The least mean squares adaptive FIR filter for narrow-band RFI suppression in radio detection of cosmic rays

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00550909" target="_blank" >RIV/68378271:_____/17:00550909 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1109/TNS.2017.2703617" target="_blank" >https://doi.org/10.1109/TNS.2017.2703617</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1109/TNS.2017.2703617" target="_blank" >10.1109/TNS.2017.2703617</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The least mean squares adaptive FIR filter for narrow-band RFI suppression in radio detection of cosmic rays

Popis výsledku v původním jazyce

Radio emission from the extensive air showers (EASs), initiated by ultrahigh-energy cosmic rays, was theoretically suggested over 50 years ago. However, due to technical limitations, successful collection of sufficient statistics can take several years. Nowadays, this detection technique is used in many experiments consisting in studying EAS. One of them is the Auger Engineering Radio Array (AERA), located within the Pierre Auger Observatory. AERA focuses on the radio emission, generated by the electromagnetic part of the shower, mainly in geomagnetic and charge excess processes. The frequency band observed by AERA radio stations is 30-80 MHz. Thus, the frequency range is contaminated by human-made and narrow-band radio frequency interferences (RFIs). Suppression of contaminations is very important to lower the rate of spurious triggers.

Název v anglickém jazyce

The least mean squares adaptive FIR filter for narrow-band RFI suppression in radio detection of cosmic rays

Popis výsledku anglicky

Radio emission from the extensive air showers (EASs), initiated by ultrahigh-energy cosmic rays, was theoretically suggested over 50 years ago. However, due to technical limitations, successful collection of sufficient statistics can take several years. Nowadays, this detection technique is used in many experiments consisting in studying EAS. One of them is the Auger Engineering Radio Array (AERA), located within the Pierre Auger Observatory. AERA focuses on the radio emission, generated by the electromagnetic part of the shower, mainly in geomagnetic and charge excess processes. The frequency band observed by AERA radio stations is 30-80 MHz. Thus, the frequency range is contaminated by human-made and narrow-band radio frequency interferences (RFIs). Suppression of contaminations is very important to lower the rate of spurious triggers.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2017

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

IEEE Transactions on Nuclear Science

ISSN

0018-9499

e-ISSN

1558-1578

Svazek periodika

64

Číslo periodika v rámci svazku

6

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

12

Strana od-do

1304-1315

Kód UT WoS článku

000404973000017

EID výsledku v databázi Scopus

2-s2.0-85022190690