CIR ahead of CH HSS sparks G1 - Minor geomagnetic storming

CIR ahead of CH HSS sparks G1 - Minor geomagnetic storming

A Co-Rotating Interaction Region (CIR) ahead of isolated positive polarity Coronal Hole High Speed Stream (CH HSS) is affecting our planet today, causing geomagnetic storming.  G1 - Minor geomagnetic storm threshold was reached 05:30 UTC.

Over the past 24 hours, solar wind parameters were indicative of a slow solar wind regime followed by onset of a CIR ahead of an isolated positive polarity CH HSS. Total IMF strength was 1 to 4 nT until after 14:00 UTC (November 20), when the IMF strength increased and reached 15 nT near 23:30 UTC. The Bz component underwent mainly weak deviations before it underwent brief and intermittent southward direction shifts after 16:00. Solar wind speed was about 330 - 350 km/s before it increased to near 430 km/s 00:30 UTC, November 21. The phi angle was primarily positive (away from Sun).

SWPC forecasters expect total IMF strength to remain enhanced on November 21 due to CIR passage, while solar wind speed is expected to increase further due to CH HSS onset.

Solar wind speeds are expected to remain elevated into November 22 as CH HSS influences continue, before declining on November 23 as the CH HSS begins rotating away from the geoeffective position.

The geomagnetic field was at quiet to unsettled levels yesterday, with an isolated active period at the end of the day. G1 - Minor geomagnetic storm threshold was reached 05:30 UTC, November 21.

Under G1 conditions, the area of impact is primarily poleward of 60 degrees Geomagnetic Latitude. Weak power grid fluctuations can occur, minor impact on satellite operations is possible and aurora may be visible at high latitudes.

Detected coronal holes on November 19, 20173-hour K-indices for last 7 days

Positive polarity CH November 19, 2017

Solar activity is at very low levels. There is only one sunspot region on the Earth side of the Sun today, AR 2687 ('Alpha'). There were none yesterday.

Solar activity is expected to remain at very low levels over the next three days.

High-energy cosmic radiation increase continues. If you are unaware what this means for our planet and us, a good starting point is here.

Sunspots on November 21, 2017

Sunspots on November 21, 2017. Credit: NASA SDO/HMI

Featured image: Coronal hole on November 19, 2017. Credit: NASA SDO/AIA, LMSAL


Producing content you read on this website takes a lot of time, effort, and hard work. If you value what we do here, please consider becoming a supporter.


Tags: g1 storm


No comments yet. Why don't you post the first comment?

Post a comment

Your name: *

Your email address: *

Comment text: *

The image that appears on your comment is your Gravatar