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    21. 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.astronet.ru/db/xware/msg/apod/2008-06-01 -- 14.6 Кб -- 01.06.2008
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    22. 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.astronet.ru/db/xware/msg/1217383 -- 15.4 Кб -- 06.11.2006
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    23. A Twisted Solar Eruptive Prominence
    ... Although large prominence s and energetic Coronal Mass Ejection s (CMEs) are relatively rare, they are again 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.astronet.ru/db/xware/msg/1331238 -- 15.3 Кб -- 25.01.2015
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    24. 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.astronet.ru/db/xware/msg/1162587 -- 15.5 Кб -- 06.11.2006
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    25. Orange Sun Scintillating
    ... winds toward Solar Maximum over the next few years, increased activity will likely ... Publications with keywords: Sun - sunspot - solar activity - H-alpha . ... Publications with words: Sun - sunspot - solar activity - H-alpha . See also: . ...
    [ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1254646 -- 15.5 Кб -- 15.11.2011
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    26. 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.astronet.ru/db/xware/msg/1161302 -- 14.5 Кб -- 06.11.2006
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    27. Астронет > 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.astronet.ru/db/msg/1228087/eng/ -- 24.1 Кб -- 01.06.2008
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    28. 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.astronet.ru/db/xware/msg/1186902 -- 14.2 Кб -- 23.02.2003
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    29. Астронет > 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.astronet.ru/db/msg/1186902/eng/ -- 22.1 Кб -- 23.02.2003
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    30. Астронет > 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.astronet.ru/db/msg/1162587/eng/ -- 17.6 Кб -- 06.11.2006
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