mode tarz, mod Fr.: mode 1) Physics: Any of the distinct patterns of oscillation that a
given periodically varying system can have. Mode, from Fr. mode, from L. modus "measure, rhythm, song, manner," from PIE base *med- "to measure, limit, judge, advise;" cf. L. meditari "to think or reflect upon, consider;" Av. mad- "to measure out, apportion, allot;" Gk. medein "to rule;" O.E. metan "to measure out." Tarz "manner, mode," Arabicized as |
model 1) (n.) model, tarzâl; 2) (v.) model sâxtan, tarzâlidan Fr.: 1) modèle; 2) modéliser 1a) A mathematical representation of a process, system, or object
developed to understand its behavior or to make predictions. The
representation always involves certain simplifications and
assumptions. See also → theory,
→ hypothesis. M.Fr. modelle (Fr. modèle), from It. modello "a model, mold," from V.L. *modellus, from L. modulus "measure, standard," from modus "manner, measure" (cf. Av. mad-, → mode), PIE *med- + -ulus, → -ula. 1) Model, from Fr. modèle.
Tarzâl, from tarz, → mode + -âl,
→ -al. |
model dependence vâbastegi bé model, ~ ~ tarzâl Fr.: dépendance du modèle In a theoretical analysis, the solution that does not correctly treat the intervening parameters, or neglects some crucial factors. |
modeling modelsâzi, tarzâleš Fr.: modélisation The simulation of a process, concept, or operation of a system often implemented by a computer program and making use of a mathematical treatment. Verbal noun of → model |
modern novin (#) Fr.: moderne 1) Relating or belonging to present and recent time.
→ modern physics. From M.Fr. moderne, from L.L. modernus, from L. modo "lately, just now," from modo "to the measure," ablative of modus "manner, measure," → mode. Novin, from now, → new, + -in adj. suffix, as in dirin, pasin, barin, kehin, mehin, behin, zirin, zabarin, pâyin, bâlâyin. |
modern physics fizik-e novin (#) Fr.: physique moderne The physics developed since about 1900, which includes Einstein's → relativity theory and → quantum mechanics, as distinguished from → classical physics. Much of modern physics is concerned with the behavior of matter and energy under extreme conditions or on the very small scale. |
modernism novingerâyi Fr.: modernisme 1) Modern spirit or character. |
modernist novingerâ Fr.: moderniste 1) An admirer of modern ideas, ways, etc. |
modernity novini (#) Fr.: modernité 1) The quality of being → modern. |
modernization novineš (#) Fr.: modernisation 1) The act of modernizing; the state of being modernized; something modernized. |
modernize novinidan (#) Fr.: moderniser To bring something up to modern standards, or adapt it to modern style, conditions, etc. |
MRN dust model model-e MRN Fr.: modèle MRN A model concerned with the distribution in size of → interstellar grains to account for observations of → interstellar extinction from 0.11 μm to 1.0 μm. The → distribution has the form N(a)da ∝ a-3.5da, where a is the grain radius. It extends from 5 nm to 1 μm for → graphite and over a narrower range for other materials. MNR, the initials of authors J. S. Mathis, W. Rumpl, and K. H. Nordsiek (1977, ApJ 217, 425), who introduced the mode; → dust; → model. |
neutral mode mod-e natâr, tarz-e ~ Fr.: mode neutre In hydrodynamic instability theory, a wave solution the amplitude of which does not change with time; it neither grows nor decays. Also called neutral wave. |
numerical modeling modelsâzi-ye adadi (#), tarzâlsâzi-ye ~ Fr.: modélisation numérique The prediction of the evolution of a system via numerical construction of approximate solutions to the governing equations. |
oblique rotator model model-e carxande-ye yekvar Fr.: modèle de rotateur oblique A stellar model in which the rotation axis is tilted relative to the magnetic dipole axis. As the star rotates, observable quantities (e.g. the line-of-sight component of the magnetic field, stellar brightness, emission lines) are modulated according to the rotational period. Such a model was first put forward by D. Stibbs (1950, MNRAS, 110, 395). |
oscillation mode tarz-e naveš, mod-e ~ Fr.: modes d'oscillation Same as → pulsation mode. → oscillation; → mode. |
p mode tarz-e p, mod-e ~ Fr.: mode p Acoustic waves trapped inside stars, which act as a resonating cavity, exhibiting millions of oscillation modes or standing waves. Same as → pressure mode. P-mode oscillations in the Sun have frequencies in the 0.2-5.5 mHz range. They are particularly intense in the 2-4 mHz range, where they are often referred to as solar "5-minute oscillations." See also → pulsation mode. P, referring to pressure; → mode. |
pancake model model-e lavâš Fr.: modèle des crêpes A model of galaxy formation in which regions of primordial gas as massive as clusters of galaxies began to collapse into thin sheets (pancakes). Within the pancakes, smaller regions of gas later collapsed to form individual galaxies. |
pointing model model-e âmâješ Fr.: modèle de pointage A mathematical model that reproduces the diurnal rotation of the Earth and is used to direct a telescope toward a precise position on the sky. |
postmodernism pasâ-novingerâyi Fr.: post-modernisme Any of a number of trends or styles in architecture, philosophy, literature, and art developed in the latter part of the 20th century often in reaction to → modernism. In philosophy, postmodernists claim that value systems are concoctions of human partial knowledge rather than systems reflecting universal objective truth. The most influential early postmodern philosophers include Jean Baudrillard, Jean-François Lyotard, and Jacques Derrida. The term postmodernism was first coined by architects to designate an architectural response against the earlier Bauhaus style, which was characterized by box-like apartment buildings, the absence of ornamentation and harmony between the function of a building and its design; → post- + → modernism. |