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Taichi Kawamura

Associate Professor

Institut de Physique du Globe de Paris

France

Research Interests

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About

Taichi Kawamura is an Assistant Professor at Institut de physique du globe de Paris, Université Paris Cité, CNRS, located in Paris, France. His research focuses on geophysical studies related to planetary seismology, including investigations of subsurface sediments on Mars, seismic signal detection in atmospheric entries, and lunar seismic data analysis. His recent work also explores seismic wave detectability on Venus and deep moonquake source regions, highlighting his commitment to advancing our understanding of planetary geophysics.

Articles (25)

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Collaborators (22)

Thomas Bodin

Institute of Marine Sciences (ICM-CSIC)

SPAIN

Taichi Kawamura

Research Interests

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Articles (25)

Lateral Variations in Lunar Crustal Thickness Inferred From Apollo Seismic and GRAIL Gravity Data

A Physics‐Based Frequency‐Temperature Seismic Anelastic Attenuation Model for Planetary Ice Shells

Investigating the Detectability of Body Wave Phases From Tidal Ice Cracking Events on Titan With the Dragonfly Short‐Period Seismometer

Numerical Simulations of 3D Scattering Structures Reveal Systematic Underestimation of Marsquake Magnitudes

Apollo 17 Lunar Surface Gravimeter as a Seismometer: Relocating Shallow‐Moonquake Sources and Implications for Source Mechanism

Subsurface fluvial sediments beneath InSight on Mars from geophysical constraints

Exploring Seismic Signal Detection and Source Identification of Atmospheric Entries: The Hayabusa2 Sample Return Capsule as a Benchmark

Analysis of Chandrayaan‐3 Lunar Seismic Data: Performance Evaluation and Interpretation of Potential Natural Seismic Events

Elastic Properties of Returned Samples From Asteroid (162173) Ryugu

Methods for Cleaning Apollo Passive Seismic Data

Seismic Wave Detectability on Venus Using Ground Deformation Sensors, Infrasound Sensors on Balloons and Airglow Imagers

Inferring the Speed of Sound and Wind in the Nighttime Martian Boundary Layer From Impact‐Generated Infrasound

Predicting Deep Moonquake Source Regions Using Their Temporal and Spatial Patterns and Machine Learning

High‐ and Low‐Frequency Waveform Analysis the Marsquake of Sol 1222: Focal Mechanism, Centroid Moment Tensor Inversion and Source Time Function

Description of Martian Convective Vortices Observed by InSight and Implications for Vertical Vortex Structure and Subsurface Physical Properties

Seismic Scattering and Absorption Properties of Mars Estimated Through Coda Analysis on a Long‐Period Surface Wave of S1222a Marsquake

Detection of Mars Normal Modes From S1222a Event and Seismic Hum

Investigation of Martian Regional Crustal Structure Near the Dichotomy Using S1222a Surface‐Wave Group Velocities

The Global Seismic Moment Rate of Mars After Event S1222a

Differences in Scattering Properties of the Shallow Crusts of Earth, Mars, and the Moon Revealed by P‐Wave Receiver Functions

Evaluation of S1222a Source Parameters Based on Site Effect Simulation and Implication for the Event Origin

High‐Frequency Receiver Functions With Event S1222a Reveal a Discontinuity in the Martian Shallow Crust

Differences in Scattering Properties of the Shallow Crusts of Earth, Mars, and the Moon Revealed by <i>P</i>‐Wave Receiver Functions

Stratification of Heterogeneity in the Lithosphere of Mars From Envelope Modeling of Event S1222a and Near Impacts: Interpretation and Implications for Very‐High‐Frequency Events

S1222a—The Largest Marsquake Detected by InSight

Collaborators (22)

Thomas Bodin

Takuya Ishizaki

Josipa Majstorović

Scott McLennan

Zongbo Xu

Lu Pan

Antoine Lucas

Philippe Lognonné

Mark Panning

Takeshi Tsuji

Keisuke Onodera

Ryota Fukai

Benjamin Fernando

Henri Samuel

Hadrien Devillepoix

Yanbin Wang

Kiwamu Nishida

Brigitte Knapmeyer-Endrun

Constantinos Charalambous

Eleonore Stutzmann

Martin Knapmeyer

Mélanie Drilleau

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