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1. Quantifying Properties of Photospheric Magnetic Cancellations in the Quiet Sun Internetwork

2. On the evolution of a sub-C class flare: a showcase for the capabilities of the revamped Catania Solar Telescope

3. Comparative case study of two methods to assess the eruptive potential of selected active regions

4. Continuum enhancements, line profiles and magnetic field evolution during consecutive flares

5. IRIS observations of magnetic interactions in the solar atmosphere between pre-existing and emerging magnetic fields. II. UV emission properties

6. IRIS observations of magnetic interactions in the solar atmosphere between pre-existing and emerging magnetic fields. I. Overall evolution

7. H${\alpha}$ and H${\beta}$ emission in a C3.3 solar flare: comparison between observations and simulations

8. Observational Evidence of a Flux Rope within a Sunspot Umbra

9. Polarised kink waves in magnetic elements: evidence for chromospheric helical waves

10. The pre-penumbral magnetic canopy in the solar atmosphere

11. Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

12. Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

13. An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory

14. Measurement of the cosmic ray spectrum above $4{\times}10^{18}$ eV using inclined events detected with the Pierre Auger Observatory

15. The magnetic structure of surges in small-scale emerging flux regions

16. The role of filament activation in a solar eruption

17. Observational evidence of torus instability as trigger mechanism for coronal mass ejections: the 2011 August 4 filament eruption

19. The Solar Activity Monitor Network – SAMNet

20. Firefly: The Case for a Holistic Understanding of the Global Structure and Dynamics of the Sun and the Heliosphere

22. Quo vadis, European Space Weather community?

23. IRIS Observations of Magnetic Interactions in the Solar Atmosphere Between Preexisting and Emerging Magnetic Fields. II. UV Emission Properties

24. Comprehensive Analysis of the Geoeffective Solar Event of 21 June 2015: Effects on the Magnetosphere, Plasmasphere, and Ionosphere Systems

26. The Solar Activity Monitor Network – SAMNet

27. Comprehensive Analysis of the Geoeffective Solar Event of 21 June 2015: Effects on the Magnetosphere, Plasmasphere, and Ionosphere Systems

33. Solar activity and its evolution across the corona: recent advances

35. Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory

36. Features of the energy spectrum of cosmic rays above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

37. Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

38. Measurement of the cosmic-ray energy spectrum above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

39. Measurement of the cosmic-ray energy spectrum above 2.5 ×10 18 eV using the Pierre Auger Observatory

40. Direct measurement of the muonic content of extensive air showers between 2 ×10 17 and 2 ×10 18 eV at the Pierre Auger Observatory

41. Features of the Energy Spectrum of Cosmic Rays above 2.5 ×10 18 eV Using the Pierre Auger Observatory

42. Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope

43. Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

44. IBIS2.0: The new Interferometric BIdimensional Spectrometer

47. Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory

48. Multi-Messenger Physics With the Pierre Auger Observatory

50. Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

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