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    1. APOD: 2007 December 3 - A Complete Solar Cycle from SOHO
    ... 2007 December 3 . A Complete Solar Cycle from SOHO . Credit: SOHO - EIT Consortium , ESA , NASA . ... Credit: SOHO - EIT Consortium , ESA , NASA . Explanation: Every eleven years, our Sun goes through a solar cycle. ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap071203.html -- 5.0 Кб -- 21.12.2007
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    2. APOD: 2008 February 6 - Sunspot in the Old Solar Cycle
    ... 2008 February 6 . Sunspot in the Old Solar Cycle . Credit Copyright: Greg Piepol . ... above in a specific color of light emitted by hydrogen is sunspot 10982, one of the last sunspots of the old solar cycle ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap080206.html -- 5.6 Кб -- 12.04.2008
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    3. APOD: 2006 August 30 - A Backward Sunspot and the New Solar Cycle
    ... 2006 August 30 . A Backward Sunspot and the New Solar Cycle . Credit: MDI , SOHO , ESA , NASA . ... An 11-year solar cycle has been observed for hundreds of years by noting peaks and valleys in the average number of sunspots . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap060830.html -- 5.7 Кб -- 02.10.2012
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    4. APOD: 2006 August 7 - An Erupting Solar Prominence from SOHO
    ... In the year 2000, our Sun went though Solar Maximum , the time in its 11-year cycle where the most sunspots and explosive ... Sunspots , the Solar Cycle , and solar prominences are all caused by the Sun's changing magnetic field . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap060807.html -- 5.7 Кб -- 02.10.2012
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    5. APOD: 2001 September 24 - A Solar Prominence Erupts
    ... Last year, our Sun went though Solar Maximum , the time in its 11-year cycle where the most sunspots and explosive activities ... Sunspots , the Solar Cycle , and solar prominences are all caused by the Sun's changing magnetic field . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap010924.html -- 4.9 Кб -- 01.10.2012
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    6. APOD: 2009 June 4 - Sunspots on a Cloudy Day
    ... since the 1950s. Even the latest prediction is that the new cycle, Solar Cycle 24, will reach a maximum in May 2013 with a ... The Solar Cycle 24 sunspots recorded here are in active region AR 1019. ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap090604.html -- 5.6 Кб -- 28.02.2014
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    7. APOD: 2013 April 26 - A Year on the Sun
    ... Girdling both sides of the equator during approach to maximum in the 11-year solar cycle , the solar active regions are laced with bright loops and arcs along magnetic field lines . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap130426.html -- 5.0 Кб -- 28.02.2014
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    8. APOD: 2000 April 3 - A Twisted Solar Eruptive Prominence
    ... Although large prominence s and energetic Coronal Mass Ejection s (CMEs) are relatively rare, they are occurring more frequently now that we are near the Solar Maximum , a time of peak sunspot and solar activity in the eleven-year solar cycle . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap000403.html -- 4.7 Кб -- 01.10.2012
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    9. APOD: 2003 February 23 - A Twisted Solar Eruptive Prominence
    ... Although large prominence s and energetic Coronal Mass Ejection s (CMEs) are relatively rare, they are occurred more frequently near Solar Maximum , the time of peak sunspot and solar activity in the eleven-year solar cycle . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap030223.html -- 4.6 Кб -- 01.10.2012
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    10. APOD: 2008 June 1 - A Twisted Solar Eruptive Prominence
    ... Although large prominence s and energetic Coronal Mass Ejection s (CMEs) are relatively rare, they are occurred more frequently near Solar Maximum , the time of peak sunspot and solar activity in the eleven-year solar cycle . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap080601.html -- 5.4 Кб -- 05.09.2008
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