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1. The Ninth NTIRE 2024 Efficient Super-Resolution Challenge Report

6. Three-dimensional magnetic reconnection in astrophysical plasmas

7. Evidence for lunar tide effects in Earth’s plasmasphere

11. Direct Observation of Short Large-Amplitude Magnetic Field Structures from Formation to Destruction.

12. Statistical Analysis of Whistler Precursors Upstream of Foreshock Transient Shocks: MMS Observations

14. Statistical analysis of whistler precursors upstream of foreshock transient shocks : MMS observations

15. Dayside Magnetodisk Reconnection in Jovian System: Galileo and Voyager Observation.

17. Comparison of formulas for resonant interactions between energetic electrons and oblique whistler-mode waves

18. Effects of Plasma Density on the Spatial and Temporal Scale Sizes of Plasmaspheric Hiss.

21. Observation of electron and ion gyroscale vortices in the terrestrial magnetosheath

25. Possible Formation Mechanism of Lunar Hematite

26. Juno's multi-instruments observations during the flybys of auroral bright spots in Jupiter's polar aurorae

27. Evidence of plasma lunar tide in the Earth-Moon system

29. Motion of Classic and Spontaneous Hot Flow Anomalies Observed by Cluster

30. Determining the Global Scale Size of Chorus Waves in the Magnetosphere

31. Revealing the source of Jupiter’s x-ray auroral flares

34. Revealing the source of Jupiter’s x-ray auroral flares

35. Propagation characteristics of hot flow anomalies

40. Flying through a dawn storm: a multi-instrument study of the traversal of a dawn storm by Juno on February 7th 2018

41. Jupiter's aurora liveliness during solar minimum

42. Bright spot auroras in Jupiter’s polar region: Juno-UVS observations

43. Morphology of Jupiter's Polar Auroral Bright Spot Emissions via Juno-UVS Observations

45. The observational evidence of electron mirror mode

46. Electron acceleration in small-size magnetic holes

48. A wedgelet current system on Saturn

49. A three-dimensional model of spiral null pair to form ion-scale flux ropes in magnetic reconnection region observed by Cluster

50. Propagation properties of foreshock cavitons: Cluster observations

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