HelioWebN. E. Raouafi
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A[N. E. Raouafi]
AC["Associated Concepts (22)"]
AW["Authored Works (66)"]
CA["Linked Co-Authors (74)"]
CI["Linked Collaborating Institutions (85)"]
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AW== author ==>CA
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click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0003-2409-3742
- OpenAlex ID
- https://openalex.org/A5006894879 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Magnetic field
- Nuclear physics
- Plasma
- Solar wind
- Astronomy
- Astrophysics
- Biology
- Coronal mass ejection
- Astrobiology
- Geology
- Engineering
- Geography
- Venus
- Corona (planetary geology)
- Optics
- Meteorology
- Aerospace engineering
- Coronal hole
- Chemistry
- Computational physics
Authored Works
sorted by decreasing year, and then by display-name
- The Firefly Constellation: Exploring the Heliosphere from the Solar Interior to the Solar Wind
- Switchbacks, microstreams and broadband turbulence in the solar wind
- Statistical properties of the switchbacks observed during the first 11 encounters of the Parker Solar Probe
- Solar Wind Protons and Alphas Properties inside the Sub-Alfvenic Regions
- Solar Polar - The Why, When, and How
- Reconstructing the spatial field-perpendicular energy spectrum of magnetic fluctuations near and below the Alfven critical point
- Parker Solar Probe: Mission Status, Discoveries, and Outlook
- Parker Solar Probe Science Planning and Data Volume Optimization
- Magnetic Field Reconnection as the Source of the Solar wind
- Interchange reconnection within coronal holes powers the fast solarwind: Suprathermal ion flows and bursty magnetic fields modulated by the network magnetic field.
- Interchange Reconnection within Coronal Holes Powers the Fast Solar Wind: Connecting Parker Solar Probe Observations and Simulations to Coronal Reconnection Dynamics
- Heliospheric System Observatory Conjunctions and Data Return for Parker Solar Probe Encounter Periods
- Turbulence Characteristics of Switchback and Nonswitchback Intervals Observed by Parker Solar Probe
- To Touch the Sun: Parker Solar Probe and the Alfven Critical Point
- The COronal Magnetism Observatory (COMO)
- Structure and dynamics of flux ropes in the solar wind with implications for switchbacks
- Small-Scale Solar Activity and its effect on the coronal environment
- Proton-Alpha Differential Flow of the Young Solar Wind: Parker Solar Probe Observations
- Parker Solar Probe: Status and Outlook Halfway Through the Prime Mission
- Parker Solar Probe observations Venusian foreshocks, shocks and particle acceleration
- On the validity of the Taylor Hypothesis in the inner heliosphere as observed by the Parker Solar Probe
- Non Detection of Lightning During the Second Parker Solar Probe Venus Gravity Assist
- New insight into the nature and origin of switchbacks thanks to a comprehensive catalogue of events
- Direct Evidence for the Dynamic Chromospheric Origin of Solar Coronal Plumes
- Can solar coronal plumelets precondition switchback events in the wind?
- Applicability of Taylor's Hypothesis during Parker Solar Probe perihelia
- A solar source of Alfvenic magnetic field switchbacks: in situ remnants of magnetic funnels on supergranulation scales
- Plumelets: Dynamic Filamentary Structures in Solar Plumes
- Parker Solar Probe: Mission Status and Outlook After two Year of Operation
- Parker Solar Probe observations of the first three Venus flybys: foreshocks, shocks and particle acceleration
- Parker Solar Probe In-Situ Observations of Magnetic Reconnection in the Near-Sun Solar Wind
- New Insights into the Dynamic Relationship between Jetlets and Plumes
- Dynamics and Flows in Active Region NOAA12737 that can contribute to Type III Bursts observed by Parker Solar Probe during Encounter 2.
