Solar_Spectrum.png(800 × 595 พิกเซล, ขนาดไฟล์: 36 กิโลไบต์, ชนิดไมม์: image/png)
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วันที่/เวลา | รูปย่อ | ขนาด | ผู้ใช้ | ความเห็น | |
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ปัจจุบัน | 16:24, 25 สิงหาคม 2550 | 800 × 595 (36 กิโลไบต์) | Transwiki approved by: w:en:User:Dmcdevit This image was copied from wikipedia:en. The original description was: == Description == This figure shows the w:en:solar radiation spectrum for direct w:en:light at both the top of the [[w:en:Earth |
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ifl prawtiifl hnathimiphaphni karichiflkhamokhrngkar khxmulekiywkbphaphimmiphaphthimiraylaexiydsungkwani Solar Spectrum png 800 595 phikesl khnadifl 36 kiolibt chnidimm image png rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khwamyx khaxthibaySolar Spectrum png aekikh hakepnipidchwyihthukkhnsamarthekhathungkhaxthibayniidodyaeplepnphasaxun khxbkhun Cestina Tento obrazek ukazuje spektrum slunecniho zareni pro prime svetlo jednak na horni hranici zemske atmosfery reprezentovane zlutou oblasti tak na hladine more cervena oblast Slunce produkuje svetlo s distribuci podobnou tomu co by se dalo ocekavat od cerneho telesa o teplote 5778 K 5505 C coz je priblizne povrchova teplota slunce Jak svetlo prochazi atmosferou cast je absorbovana plyny se specifickymi absorpcnimi pasy Dalsi svetlo je redistribuovano Rayleighovym rozptylem ktery je zodpovedny za modrou barvu atmosfery Tyto krivky jsou zalozeny na terestrickem referencnim spektru Americke spolecnosti pro testovani a materialy American Society for Testing and Materials ASTM coz jsou standardy prijate fotovoltaickym prumyslem ktere zajistuji konzistentni zkusebni podminky a jsou podobne svetlu ktere lze ocekavat v Severni Americe Zobrazuji se oblasti pro ultrafialove viditelne a infracervene svetlo English This figure shows the solar radiation spectrum for direct light at both the top of the Earth s atmosphere represented by the area in yellow and at sea level area in red The sun produces light with a distribution similar to what would be expected from a 5525 K 5250 C blackbody which is approximately the sun s surface temperature As light passes through the atmosphere some is absorbed by gases with specific absorption bands Additional light is redistributed by Rayleigh scattering which is responsible for the atmosphere s blue color These curves are based on NREL data for above the atmosphere and at sea level which are standards adopted by the photovoltaics industry to ensure consistent test conditions and are similar to the light that could be expected in North America Regions for ultraviolet visible and infrared light are indicated Espanol La figura muestra el espectro de radiacion solar de luz directa tanto arriba de la atmosfera de la Tierra representada por el area en amarillo como al nivel del mar area en rojo El sol produce luz con una distribucion similar a la que se esperaria de un cuerpo negro a 5525 K 5250 C que es latemperatura aproximada de la superficie del Sol Conforme la luz pasa a traves de la atmosfera parte de la luz es absorbida por gases en bandas de absorcion especificas Luz adicional se redistribuye por dispersion de Rayleigh la cual es responsable por el color azul de la atmosfera Estas curvas estan basadas en datos del NREL arriba de la atmosfera y al nivel del mar los cuales son estandares adoptados por la industria fotovoltaica para asegurar condiciones de prueba consistentes y son similares a la luz que se podria esperar en Norte America Se indican las regiones de luz ultravioleta visible e infrarroja Francais Cette figure montre le spectre solaire pour la lumiere directe a la limite superieure de l atmosphere terrestre representee par la zone jaune et au niveau de la mer zone rouge Le Soleil produit une lumiere dont la distribution est similaire a celle que l on attendrait d un corps noir a 5778 K 5505 C ce qui correspond approximativement a la temperature de surface du Soleil Lorsque la lumiere traverse l atmosphere une partie est absorbee par des gaz presentant des bandes d absorption specifiques D autres rayons sont redistribues