The paper explains why the solar activity index F30 is more suitable for ionospheric and thermospheric long-term trends.

The manuscript reports the first observations of continuum emission at the poleward boundary of the dayside auroral oval. The unique measurements show that a number of different emission lines and bands contribute to the broadband continuum emission. Even emission structures in the near and far infrared were observed, suggesting that multiple emitting species are responsible for the observed spectral enhancements. The authors suggest that the interplay of different heating mechanisms may be an important factor in the generation of high-latitude continuum emissions.

The study is devoted to a shock auroral event that occurred on February 26, 2023, in northern Scandinavia, and represents the first time such nighttime auroral features have been captured by ground-based cameras. Shock auroras result from a very specific driving impulse in the solar wind. While the primary effects appear on the dayside of the Earth, the authors succeeded in observing the nightside signatures, which are rare and difficult to detect. The study is a successful scientific achievement as it presents newly discovered phenomena that provide new insights into solar wind interactions with the nightside ionosphere.

This research significantly enhances our understanding of small-scale field-aligned currents observed in the cusp and auroral regions of the high-latitude ionosphere. The investigation utilizes dual-spacecraft high-resolution magnetic field measurements of the Swarm mission to reveal new characteristics of field-aligned currents across multiple scale sizes and temporal variations spanning 0.04 to 5 seconds.

This paper presents a statistical analysis of the aurora observed by the Swedish MATS satellite. These observations are new and can be an important contribution to high-latitude mesosphere/lower thermosphere science.

The paper represents a significant step forward in the numerical modelling of global ionospheric electrodynamics, incorporating the time-dependent effects of magnetic induction, with the potential for further extension to other planets in the Solar System.

The authors studied the effects of the geomagnetic mirror force on electron density enhancements in the polar atmosphere due to energetic electron precipitation. Considering this phenomenon in simulations this substantially reduced electron density, which was veryfied by observations. This could have wide consequences for the improvement of atmospheric ionization models.