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Electron density and temperature in the solar corona from multifrequency radio imaging

Astronomy and astrophysics (Berlin), 2015-11, Vol.583, p.A101

2015

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The structure of solar radio noise storms

Astronomy and astrophysics (Berlin), 2015-04, Vol.576, p.A136

2015

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Morphology of the quiet Sun between 150 and 450 MHz as observed with the Nançay radioheliograph

Astronomy and astrophysics (Berlin), 2012-04, Vol.540, p.A18

2012

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Sleeping arrangements and mass distribution of bed nets in six districts in central and northern Mozambique

Tropical medicine & international health, 2015-12, Vol.20 (12), p.1685-1695

2015

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Multiwavelength Analysis of the Impact Polarization of 2001 June 15 Solar Flare

The Astrophysical journal, 2005-09, Vol.631 (1), p.618-627

2005

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Electron density and temperature in the solar corona from multifrequency radio imaging (Corrigendum)

Astronomy and astrophysics (Berlin), 2016-01, Vol.585, p.C1

2016

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Morphology of the quiet Sun between 150 and 450 MHz as observed with the Nancay radioheliograph

Astronomy and astrophysics (Berlin), 2012-04, Vol.540, p.1-1

2012

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The Quiet Sun between 150 and 450 MHz : morphology and modeling

EAS publications series, 2012, Vol.55, p.213-221

2012

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First Results of Mg I (3p 1P1-4d 1D2) Line Linear Impact Polarization during the Solar Flare on 2001 June 15

The Astrophysical journal, 2006-10, Vol.650 (2), p.1193-1198

2006

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Information on particle acceleration and transport derived from solar flare spectropolarimetry

Advances in space research, 2005, Vol.35 (10), p.1841-1845

2005

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Impact line linear polarization as a diagnostic of 100 keV proton acceleration in solar flares

Astrophysical Journal, Supplement Series; (USA), 1990-06, Vol.73 (2), p.303-311

1990

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H α impact polarization observed in solar flares as a diagnostic of energy transport mechanisms

Journal of quantitative spectroscopy & radiative transfer, 1990-07, Vol.44 (1), p.193-201

1990

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First Results of Mg I (3p super(1)P sub(1)-4d super(1)D sub(2)) Line Linear Impact Polarization during the Solar Flare on 2001 June 15

The Astrophysical journal, 2006-10, Vol.650 (2), p.1193-1198

2006

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First results of Mg I (3p 1P1-4d 1D2) line linear impact polarization during the solar flare on 2001 june 15

The Astrophysical journal, 2006, Vol.650 (2), p.1193-1198

2006

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Coronal proton transport in the presence of Alfven waves and implications for impact line linear polarization

The Astrophysical journal, 1990-08, Vol.358 (2), p.674-679

1990

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Impact linear polarization observed in a UV chromospheric line during a solar flare

The Astrophysical journal, 1983-02, Vol.265, p.1066

1983

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Influence of helium and heavy elements on the radio absorption coefficient

Solar physics, 1971-03, Vol.17 (1), p.97-98

1971

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THEMIS as particle detector: Spectropolarimetry of solar flares

Il nuovo cimento della Società italiana di fisica. Sezione C, Geophysics and space physics, 2002, Vol.25

2002

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Conductive flux in the chromosphere derived from line linear polarization observation

Solar physics, 1983-07, Vol.86 (1-2), p.115-122

1983

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Histological responses of the endometrium to the IUD

Contraceptive delivery systems, 1981-04, Vol.2 (1), p.145

1981

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The emission of solar X-rays in the 0.5?3 wavelength range and its relation to the magnetic configuration of active centers

Solar physics, 1969-08, Vol.8 (2), p.369-375

Chambe, G.

1969

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X-rays spectroheliograms in lines of Mg xi and Mg xii

Solar physics, 1973-04, Vol.29 (2), p.341-355

1973

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Impact linear polarization observed in a UV chromospheric line during a solar flare

Advances in space research, 1982, Vol.2 (11), p.155-158

1982

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Histological response of the endometrium to IUD's (author's transl)

Contraception, fertilite, sexualite, 1980-12, Vol.8 (12), p.911

1980

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Evaluation of Convalescent Plasma for Ebola Virus Disease in Guinea

The New England journal of medicine, 2016-01, Vol.374 (1), p.33-42

2016

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Electron density and temperature in the solar corona from multifrequency radio imaging

The structure of solar radio noise storms

Morphology of the quiet Sun between 150 and 450 MHz as observed with the Nançay radioheliograph

Sleeping arrangements and mass distribution of bed nets in six districts in central and northern Mozambique

Multiwavelength Analysis of the Impact Polarization of 2001 June 15 Solar Flare

Electron density and temperature in the solar corona from multifrequency radio imaging (Corrigendum)

Morphology of the quiet Sun between 150 and 450 MHz as observed with the Nancay radioheliograph

The Quiet Sun between 150 and 450 MHz : morphology and modeling

First Results of Mg I (3p 1P1-4d 1D2) Line Linear Impact Polarization during the Solar Flare on 2001 June 15

Information on particle acceleration and transport derived from solar flare spectropolarimetry

Impact line linear polarization as a diagnostic of 100 keV proton acceleration in solar flares

H α impact polarization observed in solar flares as a diagnostic of energy transport mechanisms

First Results of Mg I (3p super(1)P sub(1)-4d super(1)D sub(2)) Line Linear Impact Polarization during the Solar Flare on 2001 June 15

First results of Mg I (3p 1P1-4d 1D2) line linear impact polarization during the solar flare on 2001 june 15

Coronal proton transport in the presence of Alfven waves and implications for impact line linear polarization

Impact linear polarization observed in a UV chromospheric line during a solar flare

Influence of helium and heavy elements on the radio absorption coefficient

THEMIS as particle detector: Spectropolarimetry of solar flares

Conductive flux in the chromosphere derived from line linear polarization observation

Histological responses of the endometrium to the IUD

The emission of solar X-rays in the 0.5?3 wavelength range and its relation to the magnetic configuration of active centers

X-rays spectroheliograms in lines of Mg xi and Mg xii

Impact linear polarization observed in a UV chromospheric line during a solar flare

Histological response of the endometrium to IUD's (author's transl)

Evaluation of Convalescent Plasma for Ebola Virus Disease in Guinea

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