- Corotating Interaction Regions observed between Solar Orbiter and Parker Solar Probe
- Young Solar Wind in the Grip of the Sun's Corona
- Waiting time (distance) distributions of magnetic field and velocity PVI events during the first Parker Solar Probe encounter
- The magnetic structure and electrodynamics of the emerging solar wind
- The Forming Slow Solar Wind Imaged along Streamer Rays by the Wide-Angle Imager on Parker Solar Probe
- Statistics of Energetic Particles in the first Parker Solar Probe Orbit: Correlations and Association with Magnetic Structures
- Solar wind streams and corotating interaction regions observed by Parker Solar Probe with corresponding observations at one AU
- Parker Solar Probe: Mission Status and Outlook After One Year of Operation
- Parker Solar Probe observations of the first Venus flyby
- Parker Solar Probe Observations of the Release of Density Blobs and Flux Ropes at the Heliospheric Current Sheet
- Multi-species modelling of the forming solar wind from the upper chromosphere to Parker Solar Probe
- MHD-Scale Energy Transfer in the Inner Heliosphere from PSP observations
- Intermittent heating in the inner Heliosphere: PSP observations
- Impacts of small coronal transients at Parker Solar Probe at times of density increases and burst of magnetic switchbacks
- Imaging the Solar Corona from Within: First Results from the Parker Solar Probe Telescope
- Analysis of the Internal Structure of the Streamer Blow Out Observed the Parker Solar Probe during the First Solar Encounter
- Alfvenicity in PSP observations: comparing different measures
- Augmented Visual Experience of Simulated Solar Phenomena
- The Connection Between the Longitudinal Extent of SEP Events and the Properties of Coronal Shocks
- Dynamics of HVECs emitted from comet C/2011 L4 as observed by STEREO
- Connectivity Between Solar Energetic Particle Observations and Their Solar Sources: The Event on 14 August 2010
- Longitudinal Properties of a Widespread Solar Energetic Particle Event on 2014 February 25: Evolution of the Parent CME and Associated Shock
- Dynamics of High-Velocity Evanescent Clumps (HVECs) Emitted from Comet C/2011 L4 (Pan-STARRS) as Observed by STEREO
- Time-Dependent Coupling of Lfm-Helio and MAS Models for CME Propagation
- The Solar Energetic Particle Event on 2013 April 11: An Investigation of the Solar Origin of its Longitudinal Widespread
- The CME event on 07 January 2014: Why was it a geomagnetic dud?
- Coronal Magnetism: Hanle Effect in UV and IR Spectral Lines
- Plasma Disturbances in the Solar Polar Regions
- Magnetic Energy and Helicity Properties of Eruptive Solar Active Regions
- Plasma Outflows Within Polar Coronal Plumes
- Modeling the Solar Dust Environment at 9.5 Solar Radii: Revealing Radiance Trends with MESSENGER Star Tracker Data
- Polar Magnetic Field Distribution as Observed by SOLIS and its relation with coronal structures
- Properties and Modeling of a CME-driven Shock out of the Plane of the sky Through UVCS/SoHO Observations
Linked Co-Authors
- A. V. Usmanov
- A. Vourlidas
- A. W. Case
- Alexandros Chasapis
- Ali Rahmati
- Bennett A. Maruca
- C. Froment
- C. J. Owen
- C. M. S. Cohen
- Chuanfei Dong
- D. J. McComas
- D. Malaspina
- D. Ruffolo
- Daniel B. Seaton
- Donald M. Hassler
- Emily Lichko
- F. S. Mozer
- G. C. Ho
- G. M. Mason
- G. P. Zank
- J. C. Kasper
- J. F. Drake
- J. G. Luhmann
- J. Gruesbeck
- J. L. Verniero
- J. S. Halekas
- J. T. Hoeksema
- J. T. Steinberg
- J. W. Bonnell
- Jean C. Perez
- Jeffrey Newmark
- Jia Huang
- K. E. Korreck
- K. G. Klein
- K. Goetz
- Krzysztof Barczynski
- L. D. Woodham
- L. Golub
- L. P. Chitta
- Lisa Upton
- M. I. Desai
- M. L. Goldstein
- M. Martinović
- M. Moncuquet
- M. Pulupa
- M. Swisdak
- Manolis K. Georgoulis
- N. M. Viall
- Oleksiy Agapitov
- P. Louarn
- Parisa Mostafavi
- R. A. Qudsi
- R. Bandyopadhyay
- R. C. Allen
- R. Chhiber
- R. J. MacDowall
- Rui Pinto
- S. Curry
- S. D. Bale
- S. E. Gibson
- S. Livi
- S. T. Badman
- S. T. Lepri
- S. Vargas Domínguez
