PD
Pascal Démoulin
Observatoire de Paris, Université Paris Diderot
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Magnetic confinement fusion research
Employment
- 1989 - Present
Education
-
Université Paris Diderot PhD in Astrophysics1987 - 1989
Projects & Funding
Projects & funding information is unavailable.
Publications (323)
- Modeling the Effect of Mass-draining on Prominence Eruptions Save
- Generic Magnetic Field Intensity Profiles of Interplanetary Coronal Mass Ejections at Mercury, Venus, and Earth From Superposed Epoch Analyses Save
- Physical Processes Involved in the EUV "Surge" Event of 9 May 2012 Save
- Exploring the biases of a new method based on minimum variance for interplanetary magnetic clouds Save
- Sequential Eruptions Triggered by Flux Emergence: Observations and Modeling Save
- Study of Three-dimensional Magnetic Structure and the Successive Eruptive Nature of Active Region 12371 Save
- Coronal Elemental Abundances in Solar Emerging Flux Regions Save
- Studying the Transfer of Magnetic Helicity in Solar Active Regions with the Connectivity-based Helicity Flux Density Method Save
- Field distribution of magnetograms from simulations of active region formation Save
- Expanding and Contracting Coronal Loops as Evidence of Vortex Flows Induced by Solar Eruptions Save
- A study of the long term evolution in active region upflows Save
- Apparent and Intrinsic Evolution of Active Region Upflows Save
- Vortex and Sink Flows in Eruptive Flares as a Model for Coronal Implosions Save
- Successive injection of opposite magnetic helicity in solar active region NOAA 11928 Save
- Evolution of the magnetic field distribution of active regions Save
- Quantitative model for the generic 3D shape of ICMEs at 1 AU Save
- Properties of Magnetic Tongues over a Solar Cycle Save
- Superposed epoch study of ICME sub-structures near Earth and their effects on Galactic cosmic rays Save
- Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU Save
- Why Are Flare Ribbons Associated with the Spines of Magnetic Null Points Generically Elongated? Save