메뉴 건너뛰기




Volumn 85, Issue 6, 1997, Pages 917-924

A three-site comparison of fade-duration measurements

Author keywords

Attenuation measurements; Communication channels; Fading channels; Microwave propagation; Satellite communication

Indexed keywords

CODES (SYMBOLS); COMMUNICATION CHANNELS (INFORMATION THEORY); ELECTROMAGNETIC WAVE ATTENUATION; ELECTROMAGNETIC WAVE PROPAGATION; ERROR CORRECTION; FADING (RADIO); MODULATION; SATELLITE COMMUNICATION SYSTEMS;

EID: 0031166260     PISSN: 00189219     EISSN: None     Source Type: Journal    
DOI: 10.1109/5.598414     Document Type: Article
Times cited : (9)

References (10)
  • 2
    • 0019057127 scopus 로고
    • ETS-II experiments part IV: Characteristics of millimeter and centimeter wavelength propagation
    • Sept.
    • M. Fujita, T. Shinozuka, T. Ihara, Y. Furuhama, and H. Inuki, ETS-II experiments part IV: Characteristics of millimeter and centimeter wavelength propagation, IEEE Trans. Aerosp. Electron. Syst., vol. AES-16, pp. 581-589, Sept. 1980.
    • (1980) IEEE Trans. Aerosp. Electron. Syst. , vol.AES16 , pp. 581-589
    • Fujita, M.1    Shinozuka, T.2    Ihara, T.3    Furuhama, Y.4    Inuki, H.5
  • 3
    • 0020128118 scopus 로고
    • Results from the 19- And 28-GHz COMSTAR satellite propagation experiments at Crawford Hill
    • May
    • D. C. Cox and H. Arnold, Results from the 19- and 28-GHz COMSTAR satellite propagation experiments at Crawford Hill, Proc. IEEE. vol. 70, pp. 458-188, May 1982.
    • (1982) Proc. IEEE. , vol.70 , pp. 458-1188
    • Cox, D.C.1    Arnold, H.2
  • 4
    • 0019875099 scopus 로고
    • Duration of rain-induced fades of signal from SIRIO at 11.6 GHz
    • Jan.
    • E. Matricciani, Duration of rain-induced fades of signal from SIRIO at 11.6 GHz, Electron. Lett., vol. 17, no. 1, pp. 29-30, Jan. 1981.
    • (1981) Electron. Lett. , vol.17 , Issue.1 , pp. 29-30
    • Matricciani, E.1
  • 5
    • 0019871324 scopus 로고
    • Analysis of 11 GHz slant path fade duration and fade slope
    • Apr.
    • F. Dintelmann, Analysis of 11 GHz slant path fade duration and fade slope, Electron. Lett., vol. 17, no. 7, pp. 267-268, Apr. 1981.
    • (1981) Electron. Lett. , vol.17 , Issue.7 , pp. 267-268
    • Dintelmann, F.1
  • 7
    • 33646936014 scopus 로고
    • Attenuation scaling by frequency in the Ku/Ka-bands using the OLYMPUS satellite
    • Sept.
    • J. Laster and W. Stutzman, Attenuation scaling by frequency in the Ku/Ka-bands using the OLYMPUS satellite, Virginia Tech, Blacksburg, SATCOM Rep. 93-16, Sept. 1993.
    • (1993) Virginia Tech, Blacksburg, SATCOM Rep. , vol.93 , Issue.16
    • Laster, J.1    Stutzman, W.2
  • 8
    • 33646913549 scopus 로고
    • Fade and inter-fade durations in Ku and Ka-band frequencies measured from the OLYMPUS satellite beacons
    • Oct.
    • H. Ajaz and A. Safaai-Jazi, Fade and inter-fade durations in Ku and Ka-band frequencies measured from the OLYMPUS satellite beacons, Virginia Tech, Blacksburg, SATCOM Rep 93-17, Oct. 1993.
    • (1993) Virginia Tech, Blacksburg, SATCOM Rep , vol.93 , Issue.17
    • Ajaz, H.1    Safaai-Jazi, A.2
  • 9
    • 0028463384 scopus 로고
    • A new method for the prediction of fade duration statistics in the satellite links above 10 GHz
    • A. Paraboni and C. Riva, A new method for the prediction of fade duration statistics in the satellite links above 10 GHz, Int. J. Satell. Commun., vol. 12, pp. 387-394, 1994.
    • (1994) Int. J. Satell. Commun. , vol.12 , pp. 387-394
    • Paraboni, A.1    Riva, C.2
  • 10
    • 84977109035 scopus 로고    scopus 로고
    • First year propagation experiment results from the New Mexico ACTS receiver terminal at 20.185 and 27.505 GHz
    • Washington, D.C., Mar
    • J. Feil, L. J. Ippolito, Jr., M. Buehrer, G. Feldhake, and S. Horan, First year propagation experiment results from the New Mexico ACTS receiver terminal at 20.185 and 27.505 GHz, presented at the AIAA Satellite Conf., Washington, D.C., Mar 1996.
    • (1996) AIAA Satellite Conf.
    • Feil, J.1    Ippolito Jr., L.J.2    Buehrer, M.3    Feldhake, G.4    Horan, S.5


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.