About: 4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges

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Attributs	Valeurs
type	work Issue
Is Part Of	http://hub.abes.fr/edp/periodical/eas/2012/volume_55
Title	4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
has manifestation of work	http://hub.abes.fr/edp/periodical/eas/2012/volume_55/issue_2012/m/print http://hub.abes.fr/edp/periodical/eas/2012/volume_55/issue_2012/m/web
publisher identifier	eas/2012/03
is Is Part Of of	Numerical modeling of the linear polarization in molecular lines of the solar flash spectrum Temporal properties of decimetric spikes in solar flares Sun’s small-scale magnetic field : from quiet region to polar region Property of emerging flux regions and corresponding response of the upper atmosphere Evolution of coronal hole boundaries observed by SDO Magnetic field distribution in the quiet and active photosphere Rotating Sunspots and Solar Eruptions Electric current density and related sigmoid in an active region The source regions of the solar wind revealed by UV/EUV spectroscopic observations On the Frequency Distributions of Solar Soft X-ray Flares Microwave burst with fine spectral structures in a solar flare on 2011 August 9 Extinction and Sky Brightness at Dome C MISOLFA : a seeing monitor for daytime turbulence parameters measurement Inversion of Zeeman Line Profiles Using Central Moments Chromospheric Evaporation in Solar Flares CME Trigger and Initiation A small-scale extreme ultraviolet wave observed by SDO Jacquinot shaped aperture for high contrast imaging of the solar corona New Technology Solar Coronagraphs Solar limb darkening function and solar diameter with eclipse observations Foreword Automated detection of filaments from He II images Kinematics and Differential Emission Measure of the Flux Rope during Coronal Mass Ejections Magnetic Reconnection in a Canopy-type Magnetic Configuration for Solar Microflares The Quiet Sun between 150 and 450 MHz : morphology and modeling Homologous flares inducing EUV filament oscillations with subsequent eruption ONSET-A New Multi-Wavelength Solar Telescope New generation Multichannel Subtractive Double Pass for imaging spectropolarimetry - The S4I prototype Height of the granulation contrast inversion layer derived from a cross-correlation method Physical properties of Moving Magnetic Features observed around a pore Heat Transport Problem in Solar Flares Three-dimensional Radiative Transfer applied to the Diagnostics of Magnetic Fields Forward-scattering Hanle effect in the solar Ca i 4227 Å line Helicity of Solar Active Regions with Solar Cycles Resistive magnetic flux emergence and formation of solar active regions Quasi-static evolution of the reconstructed magnetic field of an emerging and eruptive active region New perspectives on solar prominences Prominence-cavity regions observed in 2010 eclipse flash spectra and SWAP images Observation of magnetic reconnection at the turbulent leading edge of an interplanetary coronal mass ejection Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements Solar diameter with 2012 Venus Transit MHD simulations of the solar photosphere solar spicules and jets Vector magnetic field measurement and helicity of active regions A fast method for constructing magnetic field models of solar active regions Chromospheric magnetic fields of an active region filament Prominence seismology using ground- and space-based observations 3D Kinematic Evolution of Erupting Filaments Coronal jets in an inclined coronal magnetic field : a parametric 3D MHD study Tomographic reconstruction of polar plumes Plasmoid Ejection at a Solar Total Eclipse The contraction of flare loops and its impact on the solar lower atmosphere About the magnetic origin of Chromospheric Spicules and Coronal Jets CME development in the corona and interplanetary medium : A multi-wavelength approach A Converging View on EIT Waves The Sun-Earth Connection of Energetic Particles Current Status and Future Programs for the Measurement of Solar Magnetic Field in China ESCAPE : a first step to high resolution solar coronagraphy in Antarctica

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