Nour E. Raouafi
0000-0003-2409-3742
Johns Hopkins University Applied Physics Laboratory
117 papers found
Refreshing results…
Far‐Ultraviolet Spectra of Fast Coronal Mass Ejections Associated with X‐Class Flares
Infrared Polarimetry at the MPAe: The Solar Atmosphere from the Photosphere to the Upper Chromosphere
Does the ion cyclotron exist in the inner corona?
Molecular lines observations with THEMIS
Linear polarization of the O VI lambda 1031.92 coronal line. II. Constraints on the magnetic field and the solar wind velocity field vectors in the coronal polar holes
Erratum: Stokes parameters of resonance lines scattered by a moving, magnetic medium. Theory of the two-level atom
Stokes parameters of resonance lines scattered by a moving, magnetic medium
Linear polarization of the O VI lambda 1031.92 coronal line. I. Constraints on the solar wind velocity field vector in the polar holes
Effect of the solar wind velocity field vector on the polarization of the O VI \ensuremathλ1032 coronal line
Effect of the coronal magnetic field and the solar wind velocity field vectors on the polarization of the O VI \ensuremathλ1032 line
Stokes parameters of resonance lines scattered by a moving, magnetic medium. Theory of the two-level atom
Properties and Modeling of a CME-driven Shock out of the Plane of the sky Through UVCS/SoHO Observations
Dissertation Abstract
On VI 1031.95 ̊A Line Polarization Measurements in View of Velocity Field and Magnetic Field Diagnostics in the Inner Solar Corona: Effect of the Polar Hole
On VI 103.2 A Line Polarization Measurements In View Of Velocity Field And Magnetic Field Diagnostics In The Inner Solar Corona
Detection of the O VI 103.2 NM line polarization by the SUMER spectrometer on the SOHO spacecraft
Doppler Redistribution of Resonance Polarization of the O VI 103.2 NM Line Observed Above a Polar Hole
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