Raphaël Raynaud
3
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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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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