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The numbers are down...


A solar flare is a sudden release of an enormous amount of energy due to magnetic reconnection in the solar atmosphere, usually above sunspot regions. This energy release takes place over the entire electromagnetic spectrum. Solar flares are often classified according to their peak strength in x-rays. Scientists usually use three categories: "C" (common), "M" (medium) and "X" (extreme), with each category 10 times stronger than the previous one. As an example: an X6-flare is 10 times stronger than an M6-flare, and 600 times stronger than a C1-flare.

M for Marvelous


One of last week's highlights certainly was the M1.6-flare in NOAA 1692 near the northwest limb of the Sun. Starting late on 21 March at 21:42UT, it reached its peak flux at 22:04UT and ended at 22:36UT. The event was not accompanied by an energetic proton enhancement.

Ready... Aim... Fire!...


The Sun took a good aim at Earth this week.

Comet Pan-STARRS swings by


From the darkness of outer space, comet Pan-STARRS has come to pay us a one-time visit before receding again into the coldness of oblivion.

The comet, officially designated as C/2011 L4, was discovered in June 2011 by the Pan-STARRS telescope on Hawaii when it was still over 1 billion kilometers away from the Sun. Last Sunday, on 10 March, the comet was closer to our home star than the planet Mercury.

10 Little Indians


During the first two months of 2013, quite a few Coronal Mass Ejections (CMEs) were visible. As an example, this movie shows the CME-activity from 23 till 28 February. The 10 most interesting events were numbered and are discussed below.

Fast rise of NOAA 1678


On 18 February, a sunspot group quickly developed to the southeast (bottom left) of NOAA 1671. According to the daily NOAA reports, fresh NOAA 1678 already reached its maximum sunspot area on 21 February, being nearly three times as large as the total area of the planet Earth.

CMEs twins?


On 6 February, in the time span of just a few hours, an interesting pair of eruptive events occurred on the Sun of which it was difficult to say if they were related or not. Surely, there were two flares and two coronal mass ejections (CMEs), but their timings and outlook hinted to some magnetic commonality.

The protagonists were NOAA 1667, a simple and relatively small sunspot group in the northern hemisphere, and a 200.000 km long but not very impressive filament about 10°-15° degrees to the east ("left") of this sunspot group.

Coronal cathedral


An interesting region in the solar corona appeared over the southeast solar limb starting 1 February.

A CME’s cloaking device


In the Star Trek series, the Romulan empire disposes of an advanced technology that makes their spacecraft invisible. Using this stealth technology, they sneak up behind their unsuspecting enemies, suddenly revealing themselves and blowing the enemy spacecraft to smithereens.

A Coronal Mass Ejection (CME) used its own cloaking device to wreak geomagnetic havoc last Thursday, 17 January.

NOAA 1654 show-off


Active region NOAA 1654 appeared on 8 January at the northeast solar limb and quickly became the dominant sunspot group on the visible solar surface. On 11 January, its sunspot area equaled about 7 times the area of the Earth, and by 13 January its length was almost 19 Earth diameters. The leading spot was complex and changed its shape impressively, as can be seen in this movie covering the period from 10 January (noon) till 12 January (noon).

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