M. Putiš
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View article: Designing an API for a mineralogical database
Designing an API for a mineralogical database Open
An Application Programming Interface (API) is a secured, documented and accessible web service and an entry point to any database—both relational and non-relational. As a rule, it exposes the data in different formats and allows filt…
View article: A Review of the EUSO-Balloon Pathfinder for the JEM-EUSO Program
A Review of the EUSO-Balloon Pathfinder for the JEM-EUSO Program Open
EUSO-Balloon is a pathfinder for JEM-EUSO , the mission concept of a spaceborne observatory which is designed to observe Ultra-High Energy Cosmic Ray (UHECR)-induced Extensive Air Showers (EAS) by detecting their UltraViolet (UV) light tra…
View article: Origin and Age Determination of the Neotethys Meliata Basin Ophiolite Fragments in the Late Jurassic–Early Cretaceous Accretionary Wedge Mélange (Inner Western Carpathians, Slovakia)
Origin and Age Determination of the Neotethys Meliata Basin Ophiolite Fragments in the Late Jurassic–Early Cretaceous Accretionary Wedge Mélange (Inner Western Carpathians, Slovakia) Open
Constructive reviews of three
View article: EUSO-TA ground based fluorescence detector: analysis of the detected events
EUSO-TA ground based fluorescence detector: analysis of the detected events Open
EUSO-TA is a ground-based florescence detector built to validate the design of an ultra-high energy cosmic ray fluorescence detector to be operated in space. EUSO-TA detected the first air shower events with the technology developed within…
View article: EUSO-TA ground based fluorescence detector: analysis of the detected events
EUSO-TA ground based fluorescence detector: analysis of the detected events Open
EUSO-TA is a ground-based florescence detector built to validate the design of an ultra-high energy cosmic ray fluorescence detector to be operated in space. EUSO-TA detected the first air shower events with the technology developed within…
View article: Method for Analysis of the Effect of Geomagnetic Disturbances on Ultraviolet Airglow Intensity
Method for Analysis of the Effect of Geomagnetic Disturbances on Ultraviolet Airglow Intensity Open
Airglow is a dynamic phenomenon which depends on the geographical location, season, local time, geomagnetic activity, and other conditions. Variations in UV nighttime airglow (300–500 nm) caused by magnetospheric disturbances for several s…
View article: Implications for space-based UHECR observation from UV background light measurements by JEM-EUSO pathfinders
Implications for space-based UHECR observation from UV background light measurements by JEM-EUSO pathfinders Open
EUSO (Extreme Universe Space Observatory) is a next-generation space-based UHECR observation concept to detect extensive air shower events by the fluorescence technique. The determination of the exposure for UHECR observations is essential…
View article: Airglow dynamics observations by Mini-EUSO
Airglow dynamics observations by Mini-EUSO Open
Mini-EUSO ("UV atmosphere" in Russian Space Program) will observe Earth night side atmosphere from ISS in the UV band. The observed light consists mainly of light produced by airglow. We investigate the feasibility to observe airglow dynam…
View article: An analytically iterative method for solving problems of cosmic-ray modulation
An analytically iterative method for solving problems of cosmic-ray modulation Open
The development of an analytically iterative method for solving steady-state as well as unsteady-state problems of cosmic-ray (CR) modulation is proposed. Iterations for obtaining the solutions are constructed for the spherically symmetric…
View article: Cosmic Rays Propagation with HelMod: Difference between forward-in-time and backward-in-time approaches
Cosmic Rays Propagation with HelMod: Difference between forward-in-time and backward-in-time approaches Open
The cosmic rays modulation inside the heliosphere is well described by a transport equation introduced by Parker in 1965.To solve this equation several approaches were followed in the past.Recently the Monte Carlo approach becomes widely u…
View article: Night time measurement of the UV background by EUSO-Balloon
Night time measurement of the UV background by EUSO-Balloon Open
International audience
View article: Evaluation of scientific performance of JEM-EUSO mission with Space-X Dragon option
Evaluation of scientific performance of JEM-EUSO mission with Space-X Dragon option Open
International audience
View article: On the forward‐backward‐in‐time approach for Monte Carlo solution of Parker's transport equation: One‐dimensional case
On the forward‐backward‐in‐time approach for Monte Carlo solution of Parker's transport equation: One‐dimensional case Open
The cosmic rays propagation inside the heliosphere is well described by a transport equation introduced by Parker in 1965. To solve this equation, several approaches were followed in the past. Recently, a Monte Carlo approach became widely…
View article: Preliminary analysis of EUSO—TA data
Preliminary analysis of EUSO—TA data Open
The EUSO-TA detector is a pathfinder for the JEM-EUSO project and is currently installed in Black Rock Mesa (Utah) on the site of the Telescope Array fluorescence detectors. Aim of this experiment is to validate the observation principle o…