This page describes an image Sunspots
Image caption:
In this image the sun peppered with groups of sunspots over almost nine days between July and August 2012. The sunspots seen in this image have been sources of the solar flares and coronal mass ejections (CME). In this image particulary, the sun is approaching solar maximum in its cycle (solar cycle), where we see many spots forming along the suns' equator. These sunspots and activity are seen in the southern hemisphere, before then most of the activity was on the northern hemisphere.
Scroll to captions in other languages
Image credit:
NASA/SDO/HMI Credit Link
Related glossary terms:
Stellar Activity
, Sun
, Sunspot
Categories:
The Sun
Image license: Public Domain Public Domain icons
The media file captions presented on the OAE website were written, translated and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits for our translation project here. All media file captions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE". The media files themselves may have different licenses (see above) and should be credited as listed above under "credit".
Captions in Different Languages:
Image caption: Sur cette image, le Soleil est parsemé de groupes de taches solaires pendant près de neuf jours entre juillet et août 2012. Les taches solaires visibles sur cette image sont à l'origine des éruptions solaires et des éjections de masse coronale (CME). Sur cette image en particulier, le Soleil approche du maximum solaire de son cycle (cycle solaire), où l'on voit de nombreuses taches se former le long de l'équateur du Soleil. Ces taches et cette activité sont visibles dans l'hémisphère sud, alors qu'auparavant, l'essentiel de l'activité se situait dans l'hémisphère nord.
Image credit: NASA/SDO/HMI
Related glossary terms: activité stellaire , Soleil , Tache solaire Caption translation status: Not yet approved by a reviewer
Caption translators: Rulx Narcisse
Image caption: In questa immagine il Sole è stato punteggiato da gruppi di macchie solari per quasi nove giorni tra luglio e agosto 2012. Le macchie solari osservate in questa immagine sono state fonte di brillamenti solari ed espulsioni di massa coronale (CME). In questa immagine, in particolare, il Sole si sta avvicinando al massimo solare del suo ciclo (ciclo solare), dove vediamo formarsi molte macchie lungo l'equatore del Sole. Queste macchie solari e l'attività sono visibili nell'emisfero meridionale, mentre prima la maggior parte dell'attività aveva luogo nell'emisfero settentrionale.
Image credit: NASA/SDO/HMI
Related glossary terms: attività stellare , Macchia solare , Sole Caption translation status: Approved by a reviewer
Caption translators: Giuliana Giobbi
Caption reviewers: Rosa Valiante, Rodolfo Canestrari
