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1. Patchy Proton Aurora at Mars: A Global View of Solar Wind Precipitation Across the Martian Dayside From EMM/EMUS

3. Discrete Aurora on the Nightside of Mars: Occurrence Location and Probability

7. Mars pickup ion plume under different IMF conditions from MAVEN observations

9. A MAVEN case study of radial IMF at Mars: impacts on the dayside ionosphere

11. The global current systems of the Martian induced magnetosphere

12. Energetic Neutral Atoms at Mars: Predicted Distributions Based on MAVEN Measurements

13. Influence of Extreme Ultraviolet Irradiance Variations on the Precipitating Ion Flux From MAVEN Observations

16. Particle‐In‐Cell Modeling of Martian Magnetic Cusps and Their Role in Enhancing Nightside Ionospheric Ion Escape

17. Mars Dust Storm Effects in the Ionosphere and Magnetosphere and Implications for Atmospheric Carbon Loss

18. Influence of the solar wind dynamic pressure on the ion precipitation: MAVEN observations and simulation results

19. Energetic Neutral Atoms near Mars: Predicted Distributions Based on MAVEN Measurements

20. Spatial variations in the dust-to-gas ratio of Enceladus’ plume

21. The Morphology of the Solar Wind Magnetic Field Draping on the Dayside of Mars and Its Variability

22. Statistical analysis of the reflection of incident O+ pickup ions at Mars: MAVEN observations

23. The Mars crustal magnetic field control of plasma boundary locations and atmospheric loss: MHD prediction and comparison with MAVEN

24. Seasonal variability of Martian ion escape through the plume and tail from MAVEN observations

26. Mars Upper Atmospheric Responses to the 10 September 2017 Solar Flare: A Global, Time-Dependent Simulation

27. Space Weather Storm Responses at Mars: Lessons from A Weakly Magnetized Terrestrial Planet

28. O + ion beams reflected below the Martian bow shock: MAVEN observations

29. An Artificial Neural Network for Inferring Solar Wind Proxies at Mars

30. Loss of the Martian atmosphere to space: Present-day loss rates determined from MAVEN observations and integrated loss through time

31. Modeling the total dust production of Enceladus from stochastic charge equilibrium and simulations

32. Strong plume fluxes at Mars observed by MAVEN: An important planetary ion escape channel

33. Multifluid MHD study of the solar wind interaction with Mars' upper atmosphere during the 2015 March 8th ICME event

34. MHD model results of solar wind interaction with Mars and comparison with MAVEN plasma observations

35. A model of the spatial and size distribution of Enceladus׳ dust plume

36. MAVEN observations of the response of Mars to an interplanetary coronal mass ejection

37. Response of Mars O+ pickup ions to the 8 March 2015 ICME: Inferences from MAVEN data-based models

38. Early MAVEN Deep Dip campaign reveals thermosphere and ionosphere variability

39. The spatial distribution of planetary ion fluxes near Mars observed by MAVEN

40. Charged nanograins in the Enceladus plume

41. Multifluid MHD study of the solar wind interaction with Mars' upper atmosphere during the 2015 March 8th ICME event.

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