132 citations · 696 across the 33 of their papers we have counts for
5 papers · 1 filter
Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes
F. Matković, R. Brajša, M. Temmer +6
This study investigates and compares brightness and area of coronal bright points (CBPs) inside and outside of coronal holes (CHs) using the single-dish Band 6 observations by the…
V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?
P. Harmanec, H. Božić, P. Koubský +21
A reliable determination of the basic physical properties and variability patterns of hot emission-line stars is important for understanding the Be phenomenon and ultimately, the e…
Variation in solar differential rotation and activity in the period 1964-2016 determined by the Kanzelhöhe data set
I. Poljančić Beljan, R. Jurdana-Šepić, T. Jurkić +8
We determined the differential rotation (DR) parameters and (corresponding to the equatorial rotation velocity and the gradient of the solar DR) by tracing sunspot groups i…
Correlation between the solar magnetic field strength and the millimeter brightness temperature
I. Skokić, D. Sudar, R. Brajša
Images of the Sun at millimeter wavelengths obtained by ALMA show a significant correspondence with the magnetograms. In this paper, we investigate this correspondence by comparing…
A prediction for the 25th solar cycle maximum amplitude
R. Brajša, G. Verbanac, M. Bandić +3
The minimum - maximum method, belonging to the precursor class of the solar activity forecasting methods, is based on a linear relationship between relative sunspot number in the m…