activity
20092022
most citedAlfven Wave Solar Model (AWSoM): Coronal Heating

483 citations · 1.6k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.IM2022★ 5 cited

Connecting Solar and Stellar Flares/CMEs: Expanding Heliophysics to Encompass Exoplanetary Space Weather

B. J. Lynch, B. E. Wood, M. Jin +25

The aim of this white paper is to briefly summarize some of the outstanding gaps in the observations and modeling of stellar flares, CMEs, and exoplanetary space weather, and to di…

astro-ph.SR2022★ 31 cited

Coronal Mass Ejections and Dimmings: A Comparative Study using MHD Simulations and SDO Observations

Meng Jin, Mark C. M. Cheung, Marc L. DeRosa +2

Solar coronal dimmings have been observed extensively in the past two decades. Due to their close association with coronal mass ejections (CMEs), there is a critical need to improv…

astro-ph.SR2021★ 11 cited

Measurements of the magnetic field strengths at the bases of stellar coronae using the magnetic-field-induced transition theory

Yajie Chen, Xianyu Liu, Hui Tian +6

Measurements of the magnetic field in the stellar coronae are extremely difficult. Recently, it was proposed that the magnetic-field-induced transition (MIT) of the Fe X 257 Å line…

astro-ph.SR2021★ 28 cited

One Year in the Life of Young Suns: Data Constrained Corona-Wind Model of kappa1 Ceti

Vladimir S. Airapetian, Meng Jin, Theresa Lueftinger +5

The young magnetically active solar-like stars are efficient generators of ionizing radiation in the form of X-ray and Extreme UV (EUV) flux, stellar wind and eruptive events. Thes…

astro-ph.EP2020★ 44 cited

Atmospheric Escape From TOI-700 d: Venus versus Earth Analogs

Chuanfei Dong, Meng Jin, Manasvi Lingam

The recent discovery of an Earth-sized planet (TOI-700 d) in the habitable zone of an early-type M-dwarf by the Transiting Exoplanet Survey Satellite constitutes an important advan…

astro-ph.SR2020★ 31 cited

The solar wind from a stellar perspective: how do low-resolution data impact the determination of wind properties?

S. Boro Saikia, M. Jin, C. P. Johnstone +5

Alfvén-wave-driven 3D magnetohydrodynamic (MHD) models, which are increasingly used to predict stellar wind properties, contain unconstrained parameters and rely on low-resolution…