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Submitted on 2014-12-30
In its New Year's letter for 2014, the Sun promised great solar activity to come. True to its word, sunspot numbers reached a new monthly high in February 2014, probably indicating the maximum of the ongoing solar cycle. Throughout the year, this increased sunspot activity was accompanied by plenty of strong flares, big sunspot groups and geomagnetic unrest.
Submitted on 2014-12-12
If you are looking for solar, solar wind, and earth environment data at a glance and you want to see them on a timeline, even if you are not a computer expert: STAFF has it all.
Submitted on 2014-11-26
With only one more month to go in 2014, huge NOAA 2192 is very probably going to be *the* sunspot group of the year. After its impressive performance just a few weeks ago (see this news item), observers and forecasters were counting down to its re-appearance at the solar east limb. NOAA 2192 obliged by starting its encore performance on 12 November, getting itself a new name: NOAA 2209. Unfortunately, as is sometimes the case with sequels of blockbusters, this group did not live up to the expectations.
Submitted on 2014-11-13
We are now close to 6 years since solar cycle 24 (SC24) started the gradual climb towards its solar cycle maximum. Over the last year, solar activity was mostly elevated, with several X-class flares and large sunspot groups. As the sunspot activity varies from month to month, the monthly sunspot numbers are smoothed to get an idea of the overall evolution. It then appears, pending the smoothing formula used, that a solar cycle maximum occurred during the early spring months of 2014 (red curve in graph underneath).
Submitted on 2014-11-05
Solar filaments are clouds of ionized gas above the solar surface squeezed between magnetic regions of opposite polarity. Being cooler and denser than the plasma underneath and their surroundings, they appear as dark lines when seen on the solar disk using special filters. At the solar limb, the same features shine bright over the solar limb and are called prominences. As filaments grow longer, they are more likely to erupt, often accompanied by a coronal mass ejection (CME).
Submitted on 2014-10-29
Much has already been written on the numerous X-class flares produced by NOAA 2192. In this news item, scientists from the STCE let their light shine on some of the other issues associated to this very active region:
Submitted on 2014-10-24
On 19 October, an X1.1 flare was observed. Starting at 04:17UT, this long duration event (LDE) ended only at 05:48UT. Remarkably, the peak x-ray flux stayed at the X1.1-level for a full 6 minutes, i.e. from 05:01UT till 05:06UT. This flare was the 36th solar flare of ongoing solar cycle 24, but due to its low-level strength, it is ranked at the bottom of the X-class event list (see the Top-10).
Submitted on 2014-10-08
Last week's highlight certainly was the M7.3 flare that was produced by the sunspot complex NOAA 2172/2173. This flare peaked on 2 October at 19:01UT, and was preceded by a long duration M1.5 flare peaking at 17:44UT in the same area near the southeast solar limb.
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