Imperial College London

DrMarinaGaland

Faculty of Natural SciencesDepartment of Physics

Reader in Planetary Science
 
 
 
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Contact

 

m.galand Website

 
 
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Location

 

Huxley BuildingSouth Kensington Campus

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Summary

 

Publications

Publication Type
Year
to

121 results found

Nilsson H, Kirkwood S, Lilensten J, Galand Met al., 1997, Enhanced incoherent scatter plasma lines, Annales Geophysicae, Vol: 14, Pages: 1462-1472, ISSN: 0992-7689

Detailed model calculations of auroral secondary and photoelectron distributions for varying conditions have been used to calculate the theoretical enhancement of incoherent scatter plasma lines. These calculations are compared with EISCAT UHF radar measurements of enhanced plasma lines from both the E and F regions, and published EISCAT VHF radar measurements. The agreement between the calculated and observed plasma line enhancements is good. The enhancement from the superthermal distribution can explain even the very strong enhancements observed in the auroral E region during aurora, as previously shown by Kirkwood et al. The model calculations are used to predict the range of conditions when enhanced plasma lines will be seen with the existing high-latitude incoherent scatter radars, including the new EISCAT Svalbard radar. It is found that the detailed structure, i.e. the gradients in the suprathermal distribution, are most important for the plasma line enhancement. The level of superthermal flux affects the enhancement only in the region of low phase energy where the number of thermal electrons is comparable to the number of suprathermal electrons and in the region of high phase energy where the suprathermal fluxes fall to such low levels that their effect becomes small compared to the collision term. To facilitate the use of the predictions for the different radars, the expected signal-to-noise ratios (SNRs) for typical plasma line enhancements have been calculated. It is found that the high-frequency radars (Søndre Strømfjord, EISCAT UHF) should observe the highest SNR. but only for rather high plasma frequencies. The VHF radars (EISCAT VHF and Svalbard) will detect enhanced plasma lines over a wider range of frequencies, but with lower SNR.

Journal article

Carpenter DL, Galand M, Bell TF, Sonwalkar VS, Inan US, LaBelle J, Smith AJ, Clark TDG, Rosenberg TJet al., 1997, Quasiperiodic similar to 5-60 s fluctuations of VLF signals propagating in the Earth-ionosphere waveguide: A result of pulsating auroral particle precipitation?, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 347-361

Journal article

Nilsson H, Kirkwood S, Lilensten J, Galand Met al., 1996, Enhanced incoherent scatter plasma lines, ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 14, Pages: 1462-1472, ISSN: 0992-7689

Journal article

KIRKWOOD S, NILSSON H, LILENSTEN J, GALAND Met al., 1995, STRONGLY ENHANCED INCOHERENT-SCATTER PLASMA LINES IN AURORA, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 21343-21355, ISSN: 0148-0227

Journal article

Rodriguez S, Vinatier S, Cordier D, Carrasco N, Charnay B, Cornet T, Coustenis A, Kok RD, Freissinet C, Galand M, Geppert WD, Jauman R, Kalousova K, Koskinen TT, Lebonnois S, Gall AL, Mouélic SL, Lucas A, Mandt K, Mastrogiuseppe M, Nixon CA, Radebaugh J, Rannou P, Soderblom JM, Solomonidou A, Sotin C, Stephan K, Teanby N, Tobie G, Vuitton Vet al., Science goals and mission concepts for a future orbital and in situ exploration of Titan

In this white paper, we present a cross-section of important scientificquestions that remain partially or completely unanswered, ranging from Titanexosphere to the deep interior, and we detail which instrumentation and missionscenarios should be used to answer them. Our intention is to formulate thescience goals for the next generation of planetary missions to Titan in orderto prepare the future exploration of the moon. The ESA L-class mission conceptthat we propose is composed of a Titan orbiter and at least an in situ element(lake lander and/or drone(s)).

Working paper

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