Протуберанција: Разлика помеѓу преработките

Првиот детализиран опис на соларната протуберанција бил во 14-ти век[[Кодексот на Лаурентиан]],кој ја опишувал [[Соларната еклипса на 1-ви Мај 1185]]. Тие биле опишани како "пламени јазици на живата искра".<ref name=Montreal>{{cite web |url=http://www.astro.umontreal.ca/~paulchar/grps/histoire/newsite/sp/great_moments_e.html |title= 1185: The first description of solar prominences |author=<!--Staff writer(s); no by-line.--> |date= 2008 |website= Great Moments in the History of Solar Physics|publisher= Université de Montréal |access-date= March 30, 2015}} See pdf version [http://thebookofbeginnings.com/sources/4/HistoryofSolarPhysics.pdf here] (accessed 21 August 2015).</ref><ref name=Newsletter>{{cite journalнмс |url=http://eclipse.gsfc.nasa.gov/SENL/SENL200305.pdf |title=Solar Eclipse Newsletter |volume=8 |number=5|first1=Patrick |last1=Poitevin |first2=Joanne |last2=Edmonds|date=2003 |website= |publisher=Patrick Poitevin|accessdate=March 30, 2015}} Original text cited at {{cite web |url=http://litopys.org.ua/lavrlet/lavr22.htm |title=Лаврентьевская летопись |website=Izbornik |accessdate=30 March 2015 |page=396 |publisher=[[Russian Academy of Sciences|USSR Academy of Sciences]] |location=Leningrad |year=1927}}</ref>

* {{cite journalнмс | last=Galsgaard | first=K. |author2=Longbottom, A.W. | year=1999 | title=Formation of solar prominences by flux convergence | journal=Astrophysical Journal | volume=510 | pages=444 | doi=10.1086/306559 | bibcode=1999ApJ...510..444G}}

* {{cite journalнмс | last=Low | first=B.C. |author2=Fong, B. |author3=Fan, Y. | year=2003 | title=The mass of a solar quiescent prominence | journal=Astrophysical Journal | volume=594 | pages=1060 | doi=10.1086/377042 | bibcode=2003ApJ...594.1060L | issue=2}}