I0 is the reference intensity (1 x 10 -12 watt per square meter). |
sound quality cunâ-ye sedâ Fr.: qualité de son The number of → overtones present in a sound and their respective intensity. Like → loudness, it is a subjective quantity and cannot be measured with instruments. |
space velocity tondâ-ye fazây Fr.: vitesse spatiale The velocity of a star relative to the Sun. |
special relativity bâzanigi-ye vižé Fr.: relativité restreinte The theory formulated by A. Einstein in 1905, which is based on the following
two → postulates: → special; → relativity. |
specific density cagâli-ye âbizé Fr.: densité spécifique Same as → relative density. |
specific gravity gerâni-ye âbizé Fr.: gravité spécifique The ratio of the density of a substance at the temperature under consideration to the density of water at the temperature of its maximum density (4 °C). |
specific humidity nam-e âbizé Fr.: humidité spécifique The dimensionless ratio of the mass of water vapor to the total mass in a particular volume. → humidity |
specific intensity dartanuyi-e âbizé Fr.: intensité spécifique A measure of the amount of radiation received per unit solid angle per unit time per unit area normally from an element of surface. |
specifity âbizegi Fr.: spécifité The state or character of being → specific. |
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