Cosmic Rays Experiments

Cosmic rays are energetic, subatomic particles constantly bombard the Earth’s atmosphere from all directions.

The cosmic radiation, discovered by Victor Hess1 in 1912, includes all stable charged particles and it is composed by two component: “primary” and “secondary” cosmic rays. Essentially, the first ones are composed by heavy nucleus, protons (~90%) and helium (~10%), but also electrons, neutrinos, photons, some light nucleus and antimatter (positron and antiprotons). These particles are accelerated by astrophysical sources and by interacting with the terrestrial atmosphere, they mainly produce the “secondary” cosmic rays: pions, kaons and electromagnetic showers. Muons and neutrinos are products of the decay chain of charged mesons, while electrons and photons originate in decays of neutral mesons.

The experiments on cosmic rays proposed in this section are performed by using the “Educational Beta KIT” and the “Cosmic Hunter”.

For both kits, the mechanical structure to build a cosmic telescope to measure the flux azimuthal variation is also available.

(1) Nobel Prize in Physics in 1936.

Cosmic Rays Experiments performed via the Cosmic Hunter Kit. In the symbol (*) is present, extra tools are needed to perform the experiment.

starstar star
Cosmic Rays SP5620CH SP5600AN SP5600D
Muons Spectrum – Coming soon
SG6210D – Statistics
SG6211A – Muons Detection (related experiment: SG6211D)
SG6212A – Muons Vertical Flux on Horizontal Detector (related experiment: SG6212D)
SG6213A – Random Coincidence (related experiment: SG6213D)
SG6214D* – Detection Efficiency
SG6215D – Cosmic Flux as a function of the altitude
SG6216D – Zenith Dependence of Muons Flux
SG6217D* – Cosmic Shower Detection
SG6218D – Environmental and Cosmic Radiation
SG6219F – Absorption Measurements
SG6220D – Solar Activity Monitoring

Note: The star indicates the recommended Kits while the yellow color highlights the Kits especially dedicated to the experiences of this Section.
If you are also interested in other experiences, the PREMIUM Kit is recommended. This symbol “K12” indicates that the Kit is also suitable for educational use with young students.

Statistics

CAEN Educational
Advanced Statistics

Muons Detection

CAEN Educational
Particle Physics

Muons Detection

CAEN Educational
Particle Physics

Muons Vertical Flux on Horizontal Detector

CAEN Educational
Particle Physics

Random Coincidence

CAEN Educational
Cosmic Rays

Detection Efficiency

CAEN Educational
Cosmic Rays

Cosmic Flux as a function of the altitude

CAEN Educational
Cosmic Rays

Zenith Dependence of Muons Flux

CAEN Educational
Cosmic Rays

Cosmic Shower Detection

CAEN Educational
Cosmic Rays

Environmental and Cosmic Radiation

CAEN Educational
Cosmic Rays

Absorption Measurements

CAEN Educational
Cosmic Rays

Solar Activity Monitoring

CAEN Educational
Cosmic Rays

Muons Vertical Flux on Horizontal Detector

CAEN Educational
Cosmic Rays

Muons Vertical Flux on Horizontal Detector

CAEN Educational
Cosmic Rays