[2].  Recent Effects of small-scale dynamo on rotating columnar convection in stellar convection zones

Y. Bekki.
WHOLESUN Meeting 2025, Paris-Saclay, France, 10 Mar 2025 (Oral) 

[1].  Recent Advances in numerical modelling of solar inertial modes  [Invited / Plenary]

Y. Bekki., R. Cameron., and L. Gizon.
SDO 2025 Science Workshop: A Gathering of the Helio-hive!, Boulder, Colorado, 18 Feb 2025 (Oral) 

[4].  The Sun's differential rotation is controlled by baroclinically-unstable high-latitude inertial modes

Y. Bekki., R. Cameron., and L. Gizon.
17th European Solar Physics Meeting (ESPM-17),  Turin, Italy, 9 Sept 2024 (Oral)

[3].  Effects of small-scale dynamo on rotating columnar convection in stellar convection zones

Y. Bekki
NORDITA Workshop on Stellar Convection "Modelling, Theory, and Observations", 
Stockholm, Sweden, 26 Aug 2024 (Oral)

[2].  The Sun's differential rotation is controlled by baroclinically-unstable high-latitude inertial modes  [Invited]

Y. Bekki
International Astronomical Union (IAU) General Assembly (GA) 2024,  PhD Prize Winners Talks,
Division E "The Sun and Heliosphere", Cape Town, South Africa, 12 Aug 2024 (Oral)

[1].  The Sun's differential rotation is controlled by baroclinically-unstable inertial modes

Y. Bekki., R. Cameron., and L. Gizon.
WHOLESUN Meeting, Paris-Saclay., 13 Mar, 2024  (Oral)

[3].  The Sun's differential rotation is controlled by baroclinically unstable inertial modes

Solar Orbiter RS Working Group "Dynamo & Solar Cycle" Meeting,  online, 29 Jul, 2024

[2].  Baroclinic instability as an essential regulator of the Sun's differential rotation

COFFIES Seminar, Stanford Univ. (online), 9 Jul, 2024

[1].  Baroclinic instability: A hidden regulator of the Sun's differential rotation

ISEE Solar Seminar, Nagoya Univ. (online), 1 May, 2024

[3].  Numerical studies of solar inertial modes  [Invited]

Y. Bekki., R. Cameron., and L. Gizon.
American Geophysical Union (AGU) 2023, Session P23G "Oscillations in internal fluid layers of planets, moons, and stars"  
San Francisco, CA, USA & online., 12 Dec 2023 (Poster)

[2].  Solar inertial modes: What can we learn from them?

Y. Bekki., R. Cameron., and L. Gizon.
Asia-Pacific Regional IAU Meeting (APRIM), Fukushima, Japan, 7-11 Aug, 2023 (Poster)

[1].  Solar convective conundrum: Recent advances

Y. Bekki
Rinberg workshop on turbulence, Munich, Germany., 24 Jul, 2023

[2].  Baroclinically-unstable modes as an essential dynamical component of the Sun's convection zone

Solar & Cosmic Plasma (SCP) Seminar, Kyoto University, Japan, 17 August, 2023

[1].  Numerical modeling of inertial modes in the Sun's convection zone 

Fluid & MHD Seminar, Leeds UK (online), 16 March, 2023

[4].  Numerical modeling of solar inertial modes [Invited]

Y. Bekki., R. Cameron., and L. Gizon.
DY2W03 "Modeling, observing, and understanding flows and magnetic fields in the Earth's core and in the Sun",
INI, Cambridge, UK., 29 Nov, 2022 [link]

[3].  Modeling solar inertial modes [Invited]

Y. Bekki., R. Cameron., and L. Gizon.
CSS workshop "The Sun and planetary systems", NYUAD,  Abu-Dhabi, UAE., 10 Oct, 2022 [link]

[2].  Numerical studies of inertial modes in the Sun [Invited]

Y. Bekki., R. Cameron., and L. Gizon.
ISSI workshop "Solar and stellar dynamos: a new era", Bern, Switzerland., 16 Jun, 2022 [link]

[1].  Theory of solar oscillations in the inertial frequency range [Invited]

2021年度太陽研究連絡会シンポジウム, 博士論文発表会（オンライン開催）, 2022年2月16日

Doctoral Thesis Presentations, Japan Solar Physics Community (online), 16 Feb, 2022. 

[2].  Numerical challenges on modeling solar convection and dynamo

Computational Flow Physics (ComFyDA) Seminar, Max-Planck-Institute for Solar System Research, 5 Oct, 2022. 

