The California HIgh school Cosmic ray ObServatory (CHICOS) is a collaborative project involving Caltech, Cal State Northridge, UC Irvine, and local high schools to site a large array of particle detectors in Southern California. The detectors are located on school rooftops, and utilize the power and network infrastructure available at the schools. The main scientific goal is to study cosmic rays at ultra-high energies E > 10^(19) eV. We have fielded a total of 23 sites so far, and are beginning to collect data as we continue to deploy additional sites. We have observed our first evidence of extended air showers in coincidence with a local high school. The anticipated performance of the initial array and the potential for future expansion wi...
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic ...
Discovered by Hess during some experiments about air ionization, cosmic rays are constituted by part...
Despite large progresses in building new detectors and in the analysis techniques, the key questions...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a collaborative project involving Calt...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a collaborative project involving Calt...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a ground-based scintillator array desi...
CHICOS (California HIgh school Cosmic ray ObServatory) is presently an array of more than 140 detect...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a large area (presently 400 square kil...
Abstract: The Cosmic Ray Observatory Project (CROP) is a statewide education and research ex-perimen...
We present the results of a search for time correlations in high energy cosmic ray data (primary E >...
The Cosmic Ray Observatory Project (CROP) is a statewide education and research experiment involving...
I summarize in this paper the results and perspectives of representative ground experiments for the ...
The origin and nature of ultrahigh-energy cosmic rays (UHECRs) are one of the most intriguing myster...
The galactic cosmic–ray spectrum extends over 14 orders of magnitudes in energy and about 12 orders ...
These are some summary remarks given at the Chacaltaya meeting on cosmic ray physics, held in La Paz...
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic ...
Discovered by Hess during some experiments about air ionization, cosmic rays are constituted by part...
Despite large progresses in building new detectors and in the analysis techniques, the key questions...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a collaborative project involving Calt...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a collaborative project involving Calt...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a ground-based scintillator array desi...
CHICOS (California HIgh school Cosmic ray ObServatory) is presently an array of more than 140 detect...
The California HIgh school Cosmic ray ObServatory (CHICOS) is a large area (presently 400 square kil...
Abstract: The Cosmic Ray Observatory Project (CROP) is a statewide education and research ex-perimen...
We present the results of a search for time correlations in high energy cosmic ray data (primary E >...
The Cosmic Ray Observatory Project (CROP) is a statewide education and research experiment involving...
I summarize in this paper the results and perspectives of representative ground experiments for the ...
The origin and nature of ultrahigh-energy cosmic rays (UHECRs) are one of the most intriguing myster...
The galactic cosmic–ray spectrum extends over 14 orders of magnitudes in energy and about 12 orders ...
These are some summary remarks given at the Chacaltaya meeting on cosmic ray physics, held in La Paz...
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic ...
Discovered by Hess during some experiments about air ionization, cosmic rays are constituted by part...
Despite large progresses in building new detectors and in the analysis techniques, the key questions...