H Eklund - Astronomy and Astrophysics, 2023 - ui.adsabs.harvard.edu
Context. The solar atmosphere is highly dynamic, and observing the small-scale features is valuable for interpretations of the underlying physical processes. The contrasts and …
H Eklund - Astronomy and Astrophysics (A & A), 2023 - duo.uio.no
Context. The solar atmosphere is highly dynamic, and observing the small-scale features is valuable for interpretations of the underlying physical processes. The contrasts and …
Context. The solar atmosphere is highly dynamic, and observing the small-scale features is valuable for interpretations of the underlying physical processes. The contrasts and …
Context. The solar atmosphere is highly dynamic, and observing the small-scale features is valuable for interpretations of the underlying physical processes. The contrasts and …
H Eklund - Astronomy and Astrophysics, 2023 - diva-portal.org
Aims. The estimates of the degradation associated with the observational angular resolution allows a more accurate analysis of the data. Methods. High-cadence time-series of synthetic …
H Eklund - arXiv preprint arXiv:2211.13629, 2022 - arxiv.org
The contrasts and magnitude of observable signatures of small-scale features degrade as angular resolution decreases. High-cadence time-series of synthetic observable maps at …
Context. The solar atmosphere is highly dynamic, and observing the small-scale features is valuable for interpretations of the underlying physical processes. The contrasts and …