Raphaël Raynaud
10
Documents
Identifiants chercheurs
- raphael-raynaud
- Arxiv : raynaud_r_1
- 0000-0001-6815-7109
- IdRef : 188243488
Présentation
#### **Physics Lecturer**
Université de Paris
CEA Saclay - UMR AIM
Orme des Merisiers, Bât. 709
91191 Gif-sur-Yvette - France
Email: *firstname.lastname\_AT\_cea.fr*
#### **Research Interests**
I am primarily interested in astrophysical fluid dynamics and nonlinear phenomena, with particular focus on thermal convection and magnetohydrodynamics (MHD). This branch of fluid dynamics describes the interaction of magnetic fields with electrically conducting fluid and is particularly important in explaining the magnetic properties of planets and stars, like the Earth or the Sun.
#### **Publications**
- **[ADS](http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?db_key=AST&db_key=PHY&db_key=PRE&qform=AST&arxiv_sel=astro-ph&arxiv_sel=cond-mat&arxiv_sel=cs&arxiv_sel=gr-qc&arxiv_sel=hep-ex&arxiv_sel=hep-lat&arxiv_sel=hep-ph&arxiv_sel=hep-th&arxiv_sel=math&arxiv_sel=math-ph&arxiv_sel=nlin&arxiv_sel=nucl-ex&arxiv_sel=nucl-th&arxiv_sel=physics&arxiv_sel=quant-ph&arxiv_sel=q-bio&sim_query=YES&ned_query=YES&adsobj_query=YES&aut_logic=OR&obj_logic=OR&author=raynaud%2C+r&object=&start_mon=&start_year=&end_mon=&end_year=&ttl_logic=OR&title=&txt_logic=OR&text=&nr_to_return=200&start_nr=1&jou_pick=ALL&ref_stems=&data_and=ALL&group_and=ALL&start_entry_day=&start_entry_mon=&start_entry_year=&end_entry_day=&end_entry_mon=&end_entry_year=&min_score=&sort=SCORE&data_type=SHORT&aut_syn=YES&ttl_syn=YES&txt_syn=YES&aut_wt=1.0&obj_wt=1.0&ttl_wt=0.3&txt_wt=3.0&aut_wgt=YES&obj_wgt=YES&ttl_wgt=YES&txt_wgt=YES&ttl_sco=YES&txt_sco=YES&version=1)**
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Gravity darkening in late-type stars. I. The Coriolis effectAstronomy and Astrophysics - A&A, 2018, 609 (A124), ⟨10.1051/0004-6361/201731729⟩
Article dans une revue
hal-01706693v1
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Dipolar dynamos in stratified systemsMonthly Notices of the Royal Astronomical Society, 2015, 448, pp.2055-2065. ⟨10.1093/mnras/stv122⟩
Article dans une revue
hal-01122919v1
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Topology and field strength in spherical, anelastic dynamo simulationsAstronomy and Astrophysics - A&A, 2014, 564 (A78), ⟨10.1051/0004-6361/201322801⟩
Article dans une revue
hal-01122251v1
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Influence of the mass distribution on the magnetic field topologyAstronomy and Astrophysics - A&A, 2014, 567 (A107), ⟨10.1051/0004-6361/201423902⟩
Article dans une revue
hal-01122419v1
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Gravity darkening in late-type stars7th BCool meeting, Apr 2018, Dublin, Ireland
Communication dans un congrès
hal-02428464v1
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Latitudinal flux variations of thermal anelastic convection in a rotating spherical shellCompressible Convection Conference, Sep 2017, Lyon, France
Communication dans un congrès
hal-02428465v1
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Dipolar dynamos in stratified systemsStellar and planetary dynamos, May 2015, Goettingen, Germany
Communication dans un congrès
hal-02428467v1
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Influence of the mass distribution on the magnetic field topologyEuropean GdR Dynamo, Sep 2014, Cambridge, United Kingdom
Communication dans un congrès
hal-02428474v1
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Topology and field strength in spherical, anelastic dynamo simulationsPoster de conférence hal-02428473v1 |
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The convective approximationsEuropean GdR Dynamo, Jul 2013, Ascona, Switzerland
Poster de conférence
hal-02428472v1
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