Verbal noun of → load.
Fr.: escarpe lobée
A surface feature on a planet or satellite in the form of a line of cliffs. Lobate scarps are formed when planetary or lunar mantle cools down and contracts inside. The loss of volume squeezes portions of the outer crust together. Eventually, the crust breaks and some of it is pushed up, creating long cliffs that look like wrinkles. Lunar scarps are generally tens of kilometers long and less than 100 m high. They have formed during the last billion years.
General: A roundish projection that is part of a larger structure.
From M.L. lobus, from L.L. lobus "hull, husk, pod," from Gk. lobos "lobe of the ear, vegetable pod," probably related to leberis "husk of fruits;" from PIE base *lep- "to peel, flay."
Lap "lobe," variants lâp, lâb "piece, big piece, big cut," lappé "split pea; any of the two parts of a timber split through the length," maybe cognate with Gk. lobos, as above. Alternatively, related to Pers. las "loose," PIE *leu- "to loosen, divide, cut apart" (cf. Gk. lyein "to loosen, untie, slacken," lysus "a loosening;" L. luere "to loose, release;" → analysis).
Fr.: fonction de lobe
The configuration of the response lobes of a radiotelescope.
kuasâr-e lap ciré
Fr.: quasar à lobes dominants
A → radio-loud quasar in which the lobes dominate the whole emission. It has been conjectured that this phenomenon is an → orientation effect. If the → jet is close to the plane of the sky, the lobes will dominate. See also → core-dominated quasar.
Pertaining to, characteristic of, or restricted to a particular place or particular places.
From O.Fr. local, from L.L. localis "pertaining to a place," from L. locus "place."
Mahali, related to mahal "place, locality," from Ar.
Fr.: bras local
tangol-e mahali, hobâb-e ~
Fr.: Bulle locale
A region of low density in the → interstellar medium surrounding the → Solar System. It extends at least 300 → light-years in most directions and encompasses the stars of the immediate → solar neighborhood. The Local Bubble contains a hot, million-degree ionized hydrogen gas that emits in → X-rays. → Neutral hydrogen has a density approximately one tenth of the average for the interstellar medium in the Milky Way. The bubble is thought to be a result of the → shock waves from → supernovae sweeping through the region within the past two to four million years.
goruh-e mahali (#)
Fr.: Groupe local
A small cluster of about 40 galaxies to which our Milky Way Galaxy belongs. The Local Group occupies a volume of space nearly 10 million light-years across centered somewhere between the → Andromeda Galaxy (M31) and the Milky Way, which are the dominant galaxies of the group; Andromeda being the principal member. Both of these galaxies exhibit spiral structures, and each is attended by a large family of satellite → dwarf galaxies. The Local Group also includes a third spiral galaxy known as → Triangulum (M33), which is bound to Andromeda. The remaining members span a range of → Hubble classification types from dwarf spheroidal to Irr to Sb and Sc and cover a factor of 10 in → metallicity. The total mass of the Local Group is estimated to be about 2 x 1012 solar masses, although this value is still uncertain to within a factor of about 2. The velocities of the individual galaxies of the Local Group are not particularly high. Therefore no member is believed to be able to escape the group, which is thus considered to be gravitationally → bound. Another remarkable member of the Group is → IC 10.
local inertial frame
cârcub-e laxtnâk-e mahali, ~ laxtimand-e ~
Fr.: référentiel inertiel local
A coordinate system or frame of reference defined in the vicinity of the Earth in which Newton's first law of motion is valid; that is, a non-rotating and non-accelerating reference frame.
local interstellar cloud
abr-e andar-axtari-ye mahali
Fr.: nuage interstellaire local
local Lorentz invariance
nâvartâyi-ye Lorentz-e mahali
Fr.: invariance de Lorentz locale
Fr.: maximum local
Fr.: méridien local
The meridian through any particular place, serving as the reference for local time, in contrast to the Greenwich meridian.
Fr.: minimum local
navešgar-e mahali (#)
Fr.: oscillateur local
The oscillator in a heterodyne or superheterodyne radio receiver which produces the radio frequency oscillations with which the received wave is combined.
local position invariance
nâvartâyi-ye neheš-e mahali
Fr.: invariance de position locale
local sidereal time
zamân-e axtari-ye mahali
Fr.: temps sidéral local
Local time measured by the apparent motion of the stars. It is the most useful form of sidereal time since it gives the right ascension of a transiting celestial object at a given location.
Fr.: bras local
Same as → Orion Arm.
local standard of rest
estânde-ye mahali-ye âram
Fr.: standard local de repos
A frame of reference that turns around the Galactic center at a velocity and a distance which are the mean values for the stars in the solar neighborhood. In this reference system the stars belonging to the solar neighborhood are statistically at rest. The orbital velocity of the Local Standard of Rest around the Galaxy is about 220 km/sec.