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Etymology: [ &-'rOr-&, o-, -'ror- ] (noun.) 14th century. From Latin aurora "dawn".

Aurora borealis: kuzey yarımkürede geceleri gökyüzünde görülen renkli ışıklar, seher, (isim) Güneşteki fırtınalar sonucu meydana gelip kutuplarda geceleri görülen renkli ve hareket eden ışıklar, (mit) seher tanrıçası, Auroral: (sıfat) güneşin doğuşuna ait; kutupsal ışıklara ait, Güneşteki fırtınalar sonucu meydana gelip kutuplarda geceleri görülen renkli ve hareket eden ışıklar, Aurora australis: Güney yarımkürede geceleri gökyüzünde görülen renkli ışıklar, (isim) Seher tanrıçası, şafak tanrıçası [mit.], (isim) şafak tanrıçası [mit.], tan, şafak, Şafak tanrıçası, Eos'un latince adı. Şafak tanrıçası, seher vakti, seher tanrıçası, fecir, TAN KIZILLIĞI:Arz manyetik alanındaki partiküller gibi hareket halinde bulunan ve arzın atmosferiyle etkilenen, çoğunlukla protonlardan oluşan güneş partiküllerinin sebep olduğu, yüksek irtifadaki hava kızıllığı, aurora, aurora australis güney yarımkürede geceleri gökyüzünde görülen renkli, tulu, doğuş, Auroralar, auroras,

1 Aurora borealis: kuzey yarımkürede geceleri gökyüzünde görülen renkli ışıklar     ts
2 seher     ts
3 (isim) Güneşteki fırtınalar sonucu meydana gelip kutuplarda geceleri görülen renkli ve hareket eden ışıklar     ts
4 (mit) seher tanrıçası     ts
5 Auroral: (sıfat) güneşin doğuşuna ait; kutupsal ışıklara ait     ts
6 Güneşteki fırtınalar sonucu meydana gelip kutuplarda geceleri görülen renkli ve hareket eden ışıklar     ts
7 Aurora australis: Güney yarımkürede geceleri gökyüzünde görülen renkli ışıklar     ts
8 (isim) Seher tanrıçası     ts
9 şafak tanrıçası [mit.]  isim     ts
10 (isim) şafak tanrıçası [mit.]     ts
11 tan     ts
12 şafak     ts
13 Şafak tanrıçası     ts
14 Eos'un latince adı. Şafak tanrıçası  Mitoloji     ts
15 seher vakti  Havacılık     ts
16 seher tanrıçası     ts
17 fecir     ts
18 TAN KIZILLIĞI:Arz manyetik alanındaki partiküller gibi hareket halinde bulunan ve arzın atmosferiyle etkilenen, çoğunlukla protonlardan oluşan güneş partiküllerinin sebep olduğu, yüksek irtifadaki hava kızıllığı  Askeri     ts
19 aurora     ts
20 aurora australis güney yarımkürede geceleri gökyüzünde görülen renkli     ts
21 tulu     ts
22 doğuş     ts
23auroras Auroralar     ts
24aurorae auroras     ts
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Güneşin etkinliği sonucu atmosfere girip, yerin manyetik alanıyla etkileşimde bulunan yüklü parçacıkların oluşturduğu bir ışıma,

25 Güneşin etkinliği sonucu atmosfere girip, yerin manyetik alanıyla etkileşimde bulunan yüklü parçacıkların oluşturduğu bir ışıma     ts
 

A female given name, in quiet but regular use since the 19th century, Roman goddess of the dawn, An atmospheric phenomenon created by charged particles from the sun striking the upper atmosphere, creating coloured lights in the sky. It is usually named australis or borealis based on whether it is in the southern or northern hemispheres respectively, in quiet but regular use since the 19th century, observations, in Roman mythology, the goddess of the dawn (=the beginning of the day when light first appears) . In Greek mythology her name is Eos. City (pop., 2000: 276,393), northern central Colorado, U.S. It was founded near Denver during the silver boom of 1891 and named Fletcher; it was incorporated and renamed in 1907. Though mainly residential, it is also the site of Buckley Air National Guard Base. Roman goddess of dawn. Her Greek counterpart was Eos. Hesiod described her as the daughter of the Titans Hyperion and Theia. She was the sister of Helios, the sun, and Selene, the moon. By the Titan Astraeus, she became the mother of the winds and of the evening star. In Greek mythology she was also represented as the lover of the hunters Cephalus and Orion. Luminous phenomenon of the upper atmosphere that occurs primarily at high latitudes. Auroras in the Northern Hemisphere are called aurora borealis, or northern lights; in the Southern Hemisphere they are called aurora australis, or southern lights. Auroras are caused by the interaction of energetic particles (electrons and protons) from outside the atmosphere with atoms of the upper atmosphere. Such interaction occurs in zones surrounding the Earth's magnetic poles. During periods of intense solar activity, auroras occasionally extend to the middle latitudes, goddess of the dawn (Roman Mythology); Eos, goddess of the dawn (Greek Mythology),   Sporadic radiant emission from the upper atmosphere that usually occurs about the North and South magnetic poles of the Earth   Note 1:  Auroras are most intense at times of intense magnetic storms caused by sunspot activity   The distribution of auroral intensity with altitude shows a pronounced maximum near 100 km above the Earth   Auroras may occasionally be observed