11 citations · 28 across the 7 of their papers we have counts for
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Chromospheric heating and magnetic topology above the shared penumbra of a delta-spot: Multi-line inversions and multi-height magnetic-field extrapolations
M. Kriginsky, J. Leenaarts, J. de la Cruz Rodríguez +1
We analysed observations of the Fe I 617.3 nm, Ca II 854.2 nm, and Ca II H lines obtained with CRISP and CHROMIS at the SST. Spatially coupled non-LTE inversions constrained the ch…
The magnetic sensitivity of the Ca II H and K lines
M. Kriginsky, J. Leenaarts, J. de la Cruz Rodriguez +2
The solar chromosphere is a transition layer between the cool, dense photosphere and the hot, rarefied corona. This boundary region plays a key role in regulating energy transport…
On the magnetic and thermodynamic properties of dark fibrils in the chromosphere
Matheus Kriginsky, Ramon Oliver
Fibrillar structures are ubiquitous in the solar chromosphere and their potential for mediating the mass and energy transport in the solar atmosphere is undeniable. An accurate det…
Thermal and kinetic coronal rain diagnostics with MgII h & k lines
M. Kriginsky, R. Oliver
We performed the temperature diagnostics using inversions of data from nine spectroscopic observations obtained with the IRIS spectrograph in the MgII h & k lines. The sensitivity…
Temperature diagnostics of chromospheric fibrils
M. Kriginsky, R. Oliver, D. Kuridze
Context. Chromospheric fibrils are thin and elongated structures that connect nearby photospheric magnetic field concentrations of opposite polarities. Aims. We assess the possibil…
Magnetic field inference in active region coronal loops using coronal rain clumps
M. Kriginsky, R. Oliver, P. Antolin +2
Aims. We aim to infer information about the magnetic field in the low solar corona from coronal rain clumps using high-resolution spectropolarimetric observations in the Ca ii 8542…
Ubiquitous hundred-Gauss magnetic fields in solar spicules
M. Kriginsky, R. Oliver, N. Freij +3
Aims. We use high-resolution spectropolarimetric observations in the Ca ii 8542 A line obtained with the SST to study the magnetic field in solar spicules. Methods. The equations t…