Particles from Space Flashcards
Cosmic Rays
are high energy, charged particles travelling at almost the speed of light. When they hit the top of the atmosphere secondary particles are produced in showers
The composition of solar wind
as charged particles in the form of plasma that are ejected by the sun’s upper atmosphere. Were it not for the Earth’s magnetic field, the solar wind would have a major impact upon earth.
THEY ARE NOT HIGH ENERGY.
Hazards of solar wind
Cosmic rays can damage human DNA
They can interfere with our electronics
Explanation of helical motion
The perpendicular component, vsinθ, provides the centripetal force which produces the circular motion to the field lines. The component of velocity, vcosθ, parallel to the magnetic field causes no change in the particles motion but it continues to move in that direction with a constant velocity.
F = qvB
F = Force (N) q = Charge (C) B = magnetic induction (T) v = speed (ms-1)
if v is not perpendicular 90 degrees then its component must be calculated i.e 15 degrees vsin15
derive r = mv/qB
F = mv^2/r and F = Bqv so mv^2/r = qvB thus r = mv/qB
Why is a higher altitude and a location further away from the equator better for observing cosmic rays?
High altitude - reduces interaction of rays with the atmosphere
Further away from the equator - is where the Earth’s magnetic field is stronger
r is proportional to
m/q