within 40° or less of the equator   Note 2:  Auroras interfere with radio communications   Note 3:  In the Northern hemisphere, the aurora is called the Aurora Borealis (Northern Lights)   In the Southern hemisphere, the aurora is called the Aurora Australis (Southern Lights), Light emitted from the polar upper atmosphere as energetic electrons bombard it from space Aurora is another name for polar lights The aurora borealis (northern lights) and aurora australis (southern lights) occur most frequently in the auroral oval, (Roman mythology) goddess of the dawn; counterpart of Greek Eos an atmospheric phenomenon consisting of bands of light caused by charged solar particles following the earth's magnetic lines of force,   Sporadic radiant emission from the upper atmosphere that usually occurs about the North and South magnetic poles of the Earth   Note 1:  Auroras are most intense at times of intense magnetic storms caused by sunspot activity   The distribution of auroral intensity with altitude shows a pronounced maximum near 100 km above the Earth   Auroras may occasionally be observed within 40° or less of the equator   Note 2:  Auroras interfere with radio communications   Note 3:  In the Northern hemisphere, the aurora is called the Aurora Borealis (Northern Lights)   In the Southern hemisphere, the aurora is called the Aurora Australis (Southern Lights), The aurora borealis or aurora australis (northern or southern lights), Sporadic visible emission in the upper atmosphere most prominent at high latitudes in both hemispheres caused by an influx of atomic particles from the Sun, Glows seen over the polar regions which occur when energized particles from the Sun react with particles from the Earth, The rising light of the morning; the dawn of day; the redness of the sky just before the sun rises, The glowing light from solar particles interact with Earth's magnetic field, The rise, dawn, or beginning, The Roman personification of the dawn of day; the goddess of the morning, The poets represented her a rising out of the ocean, in a chariot, with rosy fingers dropping gentle dew, A species of crowfoot, (a) The Northern (or Southern) Lights, a display of brightly coloured lights seen by observers near the Earth's poles due to the excitation of molecules in the Earth's atmosphere by the energetic particles in the solar wind (b) Goblin fireworks Earth is particularly famed as a provider of beautiful displays due to the abundance of nitrogen and oxygen in its atmosphere, which produce the red and green colours, A glow in a planet's ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun This phenomenon is known as the Aurora Borealis in the Earth's northern hemisphere and the Aurora Australis in the Earth's Southern Hemisphere, a glow in a planets ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun, A display of colored light given off by collisions between charged particles trapped in a planet's magnetic fields and atoms of atmospheric gases near the planet's magnetic poles Aurora are visible on Earth as the aurora borealis or northern lights and the aurora australis or southern lights more!, (Latin for "dawn") a glow in a planet's ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun, a glow in a planet's ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun, the first light of day; "we got up before dawn"; "they talked until morning", an atmospheric phenomenon consisting of bands of light caused by charged solar particles following the earth's magnetic lines of force, (Roman mythology) goddess of the dawn; counterpart of Greek Eos, luminous atmospheric phenomenon (aurora australis and aurora borealis), A glow in the Earth's ionosphere caused by the interaction between the Earth's magnetic field and charged particles from the Sun (The Solar Wind) It gives rise to the "Northern Lights", or Aurora Borealis, in the Northern Hemisphere, and the Aurora Australis in the Southern Hemisphere, A glow in the sky, seen often in a ring-shaped region around the magnetic poles ("auroral zone") and occasionally further equatorward The name comes from an older one, "Aurora Borealis", Latin for "northern dawn," given because an aurora near the northern horizon (its usual location when seen in most of Europe) looks like the glow of the sky preceding sunrise Also known as "northern lights", although it occurs both north and south (Aurora Australis) of the equator The aurora is generally caused by fast electrons from space, guided earthward by magnetic field lines, and its light comes from collisions between such electrons and the atoms of the upper atmosphere, typically 100 km above ground, (short for polar aurora)--A glow in the sky, often observed in a ring-shaped region around the magnetic poles ("auroral zone") and occasionally further equatorward The name comes from an