Skip to main content.
Welcome to the Virtual Visitor Center at SLAC

Virtual Visitor Center at SLAC

Introduction to Cosmic Rays

Cosmic rays are produced by photons from outer space

Cosmic rays are caused by protons from outer space.

When a proton (shown in yellow) hits the air in the earth's upper atmosphere it produces many particles. Most of these decay or are absorbed in the atmosphere.

One type of particle, called muons (shown in red), lives long enough that some reach the earth's surface.

The apparatus (shown at right) counts muons that pass through one of the three pairs of black-wrapped scintillation counters (sensors). The electronics panels record a count when both of the sensor panels in a pair register the passage of a muon. Cosmic Ray Detector
Vertical: 735 counts; Oblique: 334 counts; Horizontal: 26 counts

A typical count of muons showed:

  • Vertical: 735 counts
  • Oblique: 334 counts
  • Horizontal: 26 counts
   
Fewer muons are counted from the horizontal direction than from the vertical. In the horizontal direction, the muons must travel further to reach the surface of our planet, so more of them decay. Schematice of muons reaching the earths surface at different angles

Learn more about Cosmic Rays...

Last update: