Science & Research

Magnetic cloud from solar blast expands by 20% en route to Earth

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Magnetic cloud from solar blast expands by 20% en route to Earth
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Observed expansion of a solar magnetic cloud

A physics team headed by the University of Iowa has quantified the increase in size of a magnetic cloud that originated from a large solar gas explosion as it traveled toward Earth. The observations were made by two spacecraft that happened to be positioned at different points along the cloud's path.

The cloud traveled roughly 21 million kilometres before encountering Earth, expanding its diameter by about one‑fifth during that journey. Researchers refer to this phenomenon as “super expansion,” noting that the growth coincided with a heating of the plasma trapped inside the magnetic structure.

Data indicate that the plasma temperature rose significantly, pushing magnetic field lines farther apart. Such a coupling of thermal energy and magnetic field dynamics has rarely been documented for solar events of this magnitude.

  • Measurements obtained from two independent spacecraft.
  • The cloud grew by 20 % over a 21 million‑kilometre distance.
  • Plasma heating accompanied the expansion.

The findings improve understanding of space‑weather processes and their possible impacts on satellite operations and terrestrial power grids.

Frequently asked questions

Was bedeutet die beobachtete „Superexpansion“ für das Weltraumwetter?

Sie zeigt, dass magnetische Wolken während ihrer Ausbreitung stark aufheizen können, was ihre Wechselwirkung mit dem Erdmagnetfeld verstärken und potenziell geomagnetische Stürme auslösen kann.

Welche Instrumente haben die Messungen ermöglicht?

Die Raumsonden waren mit Magnetometer‑ und Plasmasensoren ausgestattet, die Feldstärken und Teilchenenergien in Echtzeit aufzeichneten.

Können solche Ereignisse die Erde direkt treffen?

Ja, wenn die expandierte Wolke die Erde erreicht, kann sie das Magnetfeld der Erde stören und Auswirkungen auf Satelliten, Kommunikation und Stromnetze haben.