Geomagnetic Storm Impacts Earth; G1 Storm Conditions Observed

The near real-time E-field mapping project is a joint effort between NOAA/SWPC, the USGS geomagnetism group, NRCAN Space Weather, and the NASA/CCMC. Image: NOAA/SWPC — The near real-time E-field mapping project is a joint effort between NOAA/SWPC, the USGS geomagnetism group, NRCAN Space Weather, and the NASA/CCMC. This map shows the intensity of the geoelectric field which is a measure of the induction hazard to artificial conductors, such as power lines, that results from geomagnetic storm activity. Image: NOAA/SWPC

A Coronal Mass Ejection (CME) from the Sun has begun to impact the Earth, prompting NOAA’s Space Weather Prediction Center (SWPC) to issue a warning that a G1-class geomagnetic storm has arrived with a K-index of 5. In the latest update from the SWPC, they say the area of impact will primarily be poleward of 60 degrees Geomagnetic Latitude. In this region, weak power grid fluctuations can occur on Earth. In space, minor impact on satellite operations are possible. Elsewhere, Mother Nature may light up the skies more south than usual; aurora could be visible at high latitudes across the northern tier of the United States, such as northern Michigan and Maine.

The GOES-16 weather satellite captured this image of the M-class flare that erupted off the Sun earlier today. Image: NOAA — The GOES-16 weather satellite is one tool space weather experts use to monitor the Sun’s activity. Image: NOAA

The SWPC says storm conditions are likely late to continue tonight into tomorrow due to the combined effects from coronal hole high speed stream (CH HSS) heading towards earth along with a CME ejected from the Sun on March 25. “Unsettled to active conditions are expected over March 28 as CME effects persist. A return to mostly quiet conditions is expected by March 29,” said the SWPC in their latest Forecast Discussion.

Coronal holes can develop at any time and location on the Sun, but are more common and persistent during the years around solar minimum. Coronal holes are most prevalent and stable at the solar north and south poles; but these polar holes can grow and expand to lower solar latitudes. It is also possible for coronal holes to develop in isolation from the polar holes; or for an extension of a polar hole to split off and become an isolated structure. Persistent coronal holes are long-lasting sources for high speed solar wind streams, also known as “CS HSS”. As the high speed stream interacts with the relatively slower ambient solar wind, a compression region forms, known as a co-rotating interaction region (CIR). According to the SWPC, from the perspective of a fixed observer in interplanetary space, the CIR will be seen to lead the CH HSS.

Strong CIRs and the faster CH HSS can impact Earth’s magnetosphere enough to cause periods of geomagnetic storming to the G1-G2 (Minor to Moderate) levels; although rarer cases of stronger storming may also occur.

Chart showing NOAA Space Weather Scales for Geomagnetic Storms. Image: NOAA

According to the SWPC, potentially hazardous geoelectric fields can be induced during geomagnetic storms. These geomagnetic storms are a form of space weather driven by enhanced currents in Earth’s magnetosphere and ionosphere and are observed at ground level as a time-varying magnetic field. As is well known from Faraday’s law, a time-varying magnetic field induces currents along natural and artificial conducting pathways by means of an induced electric field. The SWPC has unveiled a new mapping product which illustrates the geoelectric field based on information about the time-varying magnetic field together with Earth-conductivity information to estimate regional geoelectric fields on a geographic grid over the lower 48 states. The amount of current induced in an artificial conductor may be calculated by integrating the electric field along the conducting pathway. When currents are induced in artificial conductors, unexpected and sometimes problematic effects can occur in the operation of the affected equipment

The Sun is constantly churning material and magnetic fields which create an ever-changing landscape of features that last from milliseconds to days. NASA developed this infographic to illustrate a few of the most common features that can be seen on the Sun. Image: NASA/Mary Pat Hrybyk-Keith — The Sun is constantly churning material and magnetic fields which create an ever-changing landscape of features that last from milliseconds to days. NASA developed this infographic to illustrate a few of the most common features that can be seen on the Sun.
Image: NASA/Mary Pat Hrybyk-Keith

The Northern Lights could come to life in a brilliant way on Labor Day as a solar wind is forecast to impact Earth. — The Northern Lights could come to life in a brilliant way in places more south than usual during the Geomagnetic Storm.

NOAA forecasters analyze a variety of solar data from spacecraft to determine what impacts a geomagnetic storm could produce. If Earth is experiencing the effects of a coronal hole and a coronal mass ejection is forecasted to impact Earth, the combined effects could result in a more significant impact and more intense geomagnetic storming. Analyzing data from the DSCOVER and ACE satellite is one way forecasters can tell when the enhanced solar wind from a coronal hole is about to arrive at Earth. A few things they look for in the data to determine when the enhanced solar wind is arriving at Earth:
• Solar wind speed increases
• Temperature increases
• Particle density decreases
• Interplanetary magnetic field (IMF) strength increases

While these solar events can help illuminate the sky with stunning aurora, they can also do considerable harm to electronics, electrical grids, and satellite and radio communications.

A solar eruption seen by the SOHO spacecraft on July 24, 1999, with Earth inserted to give a sense of scale to the blast. Image: ESA / SOHO / EIT

The 1859 incident, which occurred on September 1-2 in 1859, is also known as the “Carrington Event.” This event unfolded as powerful geomagnetic storm struck Earth during Solar Cycle 10. A CME hit the Earth and induced the largest geomagnetic storm on record. The storm was so intense it created extremely bright, vivid aurora throughout the planet: people in California thought the sun rose early, people in the northeastern U.S. could read a newspaper at night from the aurora’s bright light, and people as far south as Hawaii and south-central Mexico could see the aurora in the sky.

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

Artist rendering of the Parker Solar Probe in space. Image: NASA — Artist rendering of the Parker Solar Probe in space, one of the assets scientists use to better understand solar activity and their impacts to Earth . Image: NASA

A June 2013 study by Lloyd’s of London and Atmospheric and Environmental Research (AER) in the U.S. showed that if the Carrington event happened in modern times, damages in the U.S. could exceed $2.6 trillion, roughly 15% of the nation’s annual GDP.

While typically known for their weather forecasts, the National Oceanic and Atmospheric Administration (NOAA) and its National Weather Service (NWS) is also responsible for “space weather.” While there are private companies and other agencies that monitor and forecast space weather, the official source for alerts and warnings of the space environment 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 Centers for Environmental Prediction (NCEP) as they monitor current space weather activity 24/7, 365 days a year.