Radio recombination lines at decametre wavelengths

Astronomy and Astrophysics

Volumn 525, Issue 8, 2010, Pages

  Peters, W M ^a   Lazio, T J W ^a,b   Clarke, T E ^a   Erickson, W C ^c   Kassim, N E ^a  

^a NAVAL RESEARCH LABORATORY   (United States)

^b NASA AMES RESEARCH CENTER   (United States)

^c UNIVERSITY OF TASMANIA   (Australia)

Author keywords

instrumentation: interferometers; ISM: lines and bands; line: identification; radio lines: ISM

Indexed keywords

ANGULAR RESOLUTION; COSMOLOGY OBSERVATIONS; FILLING FACTOR; FREQUENCY TUNING RANGE; FREQUENCY-DEPENDENT; GALACTIC LATITUDE; INSTRUMENTATION: INTERFEROMETERS; INTERFEROMETRIC ARRAY; INTERSTELLAR MEDIUMS; ISM: LINES AND BANDS; LINE: IDENTIFICATION; LONG WAVELENGTH; LOW FREQUENCY ARRAYS; LOW-FREQUENCY COMPONENTS; OPTICAL DEPTH; OPTIMAL FREQUENCY; RADIO LINES: ISM; RADIO RECOMBINATION LINES; REIONIZATION; SPECTRAL FLUCTUATIONS;

HIGH FREQUENCY TELECOMMUNICATION LINES; INSTRUMENTS; INTERFEROMETERS; IONIZATION OF GASES; RADIO WAVES; SIGNAL PROCESSING;

SIGNAL DETECTION;

EID: 78649915775     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014707     Document Type: Article

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