par la diffusion de Rayleigh ce qui explique la couleur bleue de l atmosphere Ces courbes sont basees sur le spectre terrestre de reference de l American Society for Testing and Materials ASTM Il s agit de normes adoptees par l industrie photovoltaique pour garantir des conditions d essai coherentes et similaires a la lumiere a laquelle on peut s attendre en Amerique du Nord Les zones de lumiere ultraviolette visible et infrarouge sont indiquees Italiano La figura mostra lo spettro della radiazione solare per illuminazione diretta sia all inizio che alla fine del atmosfera terrestra Il sole produce una luce con una distribuzione simile a quella che ci si attenderebbe da un corpo nero a 5525 K 5250 C che e approssimativamente la temperatura superficiale del sole A mano a mano che la luce passa attraverso l atmosfera parte della radiazione e assorbita dai gas in specifiche bande di assorbimento Un contributo additivo e dovuto allo scattering Raleigh che e responsabile per il colore blu dell atmosfera Le curve sono basate sugli spettri di riferimento dell American Society for Testing and Materials ASTM che sono standard adottati dall industria fotovoltaica per assicurare condizioni di prova consistenti e sono simili al tipo di radiazione che e possibile aspettarsi nell America del nord Sono indicate le regioni per l ultravioletto il visibile e la luce infrarossaPolski Rozklad widmowy promieniowania slonecznego Portugues A figua mostra o espectro da radiacao solar direta tanto na parte mais alta da atmosfera terrestre representado pela area em amarelo como ao nivel do mar area em vermelho O Sol emite radiacao com uma distribuicao similar ao que seria esperado de um corpo negro a 5778 K 5505 C que e a temperatura aproximada da superficie do Sol A medida que a luz passa pela atmosfera terrestre parte dela e absorvida por gases com bandas de absorcao especificas A luz tambem e redistribuida por meio do fenomeno conhecido como Dispersao de Rayleigh responsavel pela cor azul da atmosfera As curvas do grafico sao baseadas no Espectro de Referencia Terrestre da American Society for Testing and Materials ASTM que sao padroes utilizados pela industria de fotovoltaicos para garantir condicoes de ensaio consistentes portanto as curvas sao similares ao espectro esperado na America do Norte Regioes para luz ultravioleta visivel e infravermelha estao indicadas עברית nbsp ספקטרום השמש מעל האטמוספירה ובגובה פני היםالعربية nbsp طيف الشمس المأخوذ بالقمر الصناعي أصفر وعلى الأرض أحمر بالمقارنة بطيف الجسم الأسود ينطبق طيف القمر الصناعي مع النظرية ويتخلل طيف الشمس المأخوذ علي الأرض بعض الفجوات الناتجة عن امتصاص جو الأرض لبعض ترددات الأشعة wnthi 9 tulakhm ph s 2551 aehlngthima ngankhxngtw phusrangsrrkh Robert A Rohde ewxrchnxun phaphnimiphaphinrupaebbewketxr SVG hakphaph SVG thaihkaraesdngphldikwa hnathiichphaphnikhwrepliynipichphaph SVG aethn File Solar Spectrum png File Solar spectrum en svg sahrbkhxmulephimetimekiywkbphaphewketxr duthi karepliynipichphaph SVG inkhxmmxns nxkcaknisamarthduephimetimekiywkb khxmulekiywkbkarrxngrbphaph SVG sahrbsxftaewrmiediywiki id inphasaxun Alemannisch nbsp Bahasa Indonesia nbsp Bahasa Melayu nbsp British English nbsp catala nbsp cestina nbsp dansk nbsp Deutsch nbsp eesti nbsp English nbsp espanol nbsp Esperanto nbsp euskara nbsp francais nbsp Frysk nbsp galego nbsp hrvatski nbsp Ido nbsp italiano nbsp lietuviu nbsp magyar nbsp Nederlands nbsp norsk bokmal nbsp norsk nynorsk nbsp occitan nbsp Plattduutsch nbsp polski nbsp portugues nbsp portugues do Brasil nbsp romană nbsp Scots nbsp sicilianu nbsp slovencina nbsp slovenscina nbsp suomi nbsp svenska nbsp Tiếng Việt nbsp Turkce nbsp veneto nbsp Ellhnika nbsp belaruskaya tarashkevica nbsp blgarski nbsp makedonski nbsp nohchijn nbsp russkij nbsp srpski srpski nbsp tatarcha tatarca nbsp ukrayinska nbsp ქართული nbsp հայերեն nbsp ব ল nbsp தம ழ nbsp മലയ ള nbsp ithy nbsp 한국어 nbsp 日本語 nbsp 简体中文 nbsp 繁體中文 nbsp עברית nbsp العربية nbsp فارسی nbsp nbsp aekikh cestina English francais italiano polski portugues עברית العربية russkij This figure was prepared by Robert A Rohde as part of the Global Warming Art project Image from Global Warming Art This