The Soudan 2 detector is located at a depth of 2090 meters-water equivalent (mwe). About 2 million muon events have been recorded. Here we report on our plans to analyze them for comparison with expectations from atmospheric cosmic ray models. Plans and capabilities to analyze multiple muons and monopoles are also discussed. 3 refs., 5 figs
© 2017 American Association of Physics Teachers. Cosmic ray muons are produced when high energy part...
A simple model is developed which predicts the average number of multi-TeV muons produced in cosmic ...
Cosmic muons are produced through interactions of primary cosmic radiation in the atmosphere. They a...
Multiple high energy muons, when studied with a large area detector, can be useful in the study of t...
Progress in the construction of the Soudan 2 nucleon decay detector which is being built at the Soud...
The Soudan 2 nucleon decay detector has recorded data since Summer 1988 using a quarter (dimensions ...
Abstract A small array of charged particle detectors above ground was run in coincidence with the So...
We describe the construction and operation of a wide angle atmospheric Cherenkov light detector. Thi...
A 37 m{sup 2} surface array which has been operating in coincidence with the Soudan 1 underground ex...
The Soudan 2 experiment has performed time-coincident cosmic ray air shower and underground muon mea...
During the period July 1987 through March 1988, a section of the Soudan 2 active shield known as the...
Typescript (photocopy).An investigation of scintillations in ground-level cosmic ray muons has been ...
A search for contained events in the Soudan 2 nucleon decay detector has been made for the initial e...
A sample of 16 million underground muons has been collected between January, 1989, and June, 1993, a...
Deep underground muon events recorded by the Soudan 2 detector, located at a depth of 2100 m of wate...
© 2017 American Association of Physics Teachers. Cosmic ray muons are produced when high energy part...
A simple model is developed which predicts the average number of multi-TeV muons produced in cosmic ...
Cosmic muons are produced through interactions of primary cosmic radiation in the atmosphere. They a...
Multiple high energy muons, when studied with a large area detector, can be useful in the study of t...
Progress in the construction of the Soudan 2 nucleon decay detector which is being built at the Soud...
The Soudan 2 nucleon decay detector has recorded data since Summer 1988 using a quarter (dimensions ...
Abstract A small array of charged particle detectors above ground was run in coincidence with the So...
We describe the construction and operation of a wide angle atmospheric Cherenkov light detector. Thi...
A 37 m{sup 2} surface array which has been operating in coincidence with the Soudan 1 underground ex...
The Soudan 2 experiment has performed time-coincident cosmic ray air shower and underground muon mea...
During the period July 1987 through March 1988, a section of the Soudan 2 active shield known as the...
Typescript (photocopy).An investigation of scintillations in ground-level cosmic ray muons has been ...
A search for contained events in the Soudan 2 nucleon decay detector has been made for the initial e...
A sample of 16 million underground muons has been collected between January, 1989, and June, 1993, a...
Deep underground muon events recorded by the Soudan 2 detector, located at a depth of 2100 m of wate...
© 2017 American Association of Physics Teachers. Cosmic ray muons are produced when high energy part...
A simple model is developed which predicts the average number of multi-TeV muons produced in cosmic ...
Cosmic muons are produced through interactions of primary cosmic radiation in the atmosphere. They a...