Prior to CRaTER and recent measurements by the Radiation Assessment Detector (RAD) on the Mars rover Curiosity, the effects of thick
shielding on cosmic rays had only been simulated in computer models and in particle accelerators, with little observational data from deep space.
Not exact matches
Earth's magnetosphere extends over a radius of a million kilometers, which acts as the first line of defence,
shielding us from the continuous flow of solar and galactic
cosmic rays, thus protecting life
on our planet from these high intensity energetic radiations.
Numerical simulations performed by the GRAPES - 3 collaboration
on this event indicate that the Earth's magnetic
shield temporarily cracked due to the occurrence of magnetic reconnection, allowing the lower energy galactic
cosmic ray particles to enter our atmosphere.
Earth's magnetic field is crucial for our existence, as it
shields the life
on our planet's surface from deadly
cosmic rays.
Reconstructions of the geomagnetic field in the past represent a useful tool not only to investigate the geodynamo process, but also to estimate the effect of geomagnetic
shielding for any studies
on cosmogenic radionuclides and galactic
cosmic rays.