older one, "aurora borealis," Latin for "northern dawn," given because an aurora near the northern horizon (its usual location when seen in most of Europe) looks like the glow of the sky preceding sunrise Also known as "northern lights," although it occurs both north and south of the equator The aurora is generally caused by fast electrons from space, guided earthward by magnetic field lines, and its light comes from collisions between such electrons and the atoms of the upper atmosphere, typically 100 km (60 miles) above ground, A faint visual phenomenon associated with geomagnetic activity, occurring mainly in the high-latitude night sky Typical auroras occur 100 to 250 km above the ground as high speed particles from the solar wind collide with atmospheric gasses at these altitudes When observed in the northern hemisphere this phenomena is known as the Aurora Borealis (northern lights), and when viewed in the southern hemisphere it is the Aurora Australis, A light-releasing phenonemon that occurs in the upper reaches of a planet’s atmosphere Caused by the interaction of the atmosphere with energetic particles from the Sun Electrons from the Sun follow the planet’s magnetic field lines toward its poles, where this phenomenon generally occurs, A faint visual (optical) phenomenon on the Earth associated with geomagnetic activity, which occurs mainly in the high-latitude night sky Typical auroras are 100 to 250 km above the ground The Aurora Borealis occurs in the northern hemisphere and the Aurora Australis occurs in the southern hemisphere, The bright emission of atoms and molecules in the polar upper atmosphere that appears as permanent, ring shaped belts called the auroral oval around the north and south geomagnetic poles It is associated with a global electrical discharge process caused by energetic particles impinging on the upper atmosphere of Earth See also: Auroras: Billboards for Electric Space, Excitation of particles from the sun spiralling in the geomagnetic field near the poles resulting in the release of energy in different forms, including light, It is created by the radiant energy emission from the sun and its interaction with the earth's upper atmosphere over the middle and high latitudes It is seen as a bright display of constantly changing light near the magnetic poles of each hemisphere In the Northern Hemisphere, it is known as the aurora borealis or Northern Lights, and in the Southern Hemisphere, this phenomena is called the aurora australis, It is created by the sporadic radiant energy emission from the sun and its interaction with the earth's upper atmosphere over the middle and high latitudes It is seen as a bright display of constantly changing light near the magnetic poles of each hemisphere In the Northern Hemisphere, it is known as the aurora borealis or Northern Lights, and in the Southern Hemisphere, this phenomena is called the aurora australis, plural of aurora,

26 A female given name, in quiet but regular use since the 19th century     ts
27 Roman goddess of the dawn     ts
28 An atmospheric phenomenon created by charged particles from the sun striking the upper atmosphere, creating coloured lights in the sky. It is usually named australis or borealis based on whether it is in the southern or northern hemispheres respectively     ts
29 in quiet but regular use since the 19th century     ts
30 observations     ts
31 in Roman mythology, the goddess of the dawn (=the beginning of the day when light first appears) . In Greek mythology her name is Eos. City (pop., 2000: 276,393), northern central Colorado, U.S. It was founded near Denver during the silver boom of 1891 and named Fletcher; it was incorporated and renamed in 1907. Though mainly residential, it is also the site of Buckley Air National Guard Base. Roman goddess of dawn. Her Greek counterpart was Eos. Hesiod described her as the daughter of the Titans Hyperion and Theia. She was the sister of Helios, the sun, and Selene, the moon. By the Titan Astraeus, she became the mother of the winds and of the evening star. In Greek mythology she was also represented as the lover of the hunters Cephalus and Orion. Luminous phenomenon of the upper atmosphere that occurs primarily at high latitudes. Auroras in the Northern Hemisphere are called aurora borealis, or northern lights; in the Southern Hemisphere they are called aurora australis, or southern lights. Auroras are caused by the interaction of energetic particles (electrons and protons) from outside the atmosphere with atoms of the upper atmosphere. Such interaction occurs in zones surrounding the Earth's magnetic poles. During periods of intense solar activity, auroras occasionally extend to the middle latitudes     ts
32 goddess of the dawn (Roman Mythology); Eos, goddess of the dawn (Greek Mythology)  isim     ts
