This animated series that i have been following since in form 1.hohoho.it's a very long time.i started followed with the manga but i only started to followed their animated series last year.last year,i already dowloaded more than 360 episodes.and i already finished watching all the episodes in the same year.haha.i'm crazy about this anime dude.this anime is crazy.their main characters,i can't tell you.they all cool.yohoho.i wonder,when this anime will finish because i can't wait any much longer.wahahahaha. Tiada apa yang menarik tentang diriku kerana aku menjalani kehidupan seharian sepertimana manusia-manusia lain lakukan untuk terus hidup.makan nasi kalau lapar minum air kalau haus.tetapi aku sentiasa belajar untuk terus hidup di bumi yang nyata ini dan juga belajar tentang kehidupan.Belajar tentang segalanya kerana belajar adalah sesuatu yang general.meminati musik yang berat,laju dan sedikit berkarat tetapi mesti rock!!ya.rock.kerana kita perlu sentiasa rock.haha.and I'm the lucky person who survived in this violent piece land of shit!!!
Aurora is a natural display of light in the sky, usually limited to Earth’s polar regions. Auroras can be seen with the unaided eye only at night. They commonly appear as arcs, clouds, and bands of moving light that can extend across the sky for thousands of miles.
![Anime kita hidup di bumi ini 2 Anime kita hidup di bumi ini 2](/uploads/1/2/5/3/125364104/655922766.jpg)
An auroral display in the Northern Hemisphere is called the aurora borealis or northern lights. An auroral display in the Southern Hemisphere is called the aurora australis.Kawartha Lake, South Ontario, Kanada, Monday (23/2)Most auroras occur about 60 to 250 miles (100 to 400 kilometers) above Earth. The most common color in an aurora is green, but displays that occur extremely high in the sky may be red or purple. Auroras result in part from Earth’s magnetic field, the area of magnetic influence that surrounds the planet.
![Kita Kita](https://scontent-arn2-1.cdninstagram.com/vp/14cb2f3b863e3c11b2c4eaa5f03f73b3/5D8DA779/t51.2885-15/e35/60239151_147678189617196_3070317351616135211_n.jpg?_nc_ht=scontent-arn2-1.cdninstagram.com&se=7&ig_cache_key=MjA1MjU1MjUwMDAzNzY0NzI2NQ%3D%3D.2)
The magnetic field dominates a region of space called the magnetosphere. Above the atmosphere, the magnetosphere contains neutral and charged particles. The charged particles are produced when the atmosphere absorbs radiation from the sun.The magnetosphere is continuously buffeted by a flow of electrically charged particles from the sun, called the solar wind. This buffeting squeezes the magnetosphere and causes the charged particles already in the magnetosphere to move along the magnetic field toward the North and South poles. There, the energetic particles collide with particles in the atmosphere, releasing energy in the form of light.The terrestrial magnetic shield acts as a barrier, protecting the Earth from energetic particles and radiation in the hot solar wind. Most of these energetic particles are deflected around the Earth by the magnetosphere, but some get trapped.
Mencari tahu 'untuk apa kita ada dibumi ini' so, jalani hidup ini sesuai petunjuk, petunjuk dari KITAB dan para pemuka Agama, sehingga mengetahui mana yang diperbolehkan maupun yang tidak diperbolehkan, pelajari, pahami dan implementasikannya dalam kehidupan sehari-hari, selanjutnya, biar yang MAHA KUASA yang menentukan hasilnya. Maka kita akan tahu bahwa menit-menit, hari-hari, minggu-minggu bahkan tahun-tahun yang kita jalani di dalam kehidupan ini adalah waktu yang menentukan kekekalan. Kekekalan itu adalah tentang bagaimana kelak kita akan berada, apakah di sorga yang kekal ataukah di neraka. Itu semua berdasarkan kepada perbuatan kita selama kita hidup di bumi ini.
Electrons trapped in the Earth’s magnetic field are accelerated along the magnetic field toward the polar regions and then strike the atmosphere to form the aurora.The particles, which stream down the magnetic field of the Earth, reach the neutral atmosphere in a rough circle called the auroral oval. This circle, or annulus, is centered over the magnetic pole and is around 3000 km in diameter during quiet times. The annulus grows larger when the magnetosphere is disturbed. The location of the auroral oval is generally found between 60 and 70 degrees north and south latitude (fig. 3).Auroral features come in many shapes and sizes.
Tall arcs and rays start brightly 100 km above the Earth’s surface and extend upward along its magnetic field for hundreds of km. These arcs or curtains can be as thin as 100 meters while extending from horizon to horizon. Auroral arcs can nearly stand still and then, as though a hand has been run along a tall curtain, the aurora will begin to dance and turn. After midnight, the aurora can take on a patchy appearance and the patches often blink on and off once every 10 seconds or so until dawn. Most of the auroral features are greenish yellow but sometimes the tall rays will turn red at their tops and along their lower edge.
On rare occasions, sunlight will hit the top part of the auroral rays creating a faint blue color. On very rare occasions (once every 10 years or so) the aurora can be a deep blood red color from top to bottom. In addition to producing light, the energetic auroral particles deposit heat.
The heat is dissipated by infrared radiation or transported away by strong winds in the upper atmosphere.The Chemistry of the AuroraThe aurora is caused by the interaction of highenergy particles (usually electrons) with neutral atoms in the Earth’s upper atmosphere. These high-energy particles can “excite” (by collisions) valence electrons that are bound to the neutral atom. The excited electrons can then return to their initial, lower energy state, and in the process release photons (light particles). This process is similar to the discharge in a neon. lamp (fig.
4).Any particular color of the aurora depends on a specific atmospheric gas and its electrical state, and on the energy of the particle that hits the atmospheric gas. Atomic oxygen is responsible for the two main colors of green (wavelength of 557.7 nm) and red (630.0 nm).Auroras are most intense during solar maximum, the most active phase in the 11-year sunspot cycle.
During this period, violent eruptions on the sun’s surface occur most frequently. These eruptions are known as solar flares and coronal mass ejections. They release additional material into the solar wind. The added material helps compress Earth’s magnetosphere, producing extremely bright auroras. It also creates sharp variations in Earth’s magnetic field, called magnetic storms. During these storms, auroras may expand toward the equator, making them visible beyond the polar regions.