by APOD Robot » Tue Jan 15, 2013 5:06 am
A Solar Ballet
Explanation: Sometimes, the Sun itself seems to dance. On just this past New Year's Eve, for example, NASA's Sun-orbiting
Solar Dynamic Observatory spacecraft imaged an
impressive prominence erupting from the Sun's surface. The
dramatic explosion was captured in ultraviolet light in the
above time lapse video covering four hours. Of particular interest is the tangled
magnetic field that directs a type of
solar ballet for the hot
plasma as it falls back to the Sun. The scale of the disintegrating
prominence is huge -- the entire
Earth would easily fit under the flowing
curtain of hot gas. 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 energy mechanism that creates a
solar prominence is still a topic of
research. As the Sun nears
Solar Maximum this year,
solar activity like
eruptive prominences should be common.
[/b]
[url=http://apod.nasa.gov/apod/ap130115.html][img]http://apod.nasa.gov/apod/calendar/S_130115.jpg[/img] [size=150]A Solar Ballet[/size][/url]
[b] Explanation: [/b] Sometimes, the Sun itself seems to dance. On just this past New Year's Eve, for example, NASA's Sun-orbiting [url=http://www.nasa.gov/mission_pages/sdo/main/index.html]Solar Dynamic Observatory[/url] spacecraft imaged an [url=http://apod.nasa.gov/apod/ap030223.html]impressive prominence[/url] erupting from the Sun's surface. The [url=http://apod.nasa.gov/apod/ap110307.html]dramatic explosion[/url] was captured in ultraviolet light in the [url=http://www.youtube.com/watch?v=Vtnof33Xu4A]above time lapse video[/url] covering four hours. Of particular interest is the tangled [url=http://solarscience.msfc.nasa.gov/the_key.shtml]magnetic field[/url] that directs a type of [url=http://www.nasa.gov/mission_pages/sdo/news/solar-ballet2.html]solar ballet[/url] for the hot [url=http://en.wikipedia.org/wiki/Plasma_%28physics%29]plasma[/url] as it falls back to the Sun. The scale of the disintegrating [url=http://apod.nasa.gov/apod/ap000809.html]prominence[/url] is huge -- the entire [url=http://apod.nasa.gov/apod/ap121207.html]Earth[/url] would easily fit under the flowing [url=http://apod.nasa.gov/apod/ap011203.html]curtain[/url] of hot gas. A quiescent [url=http://solar.physics.montana.edu/YPOP/Program/hfilament.html]prominence typically[/url] lasts about a month, and may erupt in a [url=http://lheawww.gsfc.nasa.gov/~reames/DARK7.HTML]Coronal Mass Ejection[/url] (CME) [url=http://apod.nasa.gov/apod/ap010924.html]expelling hot gas[/url] into the [url=http://en.wikipedia.org/wiki/Sweden_Solar_System]Solar System[/url]. The energy mechanism that creates a [url=http://apod.nasa.gov/apod/ap030707.html]solar prominence[/url] is still a topic of [url=http://adsabs.harvard.edu/abs/2004ApJ...600.1043Z]research[/url]. As the Sun nears [url=http://en.wikipedia.org/wiki/Solar_maximum]Solar Maximum[/url] this year, [url=http://apod.nasa.gov/apod/ap071203.html]solar activity[/url] like [url=http://apod.nasa.gov/apod/ap100510.html]eruptive prominences[/url] should be common.
[b][table][tr][td=left][url=http://asterisk.apod.com/discuss_apod.php?date=130114]<< Previous APOD[/url][/td] [td=center][url=http://asterisk.apod.com/view_retro.php?date=0115]This Day in APOD[/url][/td] [td=right][url=http://asterisk.apod.com/discuss_apod.php?date=130116]Next APOD >>[/url][/td][/tr][/table][/b]