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This is the webpage of Hideyuki Hotta, who is a scientist of solar/stellar physics. I am a professor at Nagoya University, Japan
Data
Name: Hideyuki Hotta
Sex: male
Affiliation: Nagoya university
Date of birth: June 17th, 1985
e-mail: hotta.h_at_isee.nagoya-u.ac.jp (substitute _at_ to @)
Interested in: Fluid dynamics, Magnetohydrodynamics, Thermodynamics, Astronomy, Solar physics, Numerical Simulation
Hobby: guitar, music
Education
April, 2005 - March, 2009, University of Tokyo, Bachelor course
April, 2009 - March, 2011, University of Tokyo, Master course
April, 2011 - March, 2014, University of Tokyo, Doctor course (Docter of Science)
Work
April, 2011 - March, 2014 JSPS DC1
April, 2014 - August, 2015 JSPS for abroad, HAO/NCAR Scientific visitor
July, 2015 - Tenure-track assistant professor at Chiba university
July, 2020 - Assistant professor at Chiba university
August, 2020 - Associate professor at Chiba university
April, 2023 - Professor at Nagoya university
*JSPS stands for Japan Society for the Promotion of Science
Prize
The Commendation for Science and Technology by the Minister of Education, Culture, Sports, Science and Technology, The Young Scientists’ Award (2022)
ASJ Young Astronomer Award (2021)
AAPPS-DPP Young Researcher Award (2018)
APSPM best paper award for young scientist (2011)
Encouragement award from University of Tokyo (Doctor: 2014)
Encouragement award from University of Tokyo (Master: 2011)
Invited and plenary talks in international meetings
"Solar differential rotation reproduced with high resolution magnetohydrodynamic simulations", ICNSP2022, online
"Solar interior dynamics: Convection and Magnetic field", APPC15, 2022, online (plenary talk)
"Generation of the solar magnetic field", IAU GA, 2022, online
"Numerical simulation of solar convection zone and magnetic field", ITC30, 2021, online
"High resolution simulation of solar convection zone in Fugaku", AAPPS-DPP2021, 2021, online
"Correct reproduction of solar differential rotation in high-resolution simulation with Fugaku", JpGU Meeting 2021, 2021, online
"Solar convection and dynamo action", Future Directions in Solar, Stellar and Planetary Physics, 2020, Abu Dhabi, UAE
"Solar dynamo: achievements and perspective", Hinode-13/IPELS, 2019, Tokyo, Japan
"Solar and stellar dynamos", EASW9, 2019, Nagoya university, Japan
"Solar deep convection zone to surface", Space Climate 7, 2019, Quebec, Canada
"Solar and stellar convection and dynamo", ITC27 & APPTC2018, 2018, Gifu, Japan
"High Resolution Simulations of Solar Convection Zone and Dynamo", AAPPS-DPP2018, 2018, Kanazawa, Japan
"Calculation of solar convection zone with the reduced speed of sound technique", IAU General Assembly, 2018, Vienna, Austria
"Numerical simulation of solar global convection", Asteroseismology and its impact on other branches of astronomy, 2018, Tokyo, Japan
"Recent development of solar dynamo model", Asia Pacific Solar Physics Meeting, 2017, Kyoto, Japan
"High resolution calculation of solar dynamo", MPPC meeting, 2017, Greifswald, Germany
"High-resolution calculation of solar dynamo", MR2017, 2017, Matsuyama, Japan
"Solar global convection and dynamo with reduced speed of sound technique", 7th AICS international symposium, 2017, Kobe, Japan
"Small-scale dynamo in the solar convection zone", Solar and stellar magnetic fields: a conference in honor of Manfred Schüssler, 2016, Goslar, Germany
"Large-scale MHD simulation of solar convection zone and dynamo", EASW 2016, 2016, Tsukuba, Japan
"Small- and large-scale dynamos in the solar convection zone", ICPP2016, 2016, Kaoshiung, Takwan
"Simulating Solar Convection: State of the Art and Future", Advances in Seismology: a Dialogue Across Disciplines, 2015, Mumbai, India
"Current understanding and future path of the solar dynamo", 5th East-Asia School and Workshop on Laboratory, Space, and Astrophysical plasmas, 2015, Pohang, Korea
"Small- and Large-scale dynamo in the solar convection zone", NASA LWS Workshop on Solar Dynamo Frontiers: Helioseismology, 3D Modeling, and Data Assimilation, 2015, Boulder, USA
"High resolution calculation of solar global convection and dynamo", Sunspot formation: theory, simulations and observations, 2015, Stockholm, Sweden
"High resolution calculation of solar convection zone using K-computer", PLASMA2014, 2014, Niigata, Japan
"Solar differential rotation maintained by small- and large-scale convection", ASTRONUM, 2014, Long beech, USA
"Numerical simulations of multi-scale solar global convection", AGU fall meeting, 2013, San Francisco, USA
"Current status of understanding about solar global convection", The 7th Hinode science meeting, 2013, Hida, Japan
"Connection between the mean-field solar dynamo model and the self-consistent global convection model", AOGS 10th annual meeting, 2013, Australia
"Parity of solar global magnetic field determined by turbulent diffusivity in solar flux-transport dynamo", IUGG General Assembly 2011, 2011, Australia