101 citations · 373 across the 11 of their papers we have counts for
11 papers
The ratio of horizontal to vertical displacement in solar oscillations estimated from combined SO/PHI and SDO/HMI observations
J. Schou, J. Hirzberger, D. Orozco Suárez +44
In order to make accurate inferences about the solar interior using helioseismology, it is essential to understand all the relevant physical effects on the observations. One effect…
The magnetic drivers of campfires seen by the Polarimetric and Helioseismic Imager (PHI) on Solar Orbiter
F. Kahil, J. Hirzberger, S. K. Solanki +56
The Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter (SO) spacecraft observed small extreme ultraviolet (EUV) bursts, termed campfires, that have been proposed to be bri…
Temporal relations between magnetic bright points and the solar sunspot cycle
D. Utz, R. Muller, T. Van Doorsselaere
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a changing sunspot cycle featuring roughly an 11 year period. In addition we know that…
Long-term trends of magnetic bright points: I. Number of MBPs at disc centre
D. Utz, R. Muller, S. Thonhofer +5
Context. The Sun shows an activity cycle that is caused by its varying global magnetic field. During a solar cycle, sunspots, i.e. extended regions of strong magnetic fields, occur…
Magnetic field strength distribution of magnetic bright points inferred from filtergrams and spectro-polarimetric data
D. Utz, J. Jurčák, A. Hanslmeier +3
Small scale magnetic fields can be observed on the Sun in G-band filtergrams as MBPs (magnetic bright points) or identified in spectro-polarimetric measurements due to enhanced sig…
Variations of magnetic bright point properties with longitude and latitude as observed by Hinode/SOT G-band data
D. Utz, A. Hanslmeier, A. Veronig +4
Small-scale magnetic fields can be observed on the Sun in high resolution G-band filtergrams as magnetic bright points (MBPs). We study Hinode/ Solar Optical Telescope (SOT) longit…