First-authored, refereed papers of H. Hotta

A list of first-authored, refereed publications of H. Hotta, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-6312-7944

List of publications ordered by citations
Number of papers: 19
No. of citations: 714

2022

1. Generation of Solar-like Differential Rotation [32]
   Hotta, H., Kusano, K. & Shimada, R., ApJ, 933, 199

2021

1. Solar differential rotation reproduced with high-resolution simulation [42]
   Hotta, H. & Kusano, K., Nature Astronomy, 5, 1100

2020

1. Formation of superstrong horizontal magnetic field in delta-type sunspot in radiation magnetohydrodynamic simulations [9]
   Hotta, H. & Toriumi, S., MNRAS, 498, 2925
2. On rising magnetic flux tube and formation of sunspots in a deep domain [29]
   Hotta, H. & Iijima, H., MNRAS, 494, 2523

2019

1. Weak influence of near-surface layer on solar deep convection zone revealed by comprehensive simulation from base to surface [42]
   Hotta, H., Iijima, H. & Kusano, K., Science Advances, 5, 2307

2018

1. Breaking Taylor-Proudman Balance by Magnetic Fields in Stellar Convection Zones [11]
   Hotta, H., ApJ, 860, L24

2017

1. Spatial Inhomogeneity of Kinetic and Magnetic Dissipations in Thermal Convection [1]
   Hotta, H., ApJ, 845, 164
2. Solar Overshoot Region and Small-scale Dynamo with Realistic Energy Flux [47]
   Hotta, H., ApJ, 843, 52

2016

1. Large-scale magnetic fields at high Reynolds numbers in magnetohydrodynamic simulations [102]
   Hotta, H., Rempel, M. & Yokoyama, T., Science, 351, 1427

2015

1. Efficient Small-scale Dynamo in the Solar Convection Zone [56]
   Hotta, H., Rempel, M. & Yokoyama, T., ApJ, 803, 42
2. High-resolution Calculation of the Solar Global Convection with the Reduced Speed of Sound Technique. II. Near Surface Shear Layer with the Rotation [84]
   Hotta, H., Rempel, M. & Yokoyama, T., ApJ, 798, 51

2014

1. High-resolution Calculations of the Solar Global Convection with the Reduced Speed of Sound Technique. I. The Structure of the Convection and the Magnetic Field without the Rotation [64]
   Hotta, H., Rempel, M. & Yokoyama, T., ApJ, 786, 24

2012

1. Magnetic Field Intensification by the Three-dimensional "Explosion" Process [11]
   Hotta, H., Rempel, M. & Yokoyama, T., ApJ, 759, L24
2. Estimation of Turbulent Diffusivity with Direct Numerical Simulation of Stellar Convection [7]
   Hotta, H., Iida, Y. & Yokoyama, T., ApJ, 751, L9
3. Generation of twist on magnetic flux tubes at the base of the solar convection zone [8]
   Hotta, H. & Yokoyama, T., A&A, 548, A74
4. Numerical calculation of convection with reduced speed of sound technique [43]
   Hotta, H., Rempel, M., Yokoyama, T., Iida, Y. & Fan, Y., A&A, 539, A30

2011

1. Modeling of Differential Rotation in Rapidly Rotating Solar-type Stars [28]
   Hotta, H. & Yokoyama, T., ApJ, 740, 12

2010

1. Solar Parity Issue with Flux-transport Dynamo [62]
   Hotta, H. & Yokoyama, T., ApJ, 714, L308
2. Importance of Surface Turbulent Diffusivity in the Solar Flux-Transport Dynamo [36]
   Hotta, H. & Yokoyama, T., ApJ, 709, 1009