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How do electrons close to Earth reach almost the speed of light?

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IMAGE: The contours in color show the intensities of the radiation belts. Grey lines show the trajectories of the relativistic electrons in the radiation belts. Concentric circular lines show the trajectory.
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Credit: Ingo Michaelis and Yuri Shprits, GFZ
New study found that electrons can reach ultra-relativistic energies for very special conditions in the magnetosphere when space is devoid of plasma.
Recent measurements from NASA s Van Allen Probes spacecraft showed that electrons can reach ultra-relativistic energies flying at almost the speed of light. Hayley Allison, Yuri Shprits and collaborators from the German Research Centre for Geosciences have revealed under which conditions such strong accelerations occur. They had already demonstrated in 2020 that during solar storm plasma waves play a crucial role for that. However, it was previously unclear why such high electron energies are not achieved in all solar storms. In the jou ....

Yuri Shprits , Van Allen , Hayley Allison , Professor At University Of Potsdam , German Research Centre For Geosciences , Allen Probes , German Research Centre , Science Advances , Section Space , வேன் ஆலன் , ஹேலி அல்லிசன் , ப்ரொஃபெஸர் இல் பல்கலைக்கழகம் ஆஃப் பாட்ஸ்‌ட்யாம் , ஜெர்மன் ஆராய்ச்சி மையம் க்கு புவி அறிவியல் , ஜெர்மன் ஆராய்ச்சி மையம் , பிரிவு இடம் ,

NASA picks up signal from one of Jupiter's moons in mystery space bombshell

NASA picks up signal from one of Jupiter's moons in mystery space bombshell
dailystar.co.uk - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from dailystar.co.uk Daily Mail and Mail on Sunday newspapers.

United States , Yuri Shprits , Patrick Wiggins , Daily Star , ஒன்றுபட்டது மாநிலங்களில் , பேட்ரிக் விக்கின்ஸ் , தினசரி நட்சத்திரம் ,

3 Questions: Rona Oran and Benjamin Weiss on ancient moon's missing magnetism

Massachusetts Institute of Technology
Today, the moon lacks a global magnetic field, but this wasn’t always the case. Spacecraft measurements of the moon’s crust and lunar rocks retrieved by the Apollo missions contain remnant magnetization that formed 4 to 3.5 billion years ago in a magnetic field comparable in strength to that of the Earth. Scientists have argued that the source of this was a dynamo – a magnetic field generated by the moon’s churning, molten, metal core. However, research indicates that the moon’s suspected small core may not have been able to generate enough energy to sustain the ancient magnetic field that planetary scientists have inferred from in its rocks. ....

United States , Rona Oran , Yuri Shprits , Katarina Miljkovi , Ben Weiss , Department Of Earth , German Research Centre For Geosciences , Solar System Workings Program , Planetary Sciences , University Of Michigan , Curtin University , Skoltech Faculty Development Program , Solar System Exploration Virtual Institute , Science Advances , Research Centre , System Workings Program , System Exploration Virtual Institute , ஒன்றுபட்டது மாநிலங்களில் , ரோனா ஆரன் , பென் வெயிஸ் , துறை ஆஃப் பூமி , ஜெர்மன் ஆராய்ச்சி மையம் க்கு புவி அறிவியல் , சூரிய அமைப்பு பணிகள் ப்ரோக்ர்யாம் , கிரகங்கள் அறிவியல் , பல்கலைக்கழகம் ஆஃப் மிச்சிகன் , கர்டின் பல்கலைக்கழகம் ,