คำอธิบายCosmic ray flux versus particle energy.svg
English: The flux of cosmic ray particles as a function of their energy. The flux for the lowest energies (yellow zone) are mainly attributed to solar cosmic rays, intermediate energies (blue) to galactic cosmic rays, and highest energies (purple) to extragalactic cosmic rays
Français : Le flux de particules du rayonnement cosmique (incident au sommet de l'atmosphère terrestre, par unité de surface, par unité de temps et par unité d'angle solide et par intervalle d'énergie des particules incidentes de 1 gigaélectron-volt (1 GeV)) représenté en fonction de leur énergie. Le flux des énergies les plus basses (zone jaune) sont principalement imputables aux rayons cosmiques solaires, les énergies intermédiaires (en bleu) aux rayons cosmiques galactiques, et les plus hautes énergies (violet) aux rayons cosmiques extragalactiques
วันที่
แหล่งที่มา
own work, after Swordy and De Angelis
ผู้สร้างสรรค์
Sven Lafebre
References
S. Swordy, The energy spectra and anisotropies of cosmic rays, 2001, Space Science Reviews 99, pp85–94.
A. de Angelis and M. Pimenta, Introduction to particle and astroparticle physics (Multimessenger astronomy and its particle physics foundations), Springer 2018, p577.
an updated 2018 version uploaded based on the original author's request (see [https://commons.wikimedia.org/wiki/Commons:Help_desk/Archive/2019/01#New_version_of_%22Cosmic_ray_flux_versus_particle_energy%22_image here])
== Summary == {{Information |Description=The flux of cosmic ray particles as a function of their energy. The flux for the lowest energies (yellow zone) are mainly attributed to solar cosmic rays, intermediate energies (blue) to galactic cosmic rays, and h
{{Information |Description=The flux of cosmic ray particles as a function of their energy. The flux for the lowest energies (yellow zone) are mainly attributed to solar cosmic rays, intermediate energies (blue) to galactic cosmic rays, and highest energie
ไฟล, cosmic, flux, versus, particle, energy, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลาง, อม, ลเก, ยวก, บภาพขนาดของต, วอย, าง, ของไฟล, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, ไฟล, กเซล, ขนาดไฟล, โลไบต, ปภาพ. ifl prawtiifl hnathimiphaphni karichiflswnklang khxmulekiywkbphaphkhnadkhxngtwxyang PNG nikhxngifl SVG ni 500 600 phikesl khwamlaexiydxun 200 240 phikesl 400 480 phikesl 640 768 phikesl 854 1 024 phikesl 1 708 2 048 phikesl 512 614 phikesl duphaphthimikhwamlaexiydsungkwa 8206 ifl SVG 512 614 phikesl khnadifl 113 kiolibt rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khwamyx khaxthibayCosmic ray flux versus particle energy svg English The flux of cosmic ray particles as a function of their energy The flux for the lowest energies yellow zone are mainly attributed to solar cosmic rays intermediate energies blue to galactic cosmic rays and highest energies purple to extragalactic cosmic rays Francais nbsp Le flux de particules du rayonnement cosmique incident au sommet de l atmosphere terrestre par unite de surface par unite de temps et par unite d angle solide et par intervalle d energie des particules incidentes de 1 gigaelectron volt 1 GeV represente en fonction de leur energie Le flux des energies les plus basses zone jaune sont principalement imputables aux rayons cosmiques solaires les energies intermediaires en bleu aux rayons cosmiques galactiques et les plus hautes energies violet aux rayons cosmiques extragalactiques wnthi 8 mkrakhm ph s 2562 aehlngthima own work after Swordy 1 and De Angelis 2 phusrangsrrkh Sven Lafebre References S Swordy The energy spectra and anisotropies of cosmic rays 2001 Space Science Reviews 99 pp85 94 A de Angelis and M Pimenta Introduction to particle and astroparticle physics Multimessenger astronomy and its particle physics foundations Springer 2018 p577 karxnuyatichsiththi khapheca inthanaphuthuxlikhsiththikhxngphaphhruxsuxni xnuyatihichphaphhruxsuxniphayitenguxnikhtxipni 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 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BY SA 2 5 Creative Commons Attribution Share Alike 2 5 true truekhunsamartheluxksyyaxnuyatdngklawtamtxngkarkhabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairxngkvsGraph of cosmic flux versus particle energyixethmthiaesdngxyuiniflniprakxbdwysthanalikhsiththimilikhsiththisyyaxnuyatCreative Commons Attribution ShareAlike 2 5 Generic nbsp xngkvsCreative Commons Attribution ShareAlike 3 0 Unported nbsp xngkvsCreative Commons Attribution ShareAlike 2 0 Generic nbsp xngkvsCreative Commons Attribution ShareAlike 1 0 Generic nbsp xngkvsGNU Free Documentation License version 1 2 or later nbsp xngkvswnthisrang wnkxtng8 mkrakhm 2019 prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn17 31 15 kumphaphnth 2562512 614 113 kiolibt Cherkashan updated 2018 version uploaded based on the original author 039 s request see https commons wikimedia org wiki Commons Help desk Archive 2019 01 New version of 22Cosmic ray flux versus particle energy 22 image here 21 12 12 mkrakhm 2550400 480 94 kiolibt Svenlafe commonswiki Summary Information Description The flux of cosmic ray particles as a function of their energy The flux for the lowest energies yellow zone are mainly attributed to solar cosmic rays intermediate energies blue to galactic cosmic rays and h 21 05 12 mkrakhm 2550400 480 26 kiolibt Svenlafe commonswiki Information Description The flux of cosmic ray particles as a function of their energy The flux for the lowest energies yellow zone are mainly attributed to solar cosmic rays intermediate energies blue to galactic cosmic rays and highest energie hnathimiphaphni hnatxipni oyngmathiphaphni rngsikhxsmik karichiflswnklang wikixuntxipniichiflni karichbn ar wikipedia org أشعة كونية الأشعة الكونية من خارج المجرة karichbn ast wikipedia org Radiacion cosmico karichbn az wikipedia org Kosmik sualar karichbn be wikipedia org Kasmichnyya pramyani karichbn bg wikipedia org Kosmicheski lchi karichbn blk wikipedia org က မစ ရ င တဆဝ 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