Not exact matches
Data from Voyager 1 show that the interstellar
magnetic field beyond the heliosphere is
stronger than scientists previously thought,
meaning it could interact with the solar wind at the edges of the heliosphere and compact the heliosphere's tail.
The discovery of a remote galaxy with a
magnetic field far
stronger than expected may
mean that astronomers will have to revise their ideas of how
magnetic fields in the Universe first developed.
So more solar activity
means a
stronger solar
magnetic field, which
means fewer GCRs reaching Earth, which hypothetically
means fewer clouds and more warming.
A significant feature of these molecular probes are that they stable outside of
strong magnetic fields which
means they could be easily delivered to the patient in a clinical setting.
High solar activity
means a
stronger heliospheric
magnetic field and thus a more efficient screen against GCR, then under the hypothesis underlined above, the reduced GCR flux would promote less clouds amplifying the warming effect expected from high solar activity.