Filament eruption, activity behind the limb

Sunday, 2 November 2014 11:38 UTC

Filament eruption, activity behind the limb

Solar activity on the earth-facing solar disk is low. None of the earth-facing sunspot regions are worth mentioning apart from perhaps sunspot region 2203 which is growing steadily but lacking any magnetic complexity. However, that doesn't mean the Sun has been totally quiet. Yesterday we saw a rather impressive filament eruption and today our eye fell on a massive shockwave propagating from behind the north-east limb. In this article we take a look at these two events.

Filament eruption

Yesterday we saw an impressive filament eruption from the Sun's south-eastern quadrant. The event launched a coronal mass ejection and was likely the source of an increase in the high energy protons which did not manage to reach the minor S1 solar radiation storm level.

The event launched a coronal mass ejection and coronagraph imagery from SOHO shows us that the blast is heading well east from Earth but there does seem to be a slightly wider and fainter outline (black outline on the image below) which suggest we might see a minor shock passage at Earth the coming days. The EPAM low energy protons and electrons have also increased since this eruption which could also indicate there might be a minor earth-directed component. We however do not expect a significant impact at Earth should there indeed be a minor earth-directed component.

NOAA's ENLIL model shows that this event will not arrive at Earth but NASA predicts a glancing blow from this event.

Farside blast

This morning we saw a strong shockwave originating from behind the north-east limb. This event was the source of a Type II radio sweep (signature of a shockwave traveling trough the solar corona) as measured here on Earth. This event will not have any effects on Earth of course as the associated coronal mass ejection will not be traveling towards us but it does indicate that there might be an interesting sunspot region hiding just behind the limb. This will be something to look out for in the days ahead.

ALERT: Type II Radio Emission
Begin Time: 2014 Nov 02 0941 UTC
Estimated Velocity: 695 km/s

Images/video: NASA SDO, SIDC, ESA/NASA SOHO.

Any mentioned solar flare in this article has a scaling factor applied by the Space Weather Prediction Center (SWPC), the reported solar flares are 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.

Thank you for reading this article! Did you have any trouble with the technical terms used in this article? Our help section is the place to be where you can find in-depth articles, a FAQ and a list with common abbreviations. Still puzzled? Just post on our forum where we will help you the best we can! Never want to miss out on a space weather event or one of our news articles again? Subscribe to our mailing list, follow us on Twitter and Facebook and download the SpaceWeatherLive app for Android and iOS!

Latest news

Support SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!

SpaceWeatherLive Pro
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2024/12/08X2.2
Last M-flare2024/12/22M1.1
Last geomagnetic storm2024/12/17Kp5+ (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
November 2024152.5 -13.9
December 2024103.3 -49.2
Last 30 days114 -43.9

This day in history*

Solar flares
12015M6.75
21998M3.34
32013M2.36
42013M1.97
52001M1.69
DstG
12002-67
22000-62G2
31989-60
42014-57
51982-53G1
*since 1994

Social networks