A low-noise, high-dynamic-range, digital receiver for radio astronomy applications: An efficient solution for observing radio-bursts from Jupiter, the Sun, pulsars, and other astrophysical plasmas below 30 MHz

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Ryabov, V B ^a   Vavriv, D M ^b   Zarka, P ^c   Ryabov, B P ^b   Kozhin, R ^b   Vinogradov, V V ^b   Denis, L ^d  

^a FUTURE UNIVERSITY HAKODATE   (Japan)

^b INSTITUTE OF RADIO ASTRONOMY   (Ukraine)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d Station de Radioastronomie de Nancay   (France)

Author keywords

Instrumentation: miscellaneous; Instrumentation: spectrographs; Methods: observational; Planets and satellites: individual: Jupiter; Plasmas; Pulsars: general

Indexed keywords

INSTRUMENTATION: MISCELLANEOUS; INSTRUMENTATION: SPECTROGRAPHS; METHODS:OBSERVATIONAL; PLANETS AND SATELLITES: INDIVIDUAL: JUPITER; PULSARS: GENERAL;

ASTROPHYSICS; DIGITAL RADIO; INSTRUMENTS; PLANETS; RADAR ASTRONOMY; RADIO ASTRONOMY; SPECTROGRAPHS;

SATELLITES;

EID: 77149175099     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913335     Document Type: Article

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