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This graph image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with {{vector version available|new image name}}. It is recommended to name the SVG file "Sunspot Numbers.svg" – then the template Vector version available (or Vva) does not need the new image name parameter.
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Changes in carbon-14 concentration in the Earth's atmosphere, which serves as a long term proxy of solar activity.
This figure summarizes sunspot number observations. Since c. 1749, continuous monthly averages of sunspot activity have been available and are shown here as reported by the Solar Influences Data Analysis Center, World Data Center for the Sunspot Index, at the Royal Observatory of Belgium. These figures are based on an average of measurements from many different observatories around the world. Prior to 1749, sporadic observations of sunspots are available. These were compiled and placed on consistent monthly framework by Hoyt & Schatten (1998a, 1998b).
The most prominent feature of this graph is the c. 11 year solar magnetic cycle which is associated with the natural waxing and waning of solar activity.
On longer time scales, the sun has shown considerable variability, including the long Maunder Minimum when almost no sunspots were observed, the less severe Dalton Minimum, and increased sunspot activity during the last fifty years, known as the Modern Maximum. The causes for these variations are not well understood, but because sunspots and associated faculae affect the brightness of the sun, solar luminosity is lower during periods of low sunspot activity. It is widely believed that the low solar activity during the Maunder Minimum may be among the principal causes of the chilly Little Ice Age, circa 1350-1850 A.D.
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This figure was prepared by Robert A. Rohde and is 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.
Bu sənədi GNU Azad Sənədləşdirmə Lisenziyası, Versiya 1.2 və ya Azad Proqram Fondu tərəfindən nəşr olunan hər hansı sonrakı versiya şərtlərinə əsasən dəyişməz bölmələr, ön qapaq mətnləri və arxa qapaq mətnləri olmadan köçürmək, yayımlamaq və / və ya dəyişdirmək üçün icazə verilir; Lisenziyanın bir nüsxəsi GNU Azad Sənədləşdirmə Lisenziyası adlı hissəyə daxil edilmişdir.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue
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References
Hoyt, D. V., and K. H. Schatten (1998a). "Group sunspot numbers: A new solar activity reconstruction. Part 1.". Solar Physics179: 189-219.
Hoyt, D. V., and K. H. Schatten (1998b). "Group sunspot numbers: A new solar activity reconstruction. Part 2.". Solar Physics181: 491-512.
Stott, Peter A.; Gareth S. Jones and John F. B. Mitchell (15 December 2003). "Do Models Underestimate the Solar Contribution to Recent Climate Change". Journal of Climate16: 4079-4093.
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I added another decade to the graph (through Oct., 2015). I started with the previous version was uploaded in 2006. Because it was almost a decade old, it lacked Solar Cycle 24. So I started with that version, and pasted a properly-scaled version of h...
I added another decade to the graph (through Oct., 2015). I started with the previous version was uploaded in 2006. Because it was almost a decade old, it lacked Solar Cycle 24. So I started with that version, and pasted a properly-scaled version of h...
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13:42, 1 fevral 2023
Fevral 28, 2023
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Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarSinaq gosterisi olcusu 800 336 piksel Diger olculer 320 134 piksel 640 269 piksel 1 813 762 piksel Faylin orijinali 8206 1 813 762 piksel fayl hecmi 115 KB MIME novu image png Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get This graph image could be re created using vector graphics as an SVG file This has several advantages see nbsp Commons Media for cleanup for more information If nbsp an nbsp SVG nbsp form nbsp of nbsp this nbsp image is available please upload it and afterwards replace this template with vector version available i new image name i It is recommended to name the SVG file Sunspot Numbers svg then the template Vector version available or Vva does not need the new image name parameter Xulase Changes in carbon 14 concentration in the Earth s atmosphere which serves as a long term proxy of solar activity This figure summarizes sunspot number observations Since c 1749 continuous monthly averages of sunspot activity have been available and are