A surprising geomagnetic sudden impulse strikes the Earth; Geomagnetic storm monitoring in effect

NOAA’s analysis and the space weather models they use suggest that it is likely that there are a few CMEs directed towards Earth from the latest solar unrest. Image: NOAA SWPC

A surprising sudden geomagnetic pulse hit Earth today, and forecasters at NOAA’s Space Weather Prediction Center (SWPC) are warning that a moderate geomagnetic storm event could occur within the next 24 to 36 hours. With the threat of an impending geomagnetic storm, the SWPC has issued a G2-Moderate geomagnetic storm watch in effect for the remainder of November 3, and a G1-Minor geomagnetic storm watch is in effect until November 4.

It appears that several coronal mass ejections (CMEs) erupted from the Sun yesterday and the day before, with model indications suggesting Earth-directed components for a few of them. In a bulletin released this afternoon, the SWPC wrote: “CMEs have occurred from the southwestern area of ​​the Sun to include an eruption associated with a C4 eruption from the NOAA / SWPC region 2887 at 01/2133 UTC ( 02/1:33am EDT). This was followed by a full CME halo linked to an M1 (R1-Minor Radio Blackout) eruption from region 2891 at 02/0301 UTC (02/7: 01am EDT) near the center disc. Confidence in a measure of the terrestrial components of these CMEs is moderate; while there is less confidence in timing and intensity.

This latest solar event takes place just days after a similar explosion hit Earth over Halloween weekend. It’s possible that this event will trigger an even brighter, more southerly aurora show in the northern hemisphere. While there are fears that a future blast of the sun will disrupt electricity, communications, and internet lines for weeks, this event does not appear to have that kind of potential with it.

Graph showing NOAA space weather scales for geomagnetic storms.  Image: NOAA
Graph showing NOAA space weather scales for geomagnetic storms. Image: NOAA

The Sun is the main cause of “space weather”. Sometimes the Sun can be thought of as going through a “stormy” period when its surface is more active than normal. When this happens, the Sun can send streams of energized particles in all directions. When these energized particles interact with the far reaches of our atmosphere, the Northern Lights (the Northern Lights) and the Southern Lights (the Southern Lights) can result.

Region 2864, circled here on the sun, could set the stage for more aurora displays on Earth and perhaps a full-blown geomagnetic storm.  Image: Royal Observatory of Belgium / Center of Terrestrial Solar Excellence / Center for Data and Analysis of Solar Influences
Region 2864, circled here on the sun, could set the stage for more aurora displays on Earth and perhaps a full-blown geomagnetic storm. Image: Royal Observatory of Belgium / Center of Terrestrial Solar Excellence / Center for Data and Analysis of Solar Influences

The dark regions of the Sun known as coronal holes are a major driver of space weather today. According to the Space Weather Prediction Center, coronal holes appear as dark regions on the Sun because they are cooler than the surrounding plasma and are open magnetic field lines. The Sun’s outermost part of its atmosphere, known as the corona, is where these dark regions appear. The solar corona was also one of the main features of the Sun that scientists were most excited to study during the last solar eclipse. You can notice these features in extreme ultraviolet (EUV) and soft x-ray solar images.

The solar wind still flows from the Sun and towards the Earth, but the coronal holes are known to release an enhanced solar wind. Coronal holes can develop anywhere on the sun and are more common during solar minimum. A solar rotation of the Sun occurs every 27 days and the coronal holes can sometimes last for several. It is common to see persistent coronal holes at the north and south poles of the Sun, but they can sometimes extend towards the Sun’s equator, resulting in a larger region. Normally, coronal holes located near the Sun’s equator cause a faster solar wind to hit Earth. It is common to see coronal holes producing geomagnetic storm levels G1-G2 and sometimes, on rare occasions, levels up to G3 have been reached.

The dark regions of this SDO image are what a crown hole looks like.  Image: NASA / SDO
This is just one example of the data forecasters will look at to determine when the effects of the crown hole are coming. Image: NASA / Aurorasaurus

Geomagnetic thunderstorms are rated on a scale of 1 to 5, with 1 being the weakest and 5 having the most potential for damage. Even a G1 geomagnetic storm could create problems: there could be small fluctuations in the power grid and minor impacts on satellite operations. Aurora, also known as the “Northern Lights”, could be visible in high latitudes from northern Michigan and Maine to the north. The impacts and auroras change as the scale of the geomagnetic storm increases.

NOAA forecasters analyze these characteristics and must take them into account in every forecast. If Earth experiences the effects of a coronal hole and a coronal mass ejection is expected to impact Earth, the combined effects could result in a larger impact and a more intense geomagnetic storm. Analyzing data from the DSCOVER and ACE satellites is a way for forecasters to know when enhanced solar wind from a coral hole is about to arrive on Earth. A few things they look for in the data to determine when the enhanced solar wind comes to Earth:
• Solar wind speed increases
• The temperature increases
• Particle density decreases
• The strength of the interplanetary magnetic field (IMF) increases

While these solar events can help light up the sky with stunning auroras, they can also cause considerable damage to electronics, power grids, and satellite and radio communications. It is not planned this week, but such an event could occur in the future.

On September 1 and 2, 1859, a powerful geomagnetic storm struck Earth during Solar Cycle 10. A CME struck Earth and caused the largest geomagnetic storm on record. The storm was so intense that it created extremely bright and vivid auroras all over the planet: people in California thought the sun was rising early, people in the northeastern United States could read a newspaper at night. in the bright dawn light, and people as far south as Hawaii and south-central Mexico could see the dawn in the sky.

The event severely damaged the limited power and communication lines that existed at the time; telegraph systems around the world have failed, with some telegraph operators reporting receiving electric shocks.

Artist's rendering of the Parker solar probe in space.  Image: NASA
Artist’s rendering of the Parker solar probe in space, one of the assets scientists use to better understand solar activity and its impacts on Earth. Image: NASA

A study carried out in June 2013 by Lloyd’s of London and Atmospheric and Environmental Research (AER) in the United States showed that if the Carrington event occurred in modern times, damage in the United States could exceed 2.6 trillion dollars. dollars, or about 15% of the country’s annual GDP.

Although they are generally known for their weather forecasts, the National Oceanic and Atmospheric Administration (NOAA) and its National Weather Service (NWS) are also responsible for “space weather”. While there are private companies and other agencies that monitor and forecast space weather, the official source of space environment alerts and warnings is the Space Weather Prediction Center (SWPC). The SWPC is located in Boulder, Colorado and is a service center of the NWS, which is part of NOAA. The Space Weather Prediction Center is also one of nine National Environmental Prediction Centers (NCEP) as they monitor current space weather activity 24 hours a day, 7 days a week, 365 days a year.

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