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İzahSunspots and Solar Flares.jpg
English: NASA's Solar Dynamics Observatory (SDO) captured this image of an M7.9 class flare on March 13, 2012 at 1:29 p.m. EDT. It is shown here in the 131 Angstrom wavelength, a wavelength particularly good for seeing solar flares and a wavelength that is typically colorized in teal. The flare peaked at 1:41 p.m. EDT. It was from the same active region, No. 1429, that produced flares and coronal mass ejections the entire week. The region has been moving across the face of the sun since March 2, and will soon rotate out of Earth view.
A solar flare is an intense burst of radiation coming from the release of magnetic energy associated with sunspots. Flares are our solar system’s largest explosive events. They are seen as bright areas on the sun and last from mere minutes to several hours.
Scientists classify solar flares according to their x-ray brightness. There are 3 categories: X-, M- and C-class. X-class flares are the largest of these events. M-class flares are medium-sized; they can cause brief radio blackouts that affect Earth's polar regions. Compared to X- and M-class, C-class flares are small with few noticeable consequences on Earth.
ویکیپدیا:گزیدن نگاره برگزیده/Sunspots and Solar Flares.jpg
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Dekabr 18, 2023
fayl, sunspots, solar, flares, fayl, faylın, tarixçəsi, fayl, keçidləri, faylın, qlobal, istifadəsisınaq, göstərişi, ölçüsü, piksel, digər, ölçülər, piksel, piksel, piksel, piksel, piksel, piksel, faylın, orijinalı, 8206, piksel, fayl, həcmi, mime, növü, image. Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesiSinaq gosterisi olcusu 600 600 piksel Diger olculer 240 240 piksel 480 480 piksel 768 768 piksel 1 024 1 024 piksel 2 048 2 048 piksel 4 096 4 096 piksel Faylin orijinali 8206 4 096 4 096 piksel fayl hecmi 6 5 MB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler tesvir sehifesi Faylin tesvir sehifesine get Xulase IzahSunspots and Solar Flares jpg English NASA s Solar Dynamics Observatory SDO captured this image of an M7 9 class flare on March 13 2012 at 1 29 p m EDT It is shown here in the 131 Angstrom wavelength a wavelength particularly good for seeing solar flares and a wavelength that is typically colorized in teal The flare peaked at 1 41 p m EDT It was from the same active region No 1429 that produced flares and coronal mass ejections the entire week The region has been moving across the face of the sun since March 2 and will soon rotate out of Earth view A solar flare is an intense burst of radiation coming from the release of magnetic energy associated with sunspots Flares are our solar system s largest explosive events They are seen as bright areas on the sun and last from mere minutes to several hours Scientists classify solar flares according to their x ray brightness There are 3 categories X M and C class X class flares are the largest of these events M class flares are medium sized they can cause brief radio blackouts that affect Earth s polar regions Compared to X and M class C class flares are small with few noticeable consequences on Earth Image Credit NASA Tarix 13 mart 2012 Menbe http www nasa gov multimedia imagegallery image feature 2201 html Muellif NASA Lisenziya Public domain Public domain false false This file is in the public domain in the United States because it was solely created by NASA NASA copyright policy states that NASA material is not protected by copyright unless noted See Template PD USGov NASA copyright policy page or JPL Image Use Policy Warnings Use of NASA logos insignia and emblems is restricted per U S law 14 CFR 1221 The NASA website hosts a large number of images from the Soviet Russian space agency and other non American space agencies These are not necessarily in the public domain Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI 1 See also PD Hubble and Cc Hubble The SOHO ESA amp NASA joint project implies that all materials created by its probe are copyrighted and require permission for commercial non educational use 2 Images featured on the Astronomy Picture of the Day APOD web site may be copyrighted 3 The National Space Science Data Center NSSDC site has been known to host copyrighted content Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain Unless otherwise noted CaptionsazerbaycancaAdd a one line explanation of what this file representsItems portrayed in this filetesvir ediryaranma tarixi13 mart 2012MIME type nbsp ingilisimage jpeg Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki14 03 20 mart 20124 096 4 096 6 5 MB Dipankan001 Fayl kecidleri Bu sekile olan kecidler Gunes Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur ar wikipedia org layihesinde istifadesi الشمس ca wikipedia org layihesinde istifadesi Sol en wikipedia org layihesinde istifadesi User Jonathan Chone eu wikipedia org layihesinde istifadesi Eguzkia fa wikipedia org layihesinde istifadesi خورشید ویکی پدیا گزیدن نگاره برگزیده Sunspots and Solar Flares jpg hi wikipedia org layihesinde istifadesi स र य hi wikiversity org layihesinde istifadesi स र म डल स र य ka wikipedia org layihesinde istifadesi მზე km wikipedia org layihesinde istifadesi ព រ អ ទ ត យ no wikipedia org layihesinde istifadesi Solen pl wikipedia org layihesinde istifadesi Slonce Wikiprojekt Tlumaczenie artykulow Slonce ro wikipedia org layihesinde istifadesi Soare simple wikipedia org layihesinde istifadesi User JonathanHopeThisIsUnique Sandbox sq wikipedia org layihesinde istifadesi Dielli sv wikipedia org layihesinde istifadesi Solen Menbe https az wikipedia org wiki Fayl Sunspots and Solar Flares jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,
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