image is an original work created for Global Warming Art Please refer to the image description page for more information xnuyatihkhdlxk aeckcayaela hruxddaeprexksarniphayitenguxnikhkhxngsyyaxnuyatexksaresrikhxngknu run 1 2 hruxrunid nbcaknithixxkodymulnithisxftaewresri odyimmiswnidhamaekikh immikhxkhwampkhnaaelapkhlng saenakhxngsyyaxnuyatrwmxyuinswnchux syyaxnuyatexksaresrikhxngknuhttp www gnu org copyleft fdl html GFDL GNU Free Documentation License true true iflnixyuphayitsyyaxnuyat khriexthifkhxmmxns aebbaesdngthima xnuyataebbediywkn 3 0 tnchbb khunsamarth thicaaebngpn thicathasaena aeckcay aelasngngandngklawtxip thicaeriyberiyngihm thicaddaeplngngandngklaw phayitenguxnikhtxipni aesdngthima khuntxngihekiyrtiecakhxngnganxyangehmaasm odyephimlingkipyngsyyaxnuyat aelarabuhakmikarepliynaeplng khunxacthaechnniidinrupaebbidkidtamkhwr aettxngimichinlksnathiaenawaphuihxnuyatsnbsnunkhunhruxkarichngankhxngkhun xnuyataebbediywkn hakkhunddaeplng epliynrup hruxtxetimnganni khuntxngichsyyaxnuyataebbediywknhruxaebbthiehmuxnkbsyyaxnuyatthiichkbnganniethann payaesdngsthanalikhsiththinithukephimephuxihepniptamkarepliynaeplngsyyaxnuyatkhxngmulnithiwikimiediy cak GFDL ipyng GFDL khwbkhukb CC BY SA 3 0 http creativecommons org licenses by sa 3 0 CC BY SA 3 0 Creative Commons Attribution Share Alike 3 0 true true pumkarxpohldtnchbb date time username resolution size edit summary 22 43 9 June 2007 w en User Dragons flight 800 595 37 125 GWArt khabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairraykarthiaesdngxyuiniflniprakxbdwysthanalikhsiththimilikhsiththisyyaxnuyatGNU Free Documentation License version 1 2 or later nbsp xngkvsCC BY SA 3 0wnthisrang wnkxtng9 tulakhm 2008media type nbsp xngkvsimage png prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn16 24 25 singhakhm 2550800 595 36 kiolibt BetacommandBotTranswiki approved by w en User Dmcdevit This image was copied from wikipedia en The original description was Description This figure shows the w en solar radiation spectrum for direct w en light at both the top of the w en Earth hnathimiphaphni hnatxipni oyngmathiphaphni praktkarneruxnkrack karichiflkhamokhrngkar wikixuntxipniichiflni karichbn ar wikipedia org مستخدم هيثم الصعب الإشعاع الشمسي karichbn be wikipedia org Sonechnaya radyyacyya karichbn ca wikipedia org Radiacio solar karichbn en wikipedia org Air mass astronomy Air mass solar energy User Adacore Solar Energy Wikipedia Reference desk Archives Science 2012 October 2 Wikipedia Reference desk Archives Science 2012 December 12 User Arthurcala sandbox Spectrum physical sciences karichbn en wikibooks org High School Earth Science Energy in the Atmosphere karichbn en wikiversity org Solar System technical Sun Stars Sun Stars Sun Astronomy Renewable energy The energy challenge Stars Sun Heliometry karichbn es wikipedia org Radiacion solar Energia luminica Luz solar Masa de aire astronomia Usuario MrLejinad Baul Espectro discreto karichbn eu wikipedia org Eguzki erradiazio karichbn fa wikipedia org طیف گسسته karichbn fi wikipedia org Auringon sateily karichbn hak wikipedia org Ngit theu Fuk sa karichbn he wikipedia org ויקיפדיה הכה את המומחה שאלות במדעים מדויקים ארכיון 5 karichbn it wikipedia org Utente Arthurcala Sandbox karichbn ja wikipedia org 太陽変動 利用者 Einstee sandbox karichbn ka wikipedia org სათბურის ეფექტი karichbn ko wikipedia org 태양 에너지 karichbn ro wikipedia org Variație solară karichbn ru wikipedia org Solnechnaya radiaciya Obluchyonnost fotometriya karichbn sh wikipedia org Sunceva svjetlost karichbn si wikipedia org හර ත ග ර ආචරණය karichbn sl wikipedia org Ucinek tople grede karichbn sr wikipedia org Sunceva atmosfera karichbn uz wikipedia org Havo massasi astronomiya karichbn vi wikipedia org Quang phổ rời rạc karichbn vls wikipedia org Atmosfeer Sterre karichbn zh wikipedia org 太阳光 太阳活动 温室效应 太陽輻射khxmulekiywkbphaph phaphnimikhxmulephimetim sungswnihymacakklxngdicitxlhruxsaeknenxrthisamarthekbkhxmuldngklawiwrwmkbphaphid thaphaphnithukprbprungaekikhhruxepliynaeplngcakedim khxmulbangxyangcayngkhngimepliynaeplngehmuxnphaphthithukprbprungaekikhnnsxftaewrthiichAdobe ImageReady ekhathungcak https th wikipedia org wiki ifl Solar Spectrum png