acronical setting forušod-e šâmgâhi Fr.: coucher acronyque The setting of a star at nightfall. → heliacal setting. |
affine set hangard-e karvan Fr.: ensemble affine A set → if and only if (iff) for any two points in the → set, the line through them is contained in the set. In other words, for any two points in the set, their → affine combinations are in the set itself. |
alpha offset apneh-e Âlfâ Fr.: offset en ascension droite A short distance from the target, in right ascension, where the telescope is pointed for various purposes. |
apparent setting forušod-e padidâr Fr.: coucher apparent The instant of time when the object is in the West and the geometric → zenith distance is equal to 90° plus the → horizontal refraction plus the semidiameter minus the → parallax. |
bias offset apneh-e varak Fr.: biais In → CCD detectors, same as → bias and → offset. |
complete set hangard-e ospor Fr.: ensemble complet Quantum mechanics: A set of states such that any state can be represented as a superposition of them. |
crisp set hangard-e tuj Fr.: ensemble net A classical set that allows only full membership or no membership at all for its elements, as contrasted with a → fuzzy set. Crisp set can be viewed as a restricted case of the more general fuzzy set concept. |
delta offset apneh-e deltâ Fr.: offset en déclinaison A short distance from the target, in → declination, where the → telescope is pointed for various purposes. |
disk settling niyâšeš-e gerdé, ~ disk Fr.: stabilisation de disque The process whereby a → galaxy evolves from a disturbed to an ordered system, as it develops into a → rotation dominated → settled disk. |
dust settling niyâšeš-e qobâr Fr.: dépose de poussières A process occurring in → protoplanetary disks whereby relatively large → dust grains settle to the disk midplane. These grains, with sizes from → micron to → millimeter, grow from smaller dust grains and will eventually give rise to a planetary system. |
empty set hangard-e tohi Fr.: ensemble vide A set containing no → elements. |
family of sets xânevâde-ye hangardhâ Fr.: famille de comètes A → collection of → subsets of a set. |
finite set hangard-e karânmand Fr.: ensemble fini A → set whose elements can be numbered from 1 to n, for some positive integer n. |
fuzzy set hangard-e porzvâr Fr.: ensemble flou A set of → truth values in → fuzzy logic that does not have sharp boundaries. Instead, set members have degrees of membership. If the value of 1 is assigned to objects entirely within the set and a 0 is assigned to objects outside of the set, then any object partially in the set will have a value between 0 and 1. This contrast with → crisp sets in → classical logic where members assume a precise value of 1 or 0. Fuzzy sets were first introduced by Lotfi A. Zadeh (1965) and defined as follows. Let X be a space of points, with a generic element of X denoted by x. Thus X = {x}. A fuzzy set A in X is characterized by a → membership function fA(x) which associates with each point in X a real number in the interval [0,1], with the values of fA(x) at x representing the "grade of membership" of x in A. Thus, the nearer the value of fA(x) to unity, the higher the grade of membership of x in A. Generally, the intersection operations of fuzzy sets are the expansion of that operation on → nonfuzzy sets. In other words, operations on nonfuzzy sets are a particular case of operations on fuzzy sets. |
gravitational settling niyâšeš-e gerâneši Fr.: décantation par gravité A physical process occurring in → stellar atmospheres whereby in a very stable atmosphere → heavy elements are gravitationally pulled down preferentially. If such an atmosphere is stable for long periods of time, the → absorption lines of heavy elements may therefore become very weak. Observationally, the star seems to contain only → hydrogen and → helium. Gravitational settling takes place in the Sun at the bottom of the outer → convective zone where helium is dragged down, leading to a surface He abundant smaller than the cosmic value. It occurs also in the atmospheres of → brown dwarfs and → planets. See also → radiative levitation, → element diffusion, → thermal diffusion. → gravitational; → settling. |
heliacal setting forušod-e hurâné Fr.: coucher héliaque The last visible setting of a star below the western horizon just after sunset entering into a conjunction with the Sun. |
infinite set hangard-e bikarân Fr.: ensemble infini A set which can be put in a one-to-one correspondence with part of itself. |
Mandelbrot set hangard-e Mandelbrot Fr.: ensemble de Mandelbrot A set of points in the complex plane, the boundary of which forms a fractal with varying shapes at different magnifications. Mathematically, it is the set of all C values for which the iteration zn+1 = zn2 + C, starting from z0 = 0, does not diverge to infinity. Discovered by Benoît Mandelbrot (1924-) a Polish-born French mathematician, best known as the "father of fractal geometry;" → set. |
moonset forušod-e mâng (#) Fr.: coucher de la lune The crossing of the visible horizon by the upper limb of the descending Moon. |
moonset lag lek-e forušod-e mâng Fr.: retard du coucher de la lune |