shown here as reported by the Solar Influences Data Analysis Center World Data Center for the Sunspot Index at the Royal Observatory of Belgium These figures are based on an average of measurements from many different observatories around the world Prior to 1749 sporadic observations of sunspots are available These were compiled and placed on consistent monthly framework by Hoyt amp Schatten 1998a 1998b The most prominent feature of this graph is the c 11 year solar magnetic cycle which is associated with the natural waxing and waning of solar activity On longer time scales the sun has shown considerable variability including the long Maunder Minimum when almost no sunspots were observed the less severe Dalton Minimum and increased sunspot activity during the last fifty years known as the Modern Maximum The causes for these variations are not well understood but because sunspots and associated faculae affect the brightness of the sun solar luminosity is lower during periods of low sunspot activity It is widely believed that the low solar activity during the Maunder Minimum may be among the principal causes of the chilly Little Ice Age circa 1350 1850 A D Copyright This figure was prepared by Robert A Rohde and is 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 Bu senedi GNU Azad Senedlesdirme Lisenziyasi Versiya 1 2 ve ya Azad Proqram Fondu terefinden nesr olunan her hansi sonraki versiya sertlerine esasen deyismez bolmeler on qapaq metnleri ve arxa qapaq metnleri olmadan kocurmek yayimlamaq ve ve ya deyisdirmek ucun icaze verilir Lisenziyanin bir nusxesi GNU Azad Senedlesdirme Lisenziyasi adli hisseye daxil edilmisdir http www gnu org copyleft fdl html GFDL GNU Free Documentation License true true Bu fayl Creative Commons Attribution Share Alike 3 0 Sinqapur lisenziyasi altinda yayimlanir Azadsiniz paylasmaq eseri kocurmek paylamaq ve oturmek ucun remiks etmek eseri adaptasiya etmek Asagidaki sertlere riayet etmekle istinad Muvafiq kredit vermelisiniz lisenziyaya bir kecid vermelisiniz ve deyisikliklerin olub olmadigini bildirmelisiniz Bunu her hansi bir aglabatan sekilde ede bilersiniz ancaq lisenziyalasdiricinin sizi ve ya istifadenizi tesdiqlemesini teklif eden bir sekilde deyil benzer paylasma Eseri remix edirsinizse deyisdirirsinizse ve ya uzerinde is aparirsinizsa oz tohfelerinizi orijinalda oldugu kimi eyni ve ya uygun lisenziya altinda yayimlamalisiniz This licensing tag was added to this file as part of the GFDL licensing update http creativecommons org licenses by sa 3 0 CC BY SA 3 0 Creative Commons Attribution Share Alike 3 0 true true References Hoyt D V and K H Schatten 1998a Group sunspot numbers A new solar activity reconstruction Part 1 Solar Physics 179 189 219 Hoyt D V and K H Schatten 1998b Group sunspot numbers A new solar activity reconstruction Part 2 Solar Physics 181 491 512 Stott Peter A Gareth S Jones and John F B Mitchell 15 December 2003 Do Models Underestimate the Solar Contribution to Recent Climate Change Journal of Climate 16 4079 4093 CaptionsazerbaycancaAdd a one line explanation of what this file representsItems portrayed in this filetesvir edircopyright status nbsp ingiliscopyrighted nbsp ingilislisenziyaGNU Free Documentation License version 1 2 or later nbsp ingilisCreative Commons Attribution ShareAlike 3 0 Unported nbsp ingilisMIME type nbsp ingilisimage png Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki13 44 1 fevral 20231 813 762 115 KB Dragons flightUpdate time series to January 2023 11 37 24 avqust 20221 813 762 115 KB Dragons flightUpdate time series to present 15 21 23 noyabr 20151 020 425 78 KB NCdaveI added another decade to the graph through Oct 2015 I started with the previous version was uploaded in 2006 Because it was almost a decade old it lacked Solar Cycle 24 So I started with that version and pasted a properly scaled version of h 15 18 23 noyabr 20151 000 425 42 KB NCdaveReverted to version as of 20 16 20 July 2006 UTC 15 15 23 noyabr 20151 020 425 78 KB NCdaveI added another decade to the graph through Oct 2015 I started with the previous version was uploaded in 2006 Because it was almost a decade old it lacked Solar Cycle 24 So I started with that version and pasted a properly scaled version of h 20 16 20 iyul 20061 000 425 42 KB Nils Simon Fayl kecidleri Bu sekile olan kecidler Gunes dovresi Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur af wikipedia org layihesinde istifadesi Sonsiklus ar wikipedia org layihesinde istifadesi ذروة شمسية دورة الشمس الدنيا be wikipedia org layihesinde istifadesi Sonechnaya aktyynasc bg wikipedia org layihesinde istifadesi Slnchev cikl ca 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