16 citations as recorded by crossref.

1. First 3D hybrid-Vlasov global simulation of auroral proton precipitation and comparison with satellite observations M. Grandin et al. 10.1051/swsc/2023017
2. UV Study of the Fourth Positive Band System of CO and O i 135.6 nm From Electron Impact on CO and CO2 J. Ajello et al. 10.1029/2018JA026308
3. Numerical simulation of the effects of a solar energetic particle event on the ionosphere of Mars V. Sheel et al. 10.1029/2011JA017455
4. Ionization processes in the atmosphere of Titan G. Gronoff et al. 10.1051/0004-6361/200912371
5. Atmospheric Escape Processes and Planetary Atmospheric Evolution G. Gronoff et al. 10.1029/2019JA027639
6. Polar cap arcs from the magnetosphere to the ionosphere: kinetic modelling and observations by Cluster and TIMED R. Maggiolo et al. 10.5194/angeo-30-283-2012
7. Separating and quantifying ionospheric responses to proton and electron precipitation over Svalbard B. Lanchester et al. 10.1029/2011JA016474
8. The Kinetic Monte Carlo Model of the Auroral Electron Precipitation into N2-O2 Planetary Atmospheres D. Bisikalo et al. 10.3390/universe8080437
9. Dayglow on Mars: Kinetic modelling with SPICAM UV limb data C. Simon et al. 10.1016/j.pss.2008.08.012
10. The precipitation of keV energetic oxygen ions at Mars and their effects during the comet Siding Spring approach G. Gronoff et al. 10.1002/2014GL060902
11. Advancing Our Understanding of Martian Proton Aurora Through a Coordinated Multi‐Model Comparison Campaign A. Hughes et al. 10.1029/2023JA031838
12. Cross sections for the O II (83.4 nm) emission from electron impact on O2 C. Malone et al. 10.1029/2008JA013160
13. The auroral red line polarisation: modelling and measurements J. Lilensten et al. 10.1051/swsc/2015027
14. H Balmer lines in terrestrial aurora: Historical record and new observations by OSIRIS on Odin R. Gattinger et al. 10.1029/2010JA015338
15. What characterizes planetary space weather? J. Lilensten et al. 10.1007/s00159-014-0079-6
16. Energy mapping of Jupiter’s auroral electrons from Juno/UVS data using a new H2 UV emission model B. Benmahi et al. 10.1051/0004-6361/202348634