33   Sporadic radiant emission from the upper atmosphere that usually occurs about the North and South magnetic poles of the Earth   Note 1:  Auroras are most intense at times of intense magnetic storms caused by sunspot activity   The distribution of auroral intensity with altitude shows a pronounced maximum near 100 km above the Earth   Auroras may occasionally be observed within 40° or less of the equator   Note 2:  Auroras interfere with radio communications   Note 3:  In the Northern hemisphere, the aurora is called the Aurora Borealis (Northern Lights)   In the Southern hemisphere, the aurora is called the Aurora Australis (Southern Lights)     ts
34 Light emitted from the polar upper atmosphere as energetic electrons bombard it from space Aurora is another name for polar lights The aurora borealis (northern lights) and aurora australis (southern lights) occur most frequently in the auroral oval     ts
35 (Roman mythology) goddess of the dawn; counterpart of Greek Eos an atmospheric phenomenon consisting of bands of light caused by charged solar particles following the earth's magnetic lines of force     ts
36   Sporadic radiant emission from the upper atmosphere that usually occurs about the North and South magnetic poles of the Earth   Note 1:  Auroras are most intense at times of intense magnetic storms caused by sunspot activity   The distribution of auroral intensity with altitude shows a pronounced maximum near 100 km above the Earth   Auroras may occasionally be observed within 40° or less of the equator   Note 2:  Auroras interfere with radio communications   Note 3:  In the Northern hemisphere, the aurora is called the Aurora Borealis (Northern Lights)   In the Southern hemisphere, the aurora is called the Aurora Australis (Southern Lights)     ts
37 The aurora borealis or aurora australis (northern or southern lights)     ts
38 Sporadic visible emission in the upper atmosphere most prominent at high latitudes in both hemispheres caused by an influx of atomic particles from the Sun     ts
39 Glows seen over the polar regions which occur when energized particles from the Sun react with particles from the Earth     ts
40 The rising light of the morning; the dawn of day; the redness of the sky just before the sun rises     ts
41 The glowing light from solar particles interact with Earth's magnetic field     ts
42 The rise, dawn, or beginning     ts
43 The Roman personification of the dawn of day; the goddess of the morning     ts
44 The poets represented her a rising out of the ocean, in a chariot, with rosy fingers dropping gentle dew     ts
45 A species of crowfoot     ts
46 (a) The Northern (or Southern) Lights, a display of brightly coloured lights seen by observers near the Earth's poles due to the excitation of molecules in the Earth's atmosphere by the energetic particles in the solar wind (b) Goblin fireworks Earth is particularly famed as a provider of beautiful displays due to the abundance of nitrogen and oxygen in its atmosphere, which produce the red and green colours     ts
47 A glow in a planet's ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun This phenomenon is known as the Aurora Borealis in the Earth's northern hemisphere and the Aurora Australis in the Earth's Southern Hemisphere     ts
48 a glow in a planets ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun     ts
49 A display of colored light given off by collisions between charged particles trapped in a planet's magnetic fields and atoms of atmospheric gases near the planet's magnetic poles Aurora are visible on Earth as the aurora borealis or northern lights and the aurora australis or southern lights more!     ts
50 (Latin for "dawn") a glow in a planet's ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun     ts
51 a glow in a planet's ionosphere caused by the interaction between the planet's magnetic field and charged particles from the Sun     ts
52 the first light of day; "we got up before dawn"; "they talked until morning"     ts
53 an atmospheric phenomenon consisting of bands of light caused by charged solar particles following the earth's magnetic lines of force     ts
54 (Roman mythology) goddess of the dawn; counterpart of Greek Eos     ts
55 luminous atmospheric phenomenon (aurora australis and aurora borealis)  isim     ts
56 A glow in the Earth's ionosphere caused by the interaction between the Earth's magnetic field and charged particles from the Sun (The Solar Wind) It gives rise to the "Northern Lights", or Aurora Borealis, in the Northern Hemisphere, and the Aurora Australis in the Southern Hemisphere     ts
