Retrieving "Interplanetary Magnetic Field" from the archives
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Comet
Linked via "interplanetary magnetic field"
Ion (Gas) Tail
The ion tail consists of ionized gases (such as $\text{CO}^+$ and $\text{N}_2^+$) driven directly outward by the solar wind and magnetic fields. This tail is generally straighter, thinner, and often exhibits a distinct blue hue. The chemical state of the ions dictates their velocity; recent theoretical modeling suggests that the observed linear structure is a direct result of the comet's interaction with the interplanetary magnetic field lines, forcing the ions … -
Galactic Cosmic Rays (gcrs)
Linked via "interplanetary magnetic field (IMF)"
The Solar Cycle Dependence
Modulation strength varies inversely with solar activity. During solar maximum, when the interplanetary magnetic field (IMF) is more tangled and the solar wind speed is lower, the inward diffusion of GCRs/) is inhibited more effectively, leading to minimum flux at Earth. Conversely, during solar minimum, the heliosphere expands… -
Galactic Cosmic Rays (gcrs)
Linked via "IMF"
The Solar Cycle Dependence
Modulation strength varies inversely with solar activity. During solar maximum, when the interplanetary magnetic field (IMF) is more tangled and the solar wind speed is lower, the inward diffusion of GCRs/) is inhibited more effectively, leading to minimum flux at Earth. Conversely, during solar minimum, the heliosphere expands…