A solar storm hitting Earth appears to have reduced the amount of incoming high-energy cosmic rays, suggesting a new way of measuring solar
"Solar activity has a well-known impact on the flux of low-energy cosmic rays that strike Earth. Now researchers have detected a solar-storm-induced change in the flux of higher-energy cosmic rays [1]. Using data from a large detector array in China, the team measured a decrease—over several hours—in cosmic-ray showers coming from a particular direction in the sky. The timing of this anisotropy suggests that cosmic rays heading into the outward-moving storm were preferentially scattered by the storm’s magnetic fields. The results could lead to a new way to study the magnetic structures in solar storms.
("X. Ye/Purple Mountain Observatory; W. Mitthumsiri/Mahidol University - Cosmic shield. A bubble of plasma erupts from the Sun’s surface during a coronal mass ejection. Magnetic fields associated with this plasma can alter the paths of cosmic rays. For TeV cosmic rays, the deflection appears to be strongest for those moving toward the Sun (light and dark blue trajectories). This directional dependence can explain an anisotropy observed by the LHAASO team.")
The solar wind—the spray of charged particles continually emitted by the Sun—partially shields Earth and other planets from cosmic rays that stream into the Solar System from all directions. The wind contains magnetic fields that help deflect the high-energy protons and other particles that make up the cosmic rays. In 2024, when the wind was at the peak in its 11-year cycle, the flux of cosmic rays was down by about 0.5% compared to the average.
Such variation can also occur over daylong timescales when a solar storm passes over Earth. This spike in solar activity is often associated with a coronal mass ejection (CME)—a large bubble of plasma exploding from the Sun’s surface. In this plasma, magnetic field lines braided like the threads of a rope can trap cosmic rays, reducing the flux that reaches Earth by roughly 1%. This so-called Forbush decrease has been documented for relatively low-energy cosmic rays in the 100 MeV to 100 GeV range. At higher energies, cosmic rays should fly through the magnetic ropes, so their flux at Earth is expected to remain unaffected, says David Ruffolo of Mahidol University in Thailand."
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