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تسجيل مستخدم جديدA model-independent technique to determine one-dimensional radio source structure from interplanetary scintillation (IPS) observations
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V R Venugopal
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We outline a method of deriving one-dimensional phaseless visibility along solar wind direction from interplanetary scintillation power spectrum, together with the known visibility of a calibration source. The method is illustrated briefly. Details may be found in Edwin Jayaraj (1990).
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Aims. The phase scintillation of the European Space Agencys (ESA) Venus Express (VEX) spacecraft telemetry signal was observed at X-band (lambda = 3.6 cm) with a number of radio telescopes of the European VLBI Network (EVN) in the period 2009-2013. M
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