[1].  Numerical studies on Rossby and other inertial modes in the Sun

Geo-Astrophysical Fluid Dynamics Seminar, University of Colorado Boulder (online), 27 Sept, 2022. [Abstract]

[3].  Baroclinic instability in the Sun: origin of the high-latitude inertial modes

Y. Bekki., R. Cameron., and L. Gizon.
WHOLESUN virtual Fall Meeting, online., 21-22 Sep, 2021  (Oral)

[2].  3D non-kinematic mean-field dynamo model

Y. Bekki., and R. Cameron.
WHOLESUN virtual Spring Meeting, online., 9-11 Mar, 2021  (Oral)

[1].  Detecting Rossby waves in simulations

Y. Bekki., R. Cameron., and L. Gizon.
WHOLESUN virtual Spring Meeting, online., 9-11 Mar, 2021  (Oral)

[1].  太陽対流層のロスビー波と傾圧不安定波の数値的研究
Numerical studies on Rossby and baroclinic waves in the Sun's convection zone

GFDセミナー, 地球流体電脳倶楽部（オンライン開催）, 2021年11月16日 [発表資料・講演動画]

Geophysical Fluid Dynamics (GFD) Seminar, GFD Dennou Club (Japan, online), 16 Nov, 2021. [Presentation files]

[3].  Rossby waves and rotationally-influenced convective modes in the solar convection simulation

Y. Bekki., R. Cameron., and L. Gizon.
Physics at the Equator: From Lab to the Stars, Lyon France., 16-18 Oct, 2019  (Poster)

[2].  Effects of rotation on convection

Y. Bekki., R. Cameron., and L. Gizon.
WHOLESUN Kick-off Meeting, Paris-Saclay France., 27-29 May, 2019  (Oral)

[1].  Examining the subsurface upper boundary condition in stratified magneto-convection simulation

Y. Bekki., and R. Cameron.
Flux Emergence Workshop 2019, Tokyo Japan., 18-22 Mar, 2019  (Oral)

[2].  太陽熱対流問題に対する高プラントル数の効果
Role of the effective Prandtl number on solar convective conundrum

日本天文学会 2018 春季年会, 千葉大学, 千葉  2018年3月16日（口頭）

ASJ annual spring meeting, Chiba, Japan, 16 Mar 2018 (Oral)

[1].  Deep convective amplitude and stratification in an effectively high-Prandtl number thermal convection

Y. Bekki., H. Hotta., and T. Yokoayama.
IAU Symposium 340, Jaipur India., 19-24 Feb, 2018  (Poster)

[5].  成層の変化を介した太陽熱対流速度抑制機構：実効的プラントル数の効果
Suppression mechanism of the solar convective amplitudes via the change in the mean stratification: Role of the effective Prandtl number

第30回 理論懇シンポジウム, 東京大学, 東京  2017年12月25-27日 （ポスター）

Riron-kon Symposium, The University of Tokyo, Tokyo, Japan, 25-27 Dec 2017 (Poster)

[4].  Effects of Prandtl number on stratified convection with and without rotation

Y. Bekki., H. Hotta., and T. Yokoayama.
Helicity Thinkshop 3, Tokyo Japan., 21 Nov, 2017  (Oral)

[3].  Effects of the enhanced subadiabatic layer in effectively high Prandtl number thermal convection

Y. Bekki., H. Hotta., and T. Yokoayama.
AAS 48th SPD Meeting, Portland, OR USA., 25 Aug, 2017  (Oral)

[2].  Numerical study of double-cell-type meridional circulation based on a mean-field hydrodynamic model

Y. Bekki.,  and T. Yokoayama.
JpGU-AGU Joint Meeting, Chiba Japan., 23 May, 2017  (Poster)

[1].  高プラントル数熱対流における回転の効果
Effects of rotation on thermal convection in an effectively high Prandtl number regime

太陽研究連絡会シンポジウム, JAXA/ISAS, 神奈川  2017年2月20-22日 （ポスター）

JSPC Symposium, JAXA/ISAS,  Kanagawa, Japan, 20-22 Feb 2017 (Poster)

[3].  Effects of Prandtl number on stratified convection with and without rotation

Magnetohydrodynamics (MHD) Seminar, Kyoto University, Kyoto, Japan, 1 Dec 2017 

[2].  Convective velocity suppression via the enhancement of subadiabatic layer: Role of the effective Prandtl number

HAO local seminar on solar dynamo group, HAO, Boulder, CO USA., 6 Sept 2017 

[1].  Double-cell solar meridional circulation based on a mean-field hydrodynamic model

Solar Space Plasma (SSP) Seminar, NAOJ, Tokyo, Japan, 19 May 2017 

[3].  平均場流体モデルに基づいた２セル型太陽子午面流の研究
Studies on two-cell-type solar meridional circulation based on a mean-field hydrodynamic model

CfCA ユーザーズミーティング, 国立天文台, 東京  2016年11月29-30日 （ポスター）

CfCA uers' meeting, NAOJ, Tokyo, Japan, 29-30 Nov 2016 (Poster)

[2].  平均場モデルに基づいた２セル子午面流の研究
Studies on two-cell meridional circulation using mean-field hydrodynamic model

日本天文学会 2016 秋季年会, 愛媛  2016年9月14日（口頭）

ASJ annual fall meeting, Ehime, Japan, 14 Sept 2016 (Oral)

[1].  Numerical study of double-cell meridional circulation based on a mean-field hydrodynamic model

Y. Bekki.,  and T. Yokoayama.
Hinode 10 Science Meeting, Nagoya Japan., 5-8 Sept, 2016  (Oral)