activity
20152019
most citedIs Proxima Centauri b habitable? -- A study of atmospheric loss

159 citations · 311 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.EP201978 cited

Planetary Magnetic Field Control of Ion Escape from Weakly Magnetized Planets

Hilary Egan, Riku Jarvinen, Yingjuan Ma +1

Intrinsic magnetic fields have long been thought to shield planets from atmospheric erosion via stellar winds; however, the influence of the plasma environment on atmospheric escap…

astro-ph.EP2018

Modeling Martian Atmospheric Losses over Time: Implications for Exoplanetary Climate Evolution and Habitability

Chuanfei Dong, Yuni Lee, Yingjuan Ma +11

In this Letter, we make use of sophisticated 3D numerical simulations to assess the extent of atmospheric ion and photochemical losses from Mars over time. We demonstrate that the…

astro-ph.EP2018

Solar wind interaction with the Martian upper atmosphere: Roles of the cold thermosphere and hot oxygen corona

Chuanfei Dong, Stephen W. Bougher, Yingjuan Ma +10

We study roles of the thermosphere and exosphere on the Martian ionospheric structure and ion escape rates in the process of the solar wind-Mars interaction. We employ a four-speci…

astro-ph.EP2017

Atmospheric escape from the TRAPPIST-1 planets and implications for habitability

Chuanfei Dong, Meng Jin, Manasvi Lingam +3

The presence of an atmosphere over sufficiently long timescales is widely perceived as one of the most prominent criteria associated with planetary surface habitability. We address…

astro-ph.EP2017159 cited

Is Proxima Centauri b habitable? -- A study of atmospheric loss

Chuanfei Dong, Manasvi Lingam, Yingjuan Ma +1

We address the important question of whether the newly discovered exoplanet, Proxima Centauri b (PCb), is capable of retaining an atmosphere over long periods of time. This is done…

astro-ph.EP201574 cited

The Interaction of Venus-like, M-dwarf Planets with the Stellar Wind of Their Host Star

O. Cohen, Y. Ma, J. J. Drake +4

We study the interaction between the atmospheres of Venus-like, non-magnetized exoplanets orbiting an M-dwarf star, and the stellar wind using a multi-species Magnetohydrodynaic (M…