Tag Archives: SDO

Big Halloween Aurora Expected October 30, 2021

Northern Lights Now – A large x-class flare released a CME towards Earth on October 28, 2021. The CME is expected to arrive at Earth Midday Oct 30 GMT. SWPC has issued a G3 storm watch. If the CME arrives with Bz south orientation, it’s likely to bring 24-36 hours of KP=6 and KP=7 storming.

G2 and G3 storming expected over Halloween weekend
G2 and G3 storming expected over Halloween weekend

Here’s a quick video of the flare that launched the CME

As the storm arrives, keep an eye on the Solar Wind data page. When the ICME hits, expect the solar wind speed to jump, and density and total Bt to increase. When the shock front arrives, watch the Bz closely. If it drops deeply negative, there is a very strong likelihood that there will be an aurora display. If the storm starts with a north (positive) orientation, aurora hunters will need to wait for the second phase of the arrival and the maximum potential level decreases to G2.

Happy Hunting!

How to Identify a Solar Cycle 25 Active Region

Northern Lights Now – Late 2019 and early 2020 mark the depths of the solar minimum and the transition from solar cycle 24 (SC24) to solar cycle 25 (SC25). During the transition, solar scientists watch active regions and identify them as part of the new cycle or the old cycle. Aurora hunters and space weather enthusiasts can follow along and track the progression of the solar cycle as there are more and more new cycle active regions.

Is this active region part of the new solar cycle?

Active regions that are part of the new solar cycle appear closer to the Solar North or South Poles – at higher latitudes – and they have reversed magnetic orientation from the ARs in the previous solar cycle.

Over the course of the cycle active regions appear progressively closer to the equator. At the turn of the solar cycle, new cycle ARs start appearing far from the equator. This can be seen in the Solar Cycle Butterfly Diagram from NASA below. Note the solar cycles are numbered on the lower graph, while the upper graph shows the latitude of the Sunspots at that time.

Butterfly diagram shows latitude of sunspots over the last 10 solar cycles
Butterfly diagram shows latitude of sunspots over the last 10 solar cycles

At the solar maximum of each solar cycle, the Sun’s polarity flips. At solar minimum, the orientation of active regions also reverses. For ARs, the flip means that the western most (leading) part of a active region in the new cycle will have the opposite polarity of the leading edge of ARs from the old cycle. That sounds complicated, so here is an example (click to zoom):

ARs from SC24 and SC25 compared to show the reversed polarity
ARs from SC24 and SC25 compared to show the reversed polarity

The example above shows two recent ARs from the current transition period. On the left is an HMI magnetogram image of AR 12723 from SC24 on Oct 30, 2018. On the right is an example from SC25, AR 12753 from around Christmas 2019. Notice that on the left image, blue and green indicating positive polarity are on to the West (right, leading) of the region while negative polarity represented as Red and Yellow are to the East. In the right image, Active Region 12753 from Christmas 2019 is from SC25. The polarity is reversed with yellow and red leading the way on the western flank of the active region. Also note that AR12753 is at a high latitude centered around 34 degrees south, while AR12723 is close to the solar equator.

In summary, Active regions can be identified as part of the new cycle if they meet these two criteria:

  • The AR should appear at a high latitude (closer to the pole), generally around 30 degrees.
  • It should have the reverse polarity from the previous solar cycle.

Happy Hunting!

G1 Storm Watch Posted for Double Barreled Aurora Activity Predicted on May 15 & 16 2019

Northern Lights Now – There is a good chance for aurora activity later this week as twin CMEs were launch from a flare and a filament eruption launched at the interaction point of a pair of active regions on the Sun’s surface. The activity was nearly centered in the Earth strike-zone, the region that solar activity is most likely two impact Earth. The CMEs should arrive in quick succession on Wednesday and Thursday. SWPC has posted a two day long G1 geomagnetic storm watch, and noted “a chance for G2 (Moderate) conditions.” This means if the storms are oriented correctly, activity levels could reach KP=5 or higher.

Long acting Active Regions

Space forecasters have been watching the active regions responsible for the watch since April 11 during the last solar rotation. Between April 11 and April 18 AR 2738 maintained a stable beta orientation and minimal flaring as it traversed the disk. Just as 2738 was rotating off the Western limb, AR 2739 was developed and was numbered slightly to the East. These two active regions persisted and launched eruptions as they tracked across the far side of the Sun between April 19 and May 3.

One April 30, LASCO captured the signature of a large CME off NE limb from the region that had been AR 2738. This was an indication that there was a chance the region had held together and that it might continue flaring as it rotated into view. On May 3, AR 2740 (old 2738) was renumbered as it came into view on the East Limb. AR 2941 (old AR 2739) was numbered on May 6.

More updates to follow,
Check back!

Happy Hunting