- Salvatore Mancuso
- Sofiane Bourouaine
- T. Dudok de Wit
- T. N. Parashar
- T. Woolley
- Teresa Nieves‐Chinchilla
- Thomas Berger
- V. Krasnoselskikh
- V. M. Uritsky
- W. H. Matthaeus
Linked Collaborating Institutions
- Aberystwyth University, UK
- Academy of Athens, Research Center for Astronomy and Applied Mathematics
- American University, Washington DC
- Battelle Memorial Institute
- California Institute of Technology
- Catholic University, Washington DC
- Christian Albrechts University of Kiel, Germany
- Dartmouth College, New Hampshire
- Durham University, UK
- E.O. Hulburt Center for Space Research, NRL
- Ecole Polytechnique, LPP, Laboratoire de Physique des Plasmas
- Florida Institute of Technology
- GMU, School of Physics, Astronomy and Computational Sciences
- Georg August University of Gottingen, Germany
- George Mason University, Virginia
- Goddard Space Flight Center, Astrophysics Division
- Imperial College, Department of Physics
- Imperial College, London
- Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing
- Jet Propulsion Laboratory
- Johns Hopkins University, Applied Physics Laboratory
- Johns Hopkins University, Maryland
- Laboratoire de Physique et de Chimie de l'Environnement et de l'Espace, Orleans
- Lockheed Martin, Palo Alto
- Los Alamos National Laboratory, New Mexico
- Mahidol University, Thailand
- Massachusetts Institute of Technology
- Max-Planck-Institute for Solar System Research, Lindau
- Montana State University, Bozeman
- NASA Goddard Space Flight Center, Maryland
- NASA HQ
- NASA Marshall Space Flight Center
- National Center for Atmospheric Research, Colorado
- National Solar Observatory, Sunspot New Mexico
- National University of Colombia
- New Jersey Institute of Technology
- New Mexico State University
- Observatoire de Paris, France
- Predictive Science Inc., California
- Princeton University, Department of Astrophysical Sciences
- Princeton University, New Jersey
- Queen Mary University, School of Physics and Astronomy
- Queen Mary University, UK
- Royal Holloway University of London
- Smithsonian Astrophysical Observatory
- Southwest Research Institute, Boulder
- Southwest Research Institute, Texas
- Space Science Institute, Colorado
- Stanford University, California
- U.S. Department of the Navy, Naval Research Laboratory, Washington DC
- U.S. Environmental Protection Agency
- Universite d'Orleans, France
- University College London, Mullard Space Science Laboratory
- University of Alabama, Huntsville
- University of Alabama, Huntsville, Department of Physics
- University of Alcala, Spain
- University of Arizona
- University of Arizona, Department of Planetary Sciences
- University of California, Berkeley
- University of California, Berkeley, Department of Astronomy
- University of California, Berkeley, Department of Physics
- University of California, Berkeley, Space Sciences Laboratory
- University of California, Los Angeles
- University of California, Los Angeles, Institute of Geophysics and Planetary Physics
- University of Colorado, Boulder
- University of Colorado, Boulder, Department of Astrophysical and Planetary Sciences
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Delaware
- University of Delaware, Department of Physics and Astronomy
- University of Iowa
- University of Iowa, Department of Physics and Astronomy
- University of Kiel, Institute for Experimental and Applied Physics
- University of Liege, Department of Astrophysics, Geophysics and Oceanography
- University of Maryland, Baltimore County
- University of Maryland, College Park
- University of Michigan
- University of Michigan, Department of Atmospheric Oceanic and Space Sciences
- University of Minnesota, School of Physics and Astronomy
- University of Minnesota, Twin Cities
- University of New Hampshire
- University of Otago, New Zealand
- University of Oxford, UK
- University of Virginia
- University of Wisconsin, Madison
- Victoria University of Wellington, New Zealand
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