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What has been billed as the largest sunspot observed in several years has now rotated around to stare straight at Earth. How large is it? Active Region 1339 and the group of sunspots adjacent to it extends more than 100,000 km from end to end and each of the several dark cores is larger than Earth. The now very active Sun has already blasted out several medium- to large-sized solar flares and has the potential to hurl out more.
And the Sun is now dotted with several smaller sunspots as well. Above is an amazing image of all this activity, as captured by astrophotographer Alan Friedman. “This has been a glorious week for solar observers!” Friedman said. “Led by large sunspot region AR1339, the sun’s disk is alive with activity… the most dynamic show in many years.”
Take a look below for an incredible closeup of AR1339 taken by Friedman, as well as a movie from the Solar Dynamics Observatory showing the sunspots rotating into view.
Click on the image for a larger version on Friedman’s website, AvertedImagination.com
From all this activity, there may be a good chance for viewing aurorae. On November 9 at around 1330 UT, a magnetic filament in the vicinity of sunspot complex 1342-1343 erupted, producing a M1-class solar flare and hurling a CME into space, which will probably deliver a glancing blow to Earth’s magnetic field on Nov 11 or 12, according to SpaceWeather.com
And here’s an image from astrophotographer Raymond Gilchrist showing a labeled version of all the current sunspots: 1338, 1339, 1340, 1341, 1342, 1343, 1344.
Raymond used a Baader Solar Continuum Filter and Thousand Oaks Full Solar Filter with a Skywatcher 120mm S/T Refractor,
with a Canon 350D, 1/15th Sec Exp. at ISO400. You can see more of his images at his Flickr page.
well having this kinda information is like playing Russia rule-lat but you don’t when if your luck will turn on you but you hope for the best but i don’t think it is any thing to worrier about majorly
I understand the logic for numbering sunspot groups but the question I have is when we look at sunspot counts, especially those in Sky & Telescope that are historical data. At what resolution are the spots counted? With a small telescope only the largest spots are seen but using the images now available from the major solar observatories very tiny spots can be seen a presumably counted. Is the a lower limit on “countable” sunspots?
I understand the logic for numbering sunspot groups but the question I have is when we look at sunspot counts, especially those in Sky & Telescope that are historical data. At what resolution are the spots counted? With a small telescope only the largest spots are seen but using the images now available from the major solar observatories very tiny spots can be seen a presumably counted. Is the a lower limit on “countable” sunspots?