Publications (3)0 Total impact
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J. Alvarez-Muñiz,
E. Amaral Soares,
A. Berlin,
M. Bogdan,
M. Boháčová,
C. Bonifazi,
W. R. Carvalho Jr,
J. R. T. de Mello Neto,
P. Facal San Luis,
J. F. Genat, [......],
M. Monasor,
P. Privitera,
A. Ramos de Castro,
L. C. Reyes,
B. Rouille d'Orfeuil,
E. M. Santos,
S. Wayne,
C. Williams,
E. Zas, J. Zhou
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ABSTRACT: We present the design, implementation and data taking performance of the
MIcrowave Detection of Air Showers (MIDAS) experiment, a large field of view
imaging telescope designed to detect microwave radiation from extensive air
showers induced by ultra-high energy cosmic rays. This novel technique may
bring a tenfold increase in detector duty cycle when compared to the standard
fluorescence technique based on detection of ultraviolet photons. The MIDAS
telescope consists of a 4.5 m diameter dish with a 53-pixel receiver camera,
instrumented with feed horns operating in the commercial extended C-Band (3.4
-- 4.2 GHz). A self-trigger capability is implemented in the digital
electronics. The main objectives of this first prototype of the MIDAS telescope
- to validate the telescope design, and to demonstrate a large detector duty
cycle - were successfully accomplished in a dedicated data taking run at the
University of Chicago campus prior to installation at the Pierre Auger
Observatory.
08/2012;
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J. Alvarez-Muñiz,
A. Berlin,
M. Bogdan,
M. Boháčová,
C. Bonifazi,
W. R. Carvalho Jr,
J. R. T. de Mello Neto,
P. Facal San Luis,
J. F. Genat,
N. Hollon,
E. Mills,
M. Monasor,
P. Privitera,
L. C. Reyes,
B. Rouille d'Orfeuil,
E. M. Santos,
S. Wayne,
C. Williams,
E. Zas, J. Zhou
[show abstract]
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ABSTRACT: We present a search for microwave emission from air showers induced by
ultrahigh energy cosmic rays with the microwave detection of air showers
experiment. No events were found, ruling out a wide range of power flux and
coherence of the putative emission, including those suggested by recent
laboratory measurements.
05/2012;
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M. Monasor,
M. Bohacova,
C. Bonifazi,
G. Cataldi,
S. Chemerisov,
J. R. T. de Mello Neto,
P. Facal San Luis,
B. Fox,
P. W. Gorham,
C. Hojvat, [......],
R. Meyhandan,
L. C. Reyes,
B. Rouille d'Orfeuil,
E. M. Santos,
J. Pochez,
P Privitera,
H. Spinka,
V Verzi,
C Williams, J Zhou
[show abstract]
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ABSTRACT: We present first measurements by MAYBE of microwave emission from an electron
beam induced air plasma, performed at the electron Van de Graaff facility of
the Argonne National Laboratory. Coherent radio Cherenkov, a major background
in a previous beam experiment, is not produced by the 3 MeV beam, which
simplifies the interpretation of the data. Radio emission is studied over a
wide range of frequencies between 3 and 12 GHz. This measurement provides
further insight on microwave emission from extensive air showers as a novel
detection technique for Ultra-High Energy Cosmic Rays.
08/2011;
Institutions
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2012
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University of Chicago
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Kavli Institute for Cosmological Physics
Chicago,
IL,
USA