activity
20102023
most citedSurvival of Terrestrial N2-O2 Atmospheres in Violent XUV Environments through Efficient Atomic Line Radiative Cooling

57 citations · 172 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2023★ 2 cited

Strong depletion of C in CO induced by photolysis of CO in the Martian atmosphere calculated by a photochemical model

Tatsuya Yoshida, Shohei Aoki, Yuichiro Ueno +7

The isotopic signature of atmospheric carbon offers a unique tracer for the history of the Martian atmosphere and the origin of organic matter on Mars. Photolysis of CO is kn…

astro-ph.IM2023

Photochemical and RadiatiOn Transport model for Extensive USe (PROTEUS)

Yuki Nakamura, Naoki Terada, Shungo Koyama +10

We introduce a new flexible one-dimensional photochemical model named Photochemical and RadiatiOn Transport model for Extensive USe (PROTEUS), which consists of a Python graphical…

astro-ph.EP2022★ 3 cited

Modeling of geocoronal solar wind charge exchange events detected with Suzaku

Daiki Ishi, Kumi Ishikawa, Yoshizumi Miyoshi +2

A model of geocoronal solar wind charge exchange (SWCX) emission was built and compared to five Suzaku detections of bright geocoronal SWCX events. An exospheric neutral hydrogen d…

astro-ph.EP2022★ 57 cited

Survival of Terrestrial N2-O2 Atmospheres in Violent XUV Environments through Efficient Atomic Line Radiative Cooling

Akifumi Nakayama, Masahiro Ikoma, Naoki Terada

Atmospheres play a crucial role in planetary habitability. Around M dwarfs and young Sun-like stars, planets receiving the same insolation as the present-day Earth are exposed to i…

astro-ph.EP2022★ 32 cited

Less effective hydrodynamic escape of H-HO atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs

Tatsuya Yoshida, Naoki Terada, Masahiro Ikoma +1

Terrestrial planets currently in the habitable zones around M dwarfs likely experienced a long-term runaway greenhouse condition because of a slow decline in host-stellar luminosit…

astro-ph.SR2019★ 17 cited

Suzaku detection of enigmatic geocoronal solar wind charge exchange event associated with coronal mass ejection

Daiki Ishi, Kumi Ishikawa, Masaki Numazawa +5

Suzaku detected an enhancement of soft X-ray background associated with solar eruptions on 2013 April 14-15. The solar eruptions were accompanied by an M6.5 solar flare and a coron…

astro-ph.EP2011★ 6 cited

X-ray Observation of Mars with Suzaku at Solar Minimun

Kumi Ishikawa, Yuichiro Ezoe, Takaya Ohashi +2

Mars was observed in X-rays during April 3-5 2008 for 82 ksec with the Japanese Suzaku observatory. Mars has been known to emit X-rays via the scattering of solar X-rays and via th…

astro-ph.EP2011★ 28 cited

Enhancement of Terrestrial Diffuse X-ray Emission Associated With Coronal Mass Ejection and Geomagnetic Storm

Yuichiro Ezoe, Yoshizumi Miyoshi, Hiroshi Yoshitake +4

We present an analysis of a Suzaku observation taken during the geomagnetic storm of 2005 August 23-24. We found time variation of diffuse soft X-ray emission when a coronal mass e…

astro-ph.EP2010

Time Variability of the Geocoronal Solar Wind Charge Exchange in the Direction of the Celestial Equator

Yuichiro Ezoe, Ken Ebisawa, Noriko Y. Yamasaki +5

We report the detection of a time variable OVII line emission in a deep 100 ks Suzaku X-ray Imaging Spectrometer spectrum of the Galactic Ridge X-ray emission. The observed line in…

astro-ph.EP2010★ 27 cited

Discovery of Diffuse Hard X-ray Emission around Jupiter with Suzaku

Yuichiro Ezoe, Kumi Ishikawa, Takaya Ohashi +4

We report the discovery of diffuse hard (1-5 keV) X-ray emission around Jupiter in a deep 160 ks Suzaku XIS data. The emission is distributed over ~16x8 Jovian radius and spatially…