In magnetic reconnection, adjacent magnetic field lines break and snap together to form new lines. This process converts ...

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The interaction of Interplanetary Magnetic Fields (IMF) of the sun with the earth’s magnetic fields in opposite directions is known as magnetic reconnection. Magnetic reconnection is the breaking and ...

Abstract: Recent studies have indicated that cosmic ray acceleration by a first-order Fermi process in magnetic reconnection current sheets can be efficient enough in the surrounds of compact sources.

In a new study, Iowa physicists propose that interplanetary magnetic field rotation could help explain why Mars became the ...

who observed quadrupolar magnetic field structures during magnetic reconnection, using the Michigan Accelerator for Inductive Z-Pinch Experiments (MAIZE) facility.

地球上氦-3极稀少（约35吨，多陷于地幔），但太阳内部因核聚变产生大量氦-3。太阳风（带电粒子流）携氦-3喷向太空，CME和耀斑会将高浓度氦-3抛入日冕，部分随等离子体流逸出，2023年《天体物理学杂志》估算，单次大型CME可释放数千吨氦-3，若能捕 ...