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Piú votate - The Sun: just a star, like many others...
The Sun-EIT99promcloseG.jpg
The Sun-EIT99promcloseG.jpgOur "restless" Sun...and Us!54 visitenessun commento55555
(5 voti)
The Sun-CropplumeG.jpg
The Sun-CropplumeG.jpgOur "restless" Sun... (6)54 visitenessun commento55555
(5 voti)
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Sunspot-reversed-0.jpgSunspot-905: a sign of an incoming new "Solar Cycle"? (1)54 visiteDa "NASA - Picture of the Day" del 30 Agosto 2006:"Why is sunspot-905 backwards? Perhaps it is a key marker for the beginning of a new Magnetic Cycle on our Sun.
Every 11 years, our Sun goes through a Magnetic Cycle, at the end of which its overall magnetic orientation is reversed. An 11-year Solar Cycle has been observed for hundreds of years by noting peaks and valleys in the average number of sunspots.
Just now, the Sun is near Solar Minimum, and likely to start a long progression toward the most active time, called Solar Maximum, in about 5,5 years".
55555
(5 voti)
ZZ-ZZ-ZZ-1-The_Sun-Full-Disk_171_final.gif
ZZ-ZZ-ZZ-1-The_Sun-Full-Disk_171_final.gifBright Flare (GIF-Movie - normal)152 visitenessun commentoMareKromium55555
(4 voti)
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ZZ-ZZ-ZZ-2-The_Sun-CU_171_final.gifBright Flare (GIF-Movie - EDM)155 visitenessun commentoMareKromium55555
(4 voti)
ZZ-ZZ-ZZ-3-The_Sun-FlareX13_20220330_171A_2048p30_Sq.gif
ZZ-ZZ-ZZ-3-The_Sun-FlareX13_20220330_171A_2048p30_Sq.gifThe always restless Sun... Sun-Flare X-13116 visitenessun commentoMareKromium55555
(4 voti)
The_Sun-489332main_euvfilament-20101016-3.jpg
The_Sun-489332main_euvfilament-20101016-3.jpgIntense Solar Activity on the Sun: Sunspot 1112 and Solar Flares72 visiteImage of Sunspot Region 1112 (dated October, 18. 2010) as it continues to rotate towards the South Eastern Rim of the Sun.MareKromium55555
(4 voti)
The_Sun-489332main_euvfilament-20101016-4.jpg
The_Sun-489332main_euvfilament-20101016-4.jpgIntense Solar Activity on the Sun: Sunspot 1112 and Solar Flares72 visitePartial Filament Eruption.MareKromium55555
(4 voti)
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Sun_Spot.jpgA really beautiful and DEEP SunSpot85 visitenessun commentoMareKromium55555
(4 voti)
Athmosferic_Corona-Schneider.jpg
Athmosferic_Corona-Schneider.jpgDiamond Ring and Shadow Bands67 visiteDalla Rubrica "NASA - Picture of the Day" del giorno 24 Luglio 2010:"As the total phase of July ,11th, 2010 Solar Eclipse came to an end, Sunlight streaming past the edge of the Moon's silhouette created the fleeting appearance of a glistening Diamond Ring in the sky.
Seen through a thin cloud layer from the French Polynesian atoll of Hao it also produced remarkable Shadow Bands, flickering across the dramatic scene. Projected onto the cloud layer, the Shadow Bands are parallel to the sliver of Sunlight emerging from behind the Moon's edge.

Caused by turbulence in Earth's Atmosphere refracting the sliver of Sunlight, the narrow bands were captured in this brief, 1/400th second exposure. Shining through the cloud droplets, the Sunlight also produced a luminous atmospheric corona, not to be confused with the Solar Corona seen during Eclipse Totality.

The Atmospheric Corona is centered on the bright diamond of emerging Sunlight".
MareKromium55555
(4 voti)
Solar_Prominence~0.jpg
Solar_Prominence~0.jpgSolar Prominence67 visiteCaption NASA, da "NASA - Picture of the Day" del giorno 23 Marzo 2010:"Dramatic Prominences can sometimes be seen looming just beyond the edge of the Sun.
Such was the case last week as a Giant Prominence, visible above on the right, highlighted a Sun showing increased activity as it comes off an unusually quiet Solar Minimum. A changing carpet of hot gas is visible in the Chromosphere of the Sun in the above image taken in a very specific color of light emitted by Hydrogen.

A Solar Prominence is a cloud of Solar Gas held just above the Surface by the Sun's Magnetic Field. The Earth would easily fit below the Prominence on the right. Although very hot, Prominences typically appear dark when viewed against the Sun, since they are slightly cooler than the Surface.
A quiescent Prominence typically lasts about a month, and may erupt in a Coronal Mass Ejection (CME) expelling hot gas into the Solar System. The next day, the same prominence looked slightly different".
2 commentiMareKromium55555
(4 voti)
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Solar_Eclipse~0.jpgA "Diamond Ring" among the clouds57 visiteDa "NASA - Picture of the Day" del giorno 8 Agosto 2009:"Cloudy skies over Wuhan, China hid the delicate Solar Corona during July's Total Eclipse of the Sun. Still, the Moon's silhouette was highlighted by these glistening diamonds as the Total Eclipse Phase ended. Caused by bright Sunlight streaming through dips and valleys in the irregular terrain along the Moon's edge, the effect is known as Baily's Beads, named after Francis Baily who called attention to the phenomenon in 1836.
The dramatic appearance of the beads at the beginning or end of a Total Solar Eclipse is also known as the Diamond Ring effect. In this remarkable image, a small, pinkish solar prominence can also be seen along the edge, below the diamonds".
MareKromium55555
(4 voti)
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