You are not logged in to this journal. Log in    |   Subscription Information

Phys. Rev. Lett. 99, 171101 (2007) [5 pages]

Observations of the Askaryan Effect in Ice

P. W. Gorham,1 S. W. Barwick,2 J. J. Beatty,3 D. Z. Besson,4 W. R. Binns,5 C. Chen,6 P. Chen,6 J. M. Clem,7 A. Connolly,8 P. F. Dowkontt,5 M. A. DuVernois,9 R. C. Field,6 D. Goldstein,2 A. Goodhue,8 C. Hast,6 C. L. Hebert,1 S. Hoover,8 M. H. Israel,5 J. Kowalski,1 J. G. Learned,1 K. M. Liewer,10 J. T. Link,1,11 E. Lusczek,9 S. Matsuno,1 B. Mercurio,3 C. Miki,1 P. Miočinović,1 J. Nam,2 C. J. Naudet,10 J. Ng,6 R. Nichol,3 K. Palladino,3 K. Reil,6 A. Romero-Wolf,1 M. Rosen,1 L. Ruckman,1 D. Saltzberg,8 D. Seckel,7 G. S. Varner,1 D. Walz,6 and F. Wu2

(ANITA Collaboration)

1Department of Physics and Astronomy, University of Hawaii, Manoa, Hawaii 96822, USA
2University of California, Irvine California 92697, USA
3Department of Physics, Ohio State University, Columbus, Ohio 43210, USA
4Department of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045, USA
5Department of Physics, Washington University in St. Louis, Missouri 63130, USA
6Stanford Linear Accelerator Center, Menlo Park, California, 94025, USA
7University of Delaware, Newark, Delaware 19716, USA
8Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA
9School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
10Jet Propulsion Laboratory, Pasadena, California 91109, USA
11Currently at NASA Goddard Space Flight Center, Greenbelt, Maryland, 20771, USA

Received 13 December 2006; revised 15 June 2007; published 25 October 2007

We report on observations of coherent, impulsive radio Cherenkov radiation from electromagnetic showers in solid ice. This is the first observation of the Askaryan effect in ice. As part of the complete validation process for the ANITA experiment, we performed an experiment at the Stanford Linear Accelerator Center in June 2006 using a 7.5 metric ton ice target. We measure for the first time the large-scale angular dependence of the radiation pattern, a major factor in determining the solid-angle acceptance of ultrahigh-energy neutrino detectors.

©2007 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevLett.99.171101
DOI: 10.1103/PhysRevLett.99.171101
PACS: 95.55.Vj; 29.40.Ka; 98.70.Sa
  • 95.55.Vj
    Neutrino, muon, pion, and other elementary particle detectors; cosmic ray detectors
  • 29.40.Ka
    Cherenkov detectors
  • 98.70.Sa
    Cosmic rays including sources, origin, acceleration, and interactions
  • YEAR: 2007
KEYWORDS: Cherenkov radiation, cosmic ray interactions, ice, neutrino detection

REFERENCES (20)

For access to fully linked references, you need to log in. For access to fully linked references, you need to Log in.

CITING ARTICLES

For access to citing articles, you need to log in.
For access to citing articles, you need to Log in.



A new free weekly publication from APS

Physics - A new free weekly publication from APS
Please visit physics.aps.org
 
Article Tools