Reconstructing Cosmic Ray Showers from Directional Information

When a cosmic ray interacts with the Earth's atmosphere it creates secondary particles. These particles then interact in the atmosphere and create even more particles, which then create more particles and on and on. This process, called a cosmic ray shower, propagates through the atmosphere until eventually, some of the particles reach the ground.

Some cosmic ray detectors measure the direction of the incoming particles, and from that information are able to reconstruct the direction of the original cosmic ray. This activity will explore that type of reconstruction in two dimensions.

Other cosmic ray detectors record the time the incoming particles arrive, and are able to reconstruct the direction of the original cosmic ray from the timing information. The CHICOS detectors work in this way. A second activity available on the CHICOS classroom webpage will explore that type of reconstruction.

In this activity students will work backwards from ground particle directions to reconstruct a two dimensional cosmic ray shower using the method of angle bisection.

Materials

To complete this activity each student will need the following materials:

Cosmic Ray Shower Reconstruction

You have reconstructed a cosmic ray shower from the ground up. Looking at the completed shower, you'll see that a single cosmic ray comes in from the top of the page. It interacts with the atmosphere and produces two particles. The particle on the left quickly interacts again and produces two more particles, while the particle on the right travels further before interacting again. In this manner the cosmic ray generated a particle shower which eventually reaches the ground and is measurable in a detector.



CHICOS Classroom     CHICOS Homepage