parallax

İngilizce - Türkçe

parallax teriminin İngilizce Türkçe sözlükte anlamı: paralaks; kaçkınlık; kaçkinlik; bir nesnenin konumunun, gözlemcinin konumundaki değişim nedeniyle, bir referans sistem veya bir dizi nokta yada nesnelere göre belirgin olarak yer değiştirmesi; (Tıp) Gözlemci (müşahit) nin yeri değiştikçe cismin görünüşünde meydana gelen değişiklikler; (isim) paralaks; ıraklık açısı
parallax correction: (Askeri) MEVKİ FARKI DÜZELTMESİ: Bir hedefin; toptan ölçülen mevki ile gözetleyici mevziinden ölçülen mevkii arasındaki fark için hesaplanmış düzeltme
parallax difference: (Askeri) PARALAKS FARKI: Bir cismin tepesinin yer değiştirmesiyle kaidesine nazaran meydana gelen ve cismin bir hava fotoğrafı stereo çiftindeki iki ayrı hayaliyle ölçülen fark
parallax error: (Askeri) PARALAKS HATASI: Bir alet taksimatının, tam cepheden okunacak yerde, yandan okunması yüzünden meydana gelen hata
parallax offset mechanism: (Askeri) MEVKİ FARKI GİDERME TERTİBATI: Dinleme cihazının üzerinde bulunan ve dinleme cihazını, vereceği bilgileri kullanacak olan batarya veya ışıldaktan biraz mesafeli olarak yerleştirilmiş olmaktan doğacak mevki farkı hatalarını düzelten cihaz
false parallax: (Askeri) zahiri paralaks
angle of parallax: paralaks açısı
annual parallax: yıllık paralaks
dynamic parallax: dinamik paralaks
horizontal parallax: ufuk paralaksı
motion parallax: Hareket paralaksı
secular parallax: çağ ıraklık acısı
stellar parallax: yıldız paralaksi, yıldız ıraklık acısı
angle of parallax: (Askeri) TOPLAMA AÇISI; YAKINSAMA AÇISI; PARALAX AÇISI: Bak. "angle of convergence"
angular parallax: açısal paralaks
angular parallax: (Askeri) AÇISAL PARALAKS: Grid kuzeyi ile coğrafi kuzey arasındaki açı. Bu açı, gridin standart meridyenden uzaklaşması oranında büyür
annual parallax: (Astronomi) yıllık ıraklık açısı
false parallax: (Askeri) ZAHİRİ PARALAKS: Stereospik olarak görülen bir cismin hakiki mevkiinden dikey istikamette zahiri yer değiştirmesi, böyle bir durum, cismin kendi hareketi kadar gözetleme noktasındaki değişiklikten de ileri gelir
geocentric parallax: (Astronomi) jeosentrik paralaks
geocentric parallax: (Astronomi) yermerkezli ıraklık açısı
gun parallax: (Askeri) MEVKİ FARKI: Bak. "parallax"
heliocentric parallax: (Pisikoloji, Ruhbilim) güneş merkezli paralaks
horizontal parallax: (Astronomi) gözerimi ıraklık açısı
horizontal parallax correction: (Askeri) YATAY TOPLAMA AÇI DÜZELTMESİ: Bak. "angle of convergence"
stellar parallax: (Astronomi) yıldız paralaksı
stellar parallax: (Astronomi) yıldız ıraklık açısı

İngilizce - İngilizce

parallax teriminin İngilizce İngilizce sözlükte anlamı: The change of angular position of two stationary points relative to each other as seen by an observer, due to the motion of an observer; The angle of seeing of the Astronomical Unit; The apparent shift of an object against a background due to a change in observer position; The change in the position of an object in the heavens due to the orbit of the earth Observable parallax in the fixed stars is a proof of the rotation of the earth around the sun Explanatory Diagram; Parallax is when an object appears to change its position because the person or instrument observing it has changed their position. Difference in the direction of a celestial object as seen by observers from two widely separated points, a measurement used to find a body's distance. The two positions of the observers and that of the object form a triangle; its apex angle (at the object) is twice the parallax, which becomes smaller with increasing distance. Observations for calculating the Sun's parallax can be made simultaneously from two different places on Earth's surface; that value reaches a maximum of 8.794 seconds of arc for observers at points separated by Earth's diameter. Observing the difference in an object's position as seen from Earth at points six months apart in its orbit (stellar, or annual, parallax) allows measurements of distances (e.g., of stars) too large to be made from two places on Earth's surface. The nearest star system, Alpha Centauri, has a stellar parallax of 0.76 second of arc. Highly precise parallaxes, and thus the positions, of more than 100,000 stars in the Sun's vicinity were determined from data collected by the European Space Agency's Hipparcos satellite (launched 1989); With a lens-shutter camera, parallax is the difference between what the viewfinder sees and what the camera records, especially at close distances This is caused by the separation between the viewfinder and the picture-taking lens There is no parallax with single-lens-reflex cameras because when you look through the viewfinder, you are viewing the subject through the picture-taking lens; Angular displacement in the apparent position of a celestial body when observed from separated points; an apparent shifting of an object's position resulting from observing the object from two different vantage points Stellar parallaxes are seen when we view nearby stars from opposite sides of the Earth's orbit; The difference in appearance or position of an object when viewed from two different locations; the difference in apparent direction of an object as seen from two different vantage points; The apparent angular displacement of an object as seen in an aerial photograph with respect to a point of reference or coordinate system Parallax is caused by a difference in altitude or point of observation; the apparent displacement of an object as seen from two different points that are not on a line with the object; Parallax is the effect that nearby objects seem to move relative to far-away objects when you move to another viewpoint The parallactic angle is the angle over which the nearby object seems to move relative to the background In astronomy, the maximum parallactic angle of a star due to the motion of the Earth in its orbit around the Sun is called the star's parallax Because stars are very far away, their parallaxes are very small: the nearest star has a parallax of only 0 76 arcseconds; The difference between what the viewfinder sees and what the camera records Typical of lens/shutter cameras and is caused by a separation of the viewfinder and the picture taking lens (ie the user is not viewing the image through the picture taking lens); An effect seen in close-up photography when the viewfinder is offset by some distance from the lens The scene through the viewfinder is offset from the scene through the lens; The difference in point of view that occurs when the lens (or other device) through which the eye views a scene is separate from the lens that exposes the film; parallaxis = [Greek] change Parallax is the effect that nearby objects seem to move relative to far-away objects when you move to another viewpoint For instance, if you hold your finger in front of your nose and look at it with just one eye at a time (without moving your finger), then you'll notice that your finger blocks different parts of the background depending on which eye looks at it The parallactic angle is the angle over which the nearby object seems to move relative to the background In astronomy, the maximum parallactic angle of a star due to the motion of the Earth in its orbit around the Sun is called the star's parallax Because stars are very far away, their parallaxes are very small: the nearest star has a parallax of only 0 76 arcseconds; The apparent difference in position of a body (as the sun, or a star) as seen from some point on the earth's surface, and as seen from some other conventional point, as the earth's center or the sun; An optical illusion that causes a viewed image to apparently change position as the viewer's eye moves to either side of the eyepiece; The difference in appearance in an object when seen from different perspectives The parallax between left and right eye views produces 3-D perception Holograms are unique in providing a wide, continuous range of parallax on the image; The difference in the apparent direction or position of an object when viewed from different points expressed as an angle; The apparent displacement or the difference in apparent direction of an object as seen from two different points not on a straight line with the object (as from two different observing sites on earth); the extent to which objects in the environment move with relation to one another, based on their 3D position and the motion of the observer Position; {i} apparent shifting of position of an object that occurs when an observer changes position (Optics); The way in which an object appears to move against background objects when seen from two different locations See also: parsec; The apparent displacement, or difference of position, of an object, as seen from two different stations, or points of view; The angular difference in apparent direction of an object seen from two different viewpoints; A condition that occurs when the image of the target is not focused precisely on the reticle plane Parallax is visible as an apparent movement between the reticle and the target when the shooter moves his head or, in extreme cases, an out-of-focus image Our centerfire riflescopes under 11 power are factory-set parallax free at 100 yards: rimfire scopes at 50 yards Scopes of 11x or more have a special range focus to adjust for parallax; The apparent shift in the position of a foreground object relative to background objects due to the motion of the observer The parallax is inversely related to the distance Astronomers use the 1 AU baseline of the Earth's orbit to measure the parallax of nearby stars The parallactic angle is half the angular shift of the star on the sky over the course of a year The inverse of the parallax in arcsec is its distance in parsecs; Parallax refers to the apparent shifting of an object when viewed at different angles If you view the same object from two different angles, the perspective will change Hold your thumb out in front of you at arm's length and view it first with your right eye (left eye closed), and then with your left eye (right eye closed) Your thumb appears to move Astronomers view stars from one side of the Earth's orbit and then from the other side to attempt to detect parallax This can be done only for near stars The amount by which the star appears to move gives an indication of its distance Astronomers can also view nearby objects such as the Moon and Venus in this manner to determine distance; The apparent change in position of two objects viewed from different locations; The apparent change in location of a object due to the change in position of the observer Astronomical parallax is measured in seconds of arc; The apparent change in position of a star caused by the annual motion of the earth
parallax second: A unit of length used to measure the distances of stars from Earth, defined as the distance from the Earth of a star that has a parallax of 1 arcsecond. Approximately = 3.08568025 × 1016 meters = 3.2616 light-years
parallax seconds: plural form of parallax second
motion parallax: (Psikoloji, Ruhbilim) A depth cue that results from our motion
geocentric parallax: the parallax of a celestial body using two points on the surface of the earth as the earth rotates
heliocentric parallax: the parallax of a celestial body using two points in the earth's orbit around the sun as the baseline
horizontal parallax: the maximum parallax observed when the celestial body is at the horizon
solar parallax: It is 8
solar parallax: the angle subtended by the mean equatorial radius of the Earth at a distance of one astronomical unit
solar parallax: "80, and is the fundamental datum
solar parallax: The parallax of the sun, that is, the angle subtended at the sun by the semidiameter of the earth
stellar parallax: the heliocentric parallax of a star

parallax

Heceleme

par·al·lax

Türkçe nasıl söylenir

perıläks

Telaffuz

/ˈperəˌlaks/ /ˈpɛrəˌlæks/

Etimoloji

[ 'par-&-"laks ] (noun.) 1580. Middle French parallaxe, from Greek parallaxis, from parallassein to change, from para- + allassein to change, from allos other.

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