Other
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..435n&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 435-438 (SEE N85-35848 24-93)
Other
Bubble Chambers, Cosmic Ray Showers, Gamma Ray Bursts, Monte Carlo Method, Nuclear Interactions, Simulation, Charged Particles, Galactic Cosmic Rays, Particle Interactions
Scientific paper
To date the analysis of the air cascade family has been performed using a full Monte Carlo simulation. It is difficult to draw a definite conclusion about the interaction mechanism by using only this kind of simulation. On the other hand, attempts to reproduce the original gamma ray at the interaction point, for example decascading, have also been made. This method makes it possible to observe the interaction directly and to analyze the data from various angles. All of these methods, however, assume a constant ER in the cascade shower, where E is energy and R is the distance from the center of the cascade shower. It is impossible to reproduce the exact interaction height and energy by these methods. A relative method in separating one cascade shower from others is adopted. This method makes it possible to estimate the interaction height and energy by using information about the lateral spread of the cascade shower.
No associations
LandOfFree
New analysis of nuclear interaction observed by Mt. Kanbara emulsion chamber experiment does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with New analysis of nuclear interaction observed by Mt. Kanbara emulsion chamber experiment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New analysis of nuclear interaction observed by Mt. Kanbara emulsion chamber experiment will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-758644