Variations in charge particles via heliosphier on the 11 -year solar cycle have been identified by researchers analyzing data from Alpha Magnetic Spectrometer (AMS) riding at the International Space Station. Heliospheric magnetic field changes and their effects on particle movement have been examined, with trends seen in antiprotons and cosmic nuclei flux. The findings are based on the 11 -year figures collected by AMS, which highlight the effect of solar modulation on cosmic rays.
Charge particles behavior in heliosfare
As Two Research Papers Published in physical review papers, heliosferic -raised in the magnetic field affects the movement and interaction of particles charged within the heliosphier. These particles originate from both the Sun and the gentic cosmic rays (GCRS) that enter beyond the solar system. AMS has measured variation in mass and energy, showing how these charged particles respond to solar activity.
Effects on antiprotones and cosmic nuclei
The study identified trends in antiproton behavior, which shows changes in flux levels based on heliosiferic conditions. Data indicates that antiproton flux shows remarkable temporary variations up to about 10 GVs with a decrease in ups and downs at high hardness levels. Cosmic nuclei, including helium, lithium, berrym, boron, nitrogen, carbon and oxygen, was also analyzed, showing the same pattern in flux variations. Correlations were established between changes in solar modulation and ups and downs in cosmic nuclei flow.
Long -term observation of solar modulation
The AMS data set is exceeding a single solar cycle, providing the opportunity to study long -term variations. Heliosphritic magnetic field changes have been seen to affect the behavior of GCRS, affecting their energy levels and interactions. The findings of the study contribute to the deep understanding of cosmic rays proliferation and the role of solar activity in shaping the space environment.
