Two papers have been published (COBISS.SI-ID: 2203748 and 2204004 ): Uncertainties of estimates of inertia-gravity energy in the atmosphere. Part 1: Intercomparison of four analysis systems. Part 2: Large-scale equatorial waves.
COBISS.SI-ID: 2203748
A confirmation that satellite-derived precipitation data are a useful source of this kind of information in the tropics and subtropics. Original to the paper is its upgrade of the MODE method, which allows an identification of objects in time and analysis of their development in time.
COBISS.SI-ID: 2191204
The ''Approach unifying spin and charges'' is the only one in the literature offering a mechanism for the appearance of families and explaining the origin of the ''bare'' quark and lepton masses and their transitions among families. It predicts the fourth family, which might be observed at the LHC and the stable fifth family with masses of several 105 times the proton mass. The article explains, in accordance with cosmological and direct measurements, evolution of the fifth family in the primordial plasma up to the creation of the dark matter and its interaction with ordinary matter.
COBISS.SI-ID: 2191972
We made a comprehensive multiwavelength temporal and spectral analysis of the `fast rise exponential decay' GRB 070419A. The early-time emission in the ?-ray and X-ray bands can be explained by a central engine active for at least 250 s, while later the X-ray light curve displays a simple power-law decay. In contrast, the observed behaviour in the optical band is complex. We ruled out a highly magnetized fireball and concluded that a long-lived central engine with a finely tuned energy injection rate and a sudden cessation of the injection is required to create the observed light curves.
COBISS.SI-ID: 322433
The compact radio source Sagittarius A (Sgr A) at the centre of our Galaxy harbours a massive black hole, whose mass has been measured from stellar orbital motions. Sgr A is therefore the nearest laboratory where massive black hole astrophysics can be tested, and the environment of black holes can be investigated. Since it is not an active galactic nucleus, it also offers the possibility of observing the capture of small objects that may orbit the central black hole. We studied the effects of the strong gravitational field of the black hole on small objects, such as a comet or an asteroid.
COBISS.SI-ID: 316801