57 A glow in the sky, seen often in a ring-shaped region around the magnetic poles ("auroral zone") and occasionally further equatorward The name comes from an older one, "Aurora Borealis", Latin for "northern dawn," given because an aurora near the northern horizon (its usual location when seen in most of Europe) looks like the glow of the sky preceding sunrise Also known as "northern lights", although it occurs both north and south (Aurora Australis) of the equator The aurora is generally caused by fast electrons from space, guided earthward by magnetic field lines, and its light comes from collisions between such electrons and the atoms of the upper atmosphere, typically 100 km above ground     ts
58 (short for polar aurora)--A glow in the sky, often observed in a ring-shaped region around the magnetic poles ("auroral zone") and occasionally further equatorward The name comes from an older one, "aurora borealis," Latin for "northern dawn," given because an aurora near the northern horizon (its usual location when seen in most of Europe) looks like the glow of the sky preceding sunrise Also known as "northern lights," although it occurs both north and south of the equator The aurora is generally caused by fast electrons from space, guided earthward by magnetic field lines, and its light comes from collisions between such electrons and the atoms of the upper atmosphere, typically 100 km (60 miles) above ground     ts
59 A faint visual phenomenon associated with geomagnetic activity, occurring mainly in the high-latitude night sky Typical auroras occur 100 to 250 km above the ground as high speed particles from the solar wind collide with atmospheric gasses at these altitudes When observed in the northern hemisphere this phenomena is known as the Aurora Borealis (northern lights), and when viewed in the southern hemisphere it is the Aurora Australis     ts
60 A light-releasing phenonemon that occurs in the upper reaches of a planet’s atmosphere Caused by the interaction of the atmosphere with energetic particles from the Sun Electrons from the Sun follow the planet’s magnetic field lines toward its poles, where this phenomenon generally occurs     ts
61 A faint visual (optical) phenomenon on the Earth associated with geomagnetic activity, which occurs mainly in the high-latitude night sky Typical auroras are 100 to 250 km above the ground The Aurora Borealis occurs in the northern hemisphere and the Aurora Australis occurs in the southern hemisphere     ts
62 The bright emission of atoms and molecules in the polar upper atmosphere that appears as permanent, ring shaped belts called the auroral oval around the north and south geomagnetic poles It is associated with a global electrical discharge process caused by energetic particles impinging on the upper atmosphere of Earth See also: Auroras: Billboards for Electric Space     ts
63 Excitation of particles from the sun spiralling in the geomagnetic field near the poles resulting in the release of energy in different forms, including light     ts
64 It is created by the radiant energy emission from the sun and its interaction with the earth's upper atmosphere over the middle and high latitudes It is seen as a bright display of constantly changing light near the magnetic poles of each hemisphere In the Northern Hemisphere, it is known as the aurora borealis or Northern Lights, and in the Southern Hemisphere, this phenomena is called the aurora australis     ts
65 It is created by the sporadic radiant energy emission from the sun and its interaction with the earth's upper atmosphere over the middle and high latitudes It is seen as a bright display of constantly changing light near the magnetic poles of each hemisphere In the Northern Hemisphere, it is known as the aurora borealis or Northern Lights, and in the Southern Hemisphere, this phenomena is called the aurora australis     ts
66aurorae plural of aurora     ts
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aurora,

67 aurora     ts
 


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Sözlük . Dictionary . Wörterbuch . λεξικό . Diccionario . 字典 . словарь . Dictionnaire . القاموس . Dizionario . מילון . Matokeo . واژه نامه . 辞書
Some etymologies, pronunciations, function and usage date content for the English translation portion are from Merriam-Webster Online at www.Merriam-Webster.com. Thanks to Online Yunanca Dil Eğitimi for providing some parts of online greek dictionary. To contribute more resources please contact us. Visuals(images) are provided by Google Image Search API. Some parts of the dictionary is contributed by many users, thank you! The content on this site is for informational purposes only. Bu aramada Aurora kelimesinin sözlük anlamı ve eşanlamı nedir, nasıl okunur hakkında bilgi verilmektedir. Aurora kelimesinin etimolojik ve eşanlamları ile ilgili açıklamalar ve bilgiler eksiksiz ve hatasız olarak anılmamalıdır. Burada yer alan Aurora kelimesi ile ilgili tüm açıklamalar bilgi amaçlıdır. Eksik ve hatalı çevirileri lütfen bildiriniz.

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