(Askeri) 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
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
(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
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
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
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
(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
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
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
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
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 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
 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)
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!
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
A light-releasing phenonemon that occurs in the upper reaches of a planets atmosphere Caused by the interaction of the atmosphere with energetic particles from the Sun Electrons from the Sun follow the planets magnetic field lines toward its poles, where this phenomenon generally occurs
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
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
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
(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