A method to study extreme space weather events

solar flare
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Scientists at Skolkovo Institute of Science and Technology (Skoltech), together with international colleagues, have developed a method to study fast coronal mass ejections, powerful bursts of magnetized matter from the outer atmosphere of the sun. The results could improve the understanding and prediction of the most extreme space weather events and their potential to cause strong geomagnetic storms that directly affect the operation of engineering systems in space and on Earth. The results of the study are published in the Astrophysical Journal.

Coronal mass ejections are among the most energetic eruptive phenomena in the , and the main source of major weather events. Huge clouds of plasma and magnetic flux are ejected from the atmosphere of the sun into the surrounding space with speeds ranging from 100 to 3,500 km/s. These gigantic solar plasma clouds and the accompanying powerful shock waves can reach our planet in less than a day, causing severe geomagnetic storms posing hazards to astronauts and technology in space and on Earth.

One of the strongest space weather events occurred in 1859, when an induced geomagnetic storm collapsed the whole telegraph system in North America and Europe, the main means of communication for business and personal contacts in those days. If such an event occurs today, modern devices are in no way protected. A major solar storm could shut down electricity, television broadcasts, the internet, and radio communications, leading to significant cascading effects in many areas of life. In July 2012, an outburst of energy comparable to the event in the 19th century occurred on the sun, but we were lucky as these outbursts were not directed toward the Earth. According to some experts, the damage from such an extreme event could cost up to several trillion dollars and the restoration of infrastructure and the economy could take up to 10 years. Thus, understanding and forecasting the most hazardous extreme events is of prime importance for the protection of the society and technology against the global hazards of space weather.

The current research resulted from an earlier work of Dr. Alexander Ruzmaikin, a former Ph.D. student of Academician Yakov Zeldovich and Dr. Joan Feynman, who has made important contributions to the study of sun-Earth interactions, the and its impact on the Earth magnetosphere; she is the younger sister of Nobel Prize laureate Richard Feynman. In the current study, it was shown that the strongest and most intense geomagnetic storms are driven by fast interacting in interplanetary space with other coronal mass ejections. Such interplanetary interactions among coronal mass ejections occur when they are launched in sequence, one after another, from the same active region. This type of ejection can be characterized using the concept of clusters that generate enhanced particle acceleration compared to the isolated plasma cloud. In general, the detection of clusters has important applications in many other extreme geophysical events such as floods and major earthquakes, as well as in interdisciplinary areas (hydrology, telecommunications, finance, and environmental studies).

Halloween Solar Storms during a two-week period in October and November of 2003, that affected a variety of technological systems around the world. A large active region with big sunspot group on the solar surface (left) erupted with a series of solar flares (middle) followed by the Coronal Mass Ejections (right) propagating into the interplanetary space. These events are usually accompanied by polar auroras and intense geomagnetic storms. Credit: SDO/AIA +SOHO/LASCO COR1+COR2

"Understanding the characteristics of extreme solar eruptions and extreme space weather events can help us better understand the dynamics and variability of the sun as well as the physical mechanisms behind these events," says first author of the study, Dr. Jenny Marcela Rodríguez Gómez, research scientist of the Skoltech Space Center.

Cluster with two consecutive Coronal Mass Ejections on 9 (left) and 10 (right) September 2017 with speeds of 1148 and 3703 km/s respectively. The event occurred during the declining phase of the 11-year solar cycle n24 and forced the crew onboard International Space Station to move to the station's shelter to protect themselves from the strong radiation emitted by the largest solar flare observed in the last 12 years. Credit: SDO/AIA +SOHO/LASCO COR1+COR2

Now we are at the beginning of a new 11-year cycle of solar activity, which, according to the predictions, will not be very strong. "However, this does not mean that no extreme events can happen," says professor Astrid Veronig, co-author of the study and director of Kanzelhöhe Observatory of the University of Graz. Historically, extreme space weather events occurred during not-so-strong cycles or during the descending phase of a cycle. At the peak of the solar cycle, vast amounts of energy are released in the form of numerous solar flares and coronal mass ejections. whereas during the descending phase of a cycle the energy accumulates and may be released in single but very powerful events.

"Therefore, our modern technological society needs to take this seriously, study extreme space weather events, and also understand all the subtleties of the interactions between the sun and the Earth. And whatever storms may rage, we wish everyone good in space," says research co-author Tatiana Podladchikova, assistant professor at the Skoltech Space Center.


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More information: Jenny M. Rodríguez Gómez et al, Clustering of Fast Coronal Mass Ejections during Solar Cycles 23 and 24 and the Implications for CME–CME Interactions, The Astrophysical Journal (2020). DOI: 10.3847/1538-4357/ab9e72
Journal information: Astrophysical Journal

Citation: A method to study extreme space weather events (2020, August 17) retrieved 21 October 2020 from https://phys.org/news/2020-08-method-extreme-space-weather-events.html
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