152 citations
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- Polish Academy of SciencesPL63 papers
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6 papers · 1 filter
Plasma dynamics in the flaring loop observed by RHESSI
T. Mrozek, R. Falewicz, S. Kolomanski +1
The thick-target model predicts that in flare foot points, we should observe lowering of HXR sources' altitude with increasing energy. The foot point of HXR sources result from the…
The influence of individual stars on the long-term dynamics of comets C/2014 UN271 and C/2017 K2
Piotr A. Dybczyński, Małgorzata Królikowska
In June 2021 the discovery of an unusual comet C/2014 UN271 Bernardinelli-Bernstein has been announced. Its cometary activity beyond Uranus orbit also has refreshed interest in sim…
Influence of Heliolatitudinal Anisotropy of Solar FUV/EUV Emissions on Lyman-alpha Helioglow: SOHO/SWAN Observations and WawHelioGlow Modeling
Marek Strumik, Maciej Bzowski, Marzena A. Kubiak
Observations of the Sun's surface suggest a nonuniform radiated flux as related to the presence of bright active regions and darker coronal holes. The variations of the FUV/EUV sou…
Exploring the link between star and planet formation with Ariel
Diego Turrini, Claudio Codella, Camilla Danielski +22
The goal of the Ariel space mission is to observe a large and diversified population of transiting planets around a range of host star types to collect information on their atmosph…
Local acceleration of protons to 100 keV in a quasi-parallel bow shock
Krzysztof Stasiewicz, Bengt Eliasson, Ian J. Cohen +2
Recent observations in the quasi-parallel bow shock by the MMS spacecraft show rapid heating and acceleration of ions up to an energy of about 100 keV. It is demonstrated that a pr…
Recurrence of galactic cosmic rays intensity and anisotropy in solar minima 23/24 and 24/25 by ACE/CRIS, STEREO, SOHO/EPHIN and neutron monitors. Fourier and wavelet analysis. Dedicated to the Memory of Michael Alania
R. Modzelewska, A. Gil
Aims. We study the 27-day variations of galactic cosmic rays (GCRs) based on neutron monitor (NM), ACE/CRIS, STEREO and SOHO/EPHIN measurements, in solar minima 23/24 and 24/25 cha…