Sokolsky, Pierre
Pierre Sokolsky American physicist
Sokolsky, Pierre 1946-
VIAF ID: 14831255 (Personal)
Permalink: http://viaf.org/viaf/14831255
Preferred Forms
- 100 0 _ ‡a Pierre Sokolsky ‡c American physicist
- 200 _ | ‡a Sokolsky ‡b Pierre
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- 100 1 _ ‡a Sokolsky, Pierre
- 100 1 _ ‡a Sokolsky, Pierre
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- 100 1 _ ‡a Sokolsky, Pierre
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- 100 1 _ ‡a Sokolsky, Pierre
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- 100 1 _ ‡a Sokolsky, Pierre ‡d 1946-
4xx's: Alternate Name Forms (13)
5xx's: Related Names (6)
- 510 2 _ ‡a Columbia University
- 510 2 _ ‡a University of Chicago
- 510 2 _ ‡a University of Chicago ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
- 510 2 _ ‡a University of Illinois at Urbana-Champaign
- 510 2 _ ‡a University of Illinois ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
- 510 2 _ ‡a University of Utah
Works
Title | Sources |
---|---|
Air Shower Detection by Bistatic Radar | |
An alternative method to finding patterns in HiRes stereo data | |
Anisotropy studies around the galactic centre at EeV energies with the Auger Observatory | |
The clock in the sun : how we came to understand our nearest star | |
Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei | |
The Cosmic Ray Energy Spectrum between 2 PeV and 2 EeV Observed with the TALE Detector in Monocular Mode | |
Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiation | |
Energy spectrum of TeV gamma rays from Mrk 501 obtained by stereoscopic analysis | |
EUSO-TA – First results from a ground-based EUSO telescope | |
Evidence for 1018-eV neutral particles from the direction of Cygnus X-3 | |
Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energies | |
First Observation of the Greisen-Zatsepin-Kuzmin Suppression | |
First upper limits on the radar cross section of cosmic-ray induced extensive air showers | |
Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation | |
Gamma Ray Showers Observed at Ground Level in Coincidence With Downward Lightning Leaders | |
The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array | |
Indications of proton-dominated cosmic-ray composition above 1.6 EeV | |
INTRODUCTION TO THE SALSA, A SALTDOME SHOWER ARRAY AS A GZK NEUTRINO OBSERVATORY | |
Introduction to ultrahigh energy cosmic ray physics | |
Large area networked detectors for particle astrophysics | |
Limits on deeply penetrating particles in the >10(17) eV cosmic-ray flux | |
A measurement of the average longitudinal development profile of cosmic ray air showers between 1017 and 1018 eV | |
Measurement of the Cosmic‐Ray Energy Spectrum and Composition from 1017to 1018.3eV Using a Hybrid Technique | |
A measurement of time-averaged aerosol optical depth using air-showers observed in stereo by HiRes | |
Monocular measurement of the spectrum of UHE cosmic rays by the FADC detector of the HiRes experiment | |
Past, present, and future of UHECR observations | |
The present status of the Telescope Array experiment | |
Search for Cross‐Correlations of Ultrahigh‐Energy Cosmic Rays with BL Lacertae Objects | |
Search for EeV protons of galactic origin | |
Search for gamma rays above 10 14 eV from Cygnus X-3 during the June and July 1989 radio outbursts | |
Search for point-like sources of cosmic rays with energies above 1018.5eV in the HiRes-I monocular data set | |
SEARCHES FOR LARGE-SCALE ANISOTROPY IN THE ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE ENERGY OF 10 19 eV AT THE PIERRE AUGER OBSERVATORY AND THE TELESCOPE ARRAY | |
Study of Small-Scale Anisotropy of Ultra-High-Energy Cosmic Rays Observed in Stereo by the High Resolution Fly's Eye Detector | |
TARA: Forward-scattered radar detection of UHECR at the telescope array | |
Testing a Reported Correlation between Arrival Directions of Ultra-high-energy Cosmic Rays and a Flux Pattern from nearby Starburst Galaxies using Telescope Array Data | |
Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory | |
Upper limit on the flux of photons with energies above1019 eVusing the Telescope Array surface detector |