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1. A comparison of 3‐D model predictions of Mars' oxygen corona with early MAVEN IUVS observations. Issue 21 (5th November 2015)

2. Application of the Monte Carlo Method in Modeling Dusty Gas, Dust in Plasma, and Energetic Ions in Planetary, Magnetospheric, and Heliospheric Environments. Issue 2 (15th February 2021)