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B. Mitrica

65 papers hereh-index 4711.9k citations285 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author18

Across the 19 of 65 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE37
  • astro-ph9
  • astro-ph.IM7
  • physics.ins-det7
  • hep-ph3
  • hep-ex1
same name
  • B. Mitrica — 25 papers
  • B. Mitrica — 1 paper
  • B. Mitrica — 1 paper
  • B. Mitrica — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20052018
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above 8×1018 eV

409 citations · 3.9k across the 62 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005★ 2 cited

Absolute calibration of the LOPES antenna system

S. Nehls, LOPES Collaboration

Radio emission in extensive air showers arises from an interaction with the geomagnetic field and is subject of theoretical studies. This radio emission has advantages for the dete…

astro-ph2005

Combined LOPES and KASCADE-Grande Data Analysis

A. Haungs, LOPES Collaboration

First analyses of coincident data of the LOPES (LOfar PrototypE Station) radio antennas with the particle air shower experiment KASCADE-Grande show basic correlations in the observ…

astro-ph2005★ 1 cited

Fluctuations in the EAS radio signal derived with improved Monte Carlo simulations based on CORSIKA

Tim Huege

Cosmic ray air showers are known to emit pulsed radio emission which can be understood as coherent geosynchrotron radiation arising from the deflection of electron-positron pairs i…

astro-ph2005★ 336 cited

Detection and imaging of atmospheric radio flashes from cosmic ray air showers

H. Falcke, W. D. Apel, A. F. Badea

The nature of ultrahigh-energy cosmic rays (UHECRs) at energies >10^20 eV remains a mystery. They are likely to be of extragalactic origin, but should be absorbed within ~50 Mpc th…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.