Phase calibration of the EISCAT Svalbard Radar interferometer using optical satellite signatures

Autor: E. M. Blixt, Betty Lanchester, T. Grydeland, Nickolay Ivchenko, J. Sullivan, Mike Lockwood
Přispěvatelé: School of Physics and Astronomy [Southampton], University of Southampton, Alfven Laboratory, Royal Institute of Technology [Stockholm] (KTH ), STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC), Dept. of Physics and Technology, EGU, Publication
Jazyk: angličtina
Rok vydání: 2006
Předmět:
Atmospheric Science
010504 meteorology & atmospheric sciences
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
ionosphere
01 natural sciences
law.invention
law
Radar imaging
0103 physical sciences
radio science
Earth and Planetary Sciences (miscellaneous)
Radar
lcsh:Science
010303 astronomy & astrophysics
0105 earth and related environmental sciences
Remote sensing
Radio Science
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere

Spectral signature
[SDU.OCEAN] Sciences of the Universe [physics]/Ocean
Atmosphere

instruments and techniques
lcsh:QC801-809
Geology
Astronomy and Astrophysics
interferometry
lcsh:QC1-999
Interferometry
lcsh:Geophysics. Cosmic physics
Space and Planetary Science
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434

VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
Temporal resolution
auroral ionosphere
[SDU.STU] Sciences of the Universe [physics]/Earth Sciences
Satellite
lcsh:Q
Antenna (radio)
lcsh:Physics
Zdroj: Annales Geophysicae, Vol 24, Pp 2419-2427 (2006)
Annales Geophysicae
Annales Geophysicae, European Geosciences Union, 2006, 24 (9), pp.2419-2427
Scopus-Elsevier
Annales Geophysicae, Vol 24, Iss 9, Pp 2419-2427 (2006)
ISSN: 1432-0576
0992-7689
Popis: The link between natural ion-line enhancements in radar spectra and auroral activity has been the subject of recent studies but conclusions have been limited by the spatial and temporal resolution previously available. The next challenge is to use shorter sub-second integration times in combination with interferometric programmes to resolve spatial structure within the main radar beam, and so relate enhanced filaments to individual auroral rays. This paper presents initial studies of a technique, using optical and spectral satellite signatures, to calibrate the received phase of a signal with the position of the scattering source along the interferometric baseline of the EISCAT Svalbard Radar. It is shown that a consistent relationship can be found only if the satellite passage through the phase fringes is adjusted from the passage predicted by optical tracking. This required adjustment is interpreted as being due to the vector between the theoretical focusing points of the two antennae, i.e. the true radar baseline, differing from the baseline obtained by survey between the antenna foot points. A method to obtain a measurement of the true interferometric baseline using multiple satellite passes is outlined.
Databáze: OpenAIRE