Ducted whistlers propagating in higher‐order guided mode and recorded on board of Compass‐2 satellite by the advanced Signal Analyzer and Sampler 2

Ferencz, Orsolya E.; Bodnár, László; Ferencz, Csaba; Hamar, D.; Lichtenberger, János; Steinbach, Péter; Korepanov, V. E.; Mikhaylova, G. A.; Mikhaylov, Yuri; Кузнецов, В. Д.

doi:10.1029/2008ja013542

Cited by 11 publications

(5 citation statements)

References 13 publications

(14 reference statements)

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“…A továbbfejlesztett SAS-2-K2-es 2006-ban a Kompasz-2 orosz-magyar-ukrán műhold fedélzetén repült, és a magyar mérésekkel sikerült először igazolni az ún. vezetett terjedést whistlerek esetében műholdas adatokból (Ferencz et al 2009). 2012-ben sikerrel állt pályára a Csibisz-M orosz-magyar-ukrán műhold a Progressz teherűrhajó segítségével, fedélzetén a SAS-3-Ch műszerrel.…”

Section: Magyar Hullámmérések Műholdakonunclassified

Trabanttal a föld körül

Ferencz¹,

Steinbach²,

Lichtenberger³

et al. 2019

Haditechnika

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Section: Magyar Hullámmérések Műholdakonunclassified

Trabanttal a föld körül

Ferencz¹,

Steinbach²,

Lichtenberger³

et al. 2019

Haditechnika

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“…The core instrument of the EVE EM suite is a combined electromagnetic wave analyser and permittivity sensor. The electromagnetic wave analyser is based on a Hungarian instrument with extensive flight heritage on Compass-2, Chibis and Relec satellites and the ISS [14]. This instrument measures the horizontal electric field from 0-20 kHz by measuring the potential between two electrodes deployed on 1 m booms on opposite sides of the gondola.…”

Section: Baseline Payloadmentioning

confidence: 99%

The 2010 European Venus Explorer (EVE) mission proposal

Wilson¹,

Chassefière²,

Hinglais³

et al. 2011

Exp Astron

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International audienceThe European Venus Explorer (EVE) mission described in this paper was proposed in December 2010 to ESA as an 'M-class' mission under the Cosmic Vision programme. It consists of a single balloon platform floating in the middle of the main convective cloud layer of Venus at an altitude of 55 km, where temperatures and pressures are benign (∼25°C and ∼0.5 bar). The balloon float lifetime would be at least 10 Earth days, long enough to guarantee at least one full circumnavigation of the planet. This offers an ideal platform for the two main science goals of the mission: study of the current climate through detailed characterization of cloud-level atmosphere, and investigation of the formation and evolution of Venus, through careful measurement of noble gas isotopic abundances. These investigations would provide key data for comparative planetology of terrestrial planets in our solar system and beyond

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“…In the last years, however, with the exclusion of the motion of the medium traversed by the propagating signals, it was possible to derive precise full‐wave solutions of monochromatic and UWB signals from the Maxwell's equations [ Ferencz et al , 1996, 2001; Ferencz , 2005] with a lot of successful applications of these theoretical results mainly in space research [e.g., Ferencz et al , 2001, 2007; Lichtenberger , 2009; Ferencz et al , 2009]. The key step to derive these new solutions was the correct application of the method of inhomogeneous basic modes (MIBM) (see details given by Ferencz [1978c], Ferencz et al [2001], Ferencz [2004], and Ferencz [2005]).…”

Section: Introductionmentioning

confidence: 99%

Electromagnetic wave propagation in inhomogeneous, moving media: A general solution of the problem

Ferencz

2011

Radio Science

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[1] The exact computation, the exact modeling of the propagation of electromagnetic signals through inhomogeneous moving media, is an old theoretical and measuring/data interpretation problem, because in a lot of practical problems, such as the accurate space-time determination in satellite positioning systems, the occultation measurements, or the accurate tracking of the interplanetary probes, the electromagnetic wave (signal) traverses moving, inhomogeneous media, where the moving velocity of the media and the media itself are inhomogeneous in space, i.e., the Earth's high and low atmosphere, the planetary atmospheres, the interplanetary matter in the inner and outer solar system, etc. In other important cases of electromagnetic wave propagation, as the propagation in inhomogeneous media or the propagation of short impulses (ultrawide-band (UWB) signals), the application of the method of inhomogeneous basic modes (MIBM) was successful. In this paper it is demonstrated that the application of MIBM in the case of inhomogeneous moving media produces an exact, full-wave solution of monochromatic or UWB signals propagating through these media. The solutions are valid inside the special relativity.

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Ducted whistlers propagating in higher‐order guided mode and recorded on board of Compass‐2 satellite by the advanced Signal Analyzer and Sampler 2

Cited by 11 publications

References 13 publications

Trabanttal a föld körül

Trabanttal a föld körül

The 2010 European Venus Explorer (EVE) mission proposal

Electromagnetic wave propagation in inhomogeneous, moving media: A general solution of the problem

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