activity
20072023
most citedChromospheric Anemone Jets as Evidence of Ubiquitous Reconnection

436 citations · 1.8k across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.SR2023★ 14 cited

A Comprehensive Simulation of Solar Wind Formation from the Solar Interior: Significant Cross-field Energy Transport by Interchange Reconnection near the Sun

H. Iijima, T. Matsumoto, H. Hotta +1

The physical connection between thermal convection in the solar interior and the solar wind remains unclear due to their significant scale separation. Using an extended version of…

nucl-th2021★ 2 cited

Dineutron in the state of He

Shoya Ogawa, Takuma Matsumoto

We investigate the dineutron in the state of He via analysis of its decay mode by using the complex scaling method. In this letter, we propose the cross section for the…

astro-ph.SR2021★ 81 cited

Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE): I. Coronal Heating

Bart De Pontieu, Paola Testa, Juan Martinez-Sykora +24

The Multi-slit Solar Explorer (MUSE) is a proposed NASA MIDEX mission, currently in Phase A, composed of a multi-slit EUV spectrograph (in three narrow spectral bands centered arou…

nucl-th2021

Investigation of multi-step effects for proton inelastic scattering to the state in He

Shoya Ogawa, Takuma Matsumoto, Yoshiko Kanada-En'yo +1

Multi-step effects between bound, resonant, and non-resonant states have been investigated by the continuum-discretized coupled-channels method (CDCC). In the CDCC, a resonant stat…

nucl-th2021★ 8 cited

Three-body description of C: Role of low-lying resonances in breakup reactions

Jagjit Singh, Takuma Matsumoto, Tokuro Fukui +1

The C nucleus and related capture reaction, , have been intensively studied with an astrophysical interest. Due to the weakly-bound nature of…

astro-ph.SR2020★ 28 cited

Full compressible 3D magnetohydrodynamic simulation of solar wind

Takuma Matsumoto

Identifying the heating mechanisms of the solar corona and the driving mechanisms of solar wind are key challenges in understanding solar physics. A full three-dimensional compress…