[PDF] Top 20 Radio detection of cosmic rays with the Auger Engineering Radio Array
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Radio detection of cosmic rays with the Auger Engineering Radio Array
... graded array, with grid constants of 144, 250, 375 and 750 meters, prob- ing di ff erent energy and zenith angle ...on radio signals and one of them, in addition, allowing data bu ff ering for up to 8 ... See full document
5
Status and perspectives of the radio detection of highenergy cosmic rays
... At present also the calibration procedure for LOFAR is being improved [30], further reducing the systematic uncertainties with respect to previous work [18]. Radio emission from the Galactic center is used as a ... See full document
7
Radio detection of extensive air showers - Measurements of the properties of cosmic rays with the radio technique — past, present, future
... the radio signal distribution and will be addressed in this ...tial radio signal distribution is introduced based on morpholog- ical arguments, which gives an adequate description of the data measured by ... See full document
7
Ultimate precision in cosmic-ray radio detection — the SKA
... Kilometre Array will go online in ...low-frequency radio- astronomical observatory to date, and will facilitate a rich science programme in astron- omy and ...modest engineering changes, it will also ... See full document
6
Results and Perspectives of the Auger Engineering Radio Array
... The Auger Engineering Radio Array is the world’s largest radio detector for high-energy cosmic rays consisting of 153 autonomously-operating radio stations covering ... See full document
5
Precision measurements of cosmic rays up to the highest energies with a large radio array at the Pierre Auger Observatory
... of radio detection of cosmic rays be- gan in the early 2000s ...the radio emission ...the radio signals. The measurement of the radio foot- print of an air shower yields a ... See full document
9
INFN - LNS
... Radio detection of ultra high energy cosmic rays with the Auger Engineering Radio Array. 10:00 - 10:30 Abigail Vieregg[r] ... See full document
9
A next-generation ground array for the detection of ultrahigh-energy cosmic rays: the Fluorescence detector Array of Single-pixel Telescopes (FAST)
... of 43 ◦ with a 3.4σ significance [12]. In addition, ar- rival directions of UHECRs are found to correlate with nearby extragalactic objects at a modest 2 ∼ 3σ signif- icance level [23, 24]. There seems to be no measured ... See full document
6
Exploring cosmic rays at the highest-energy frontier with the Pierre Auger Observatory
... Pierre Auger Observatory faces the challenge of studying the origin and the nature of cosmic rays of ultrahigh ...largest cosmic-ray observatory ever built, it covers an area of 3000 km 2 in ... See full document
10
Development of the radio astronomical method of cosmic particle detection for extremely high-energy cosmic ray physics and neutrino astronomy
... large radio telescopes of Australia, USA, Russia and other countries but these experiments only put upper limits to the EHE cosmic rays ...nanosecond radio pulses from the Moon in a wider ... See full document
6
A multi-frequency analysis of radio supernova remnants and their environments in Sculptor Group SD Galaxy NGC 300 and the Small Magellanic Cloud
... of radio SNRs and their local envirnments in the direc- tion of NGC 300 and the Small Magellanic Cloud ...Compact Array (ATCA) and Very Long Array observations, 18 radio SNRs (with 3 ... See full document
18
Measurement of Ultra High Energy Cosmic Rays with CHICOS
... These two unexpected results from AGASA, if confirmed, would have important implications for both astronomy and physics and have fueled continued research of ultra-high energy cosmic rays. A nondetection of ... See full document
178
General overview of recent results from the Pierre Auger Observatory
... If the flux indeed shows a GZK feature at higher energies this implies that the sources of UHECRs must be within our cos- mological neighbourhood at distances smaller than 100 Mpc. Might this proximity open a window on ... See full document
7
Effect of Wildfire-induced Thermal Bubble on Radio Communication
... global warming; and fine particulate matter less than 2.5 µm (PM2.5) cause tract and lung infections such as acute respiratory infection [12]. During a wildfire, a large amount of heat energy is released into the ... See full document
32
Pulsar searches: from radio to gamma rays
... Abstract We report the results of four di erent pulsar searches, covering radio, X-ray, and gamma-ray wavelengths.. These searches targeted pulsars in virtually all of their guises: youn[r] ... See full document
159
Estimation of Best Spectrum Sensing Concept in Cognitive Radio Networks
... energy detection In this technique as shown in ...Energy detection spectrum sensing is otherwise known as Blind Signal detector, on the grounds that it disregards the structure of the ... See full document
5
Preliminary results of the AMIGA engineering array at the Pierre Auger Observatory
... The electronics readout works simultaneously as a counter (counts number of arriving muons) and as an in- tegrator (integrates the total signal of the arriving muons). The counter mode consists of 64 channels (one for ... See full document
6
Observation of ultra-high energy cosmic rays with the Telescope Array experiment
... TA utilizes deferent analysis techniques using three independent FD stations and the SD array. The hybrid analysis uses the FD and SD data to constrain the geometry of air showers. In the analysis, one combines ... See full document
9
Cosmic ray acceleration to ultrahigh energy in radio galaxies
... One of the best candidate UHECR acceleration mecha- nisms is di ff usive shock acceleration [DSA; 7–10], since it produces a well-defined spectral index in the particle mo- mentum distribution and the acceleration ... See full document
6
Research on stealth aircraft and its effect on radar system in modern warfare
... engineering and signal processing field made it possible for stealth technology realization in aircraft to deceive the enemy radar system effectively. However we are able to reduce visibility to certain limit due ... See full document
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