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Water stress is an indicator that plant are suffering from drought. For optimization of the crop production is necessary to indicate physiological changes, those can be represented by stem expansion or shrinkage and sap flow rate. We used the Dynagage SGA5-WS (Dynamax) sensors for the sap flow monitoring and the sensors Diameter Dendrometer Small (Ecomatik) for measuring branches diameter changes in our research. The research was realized during two seasons, in the summer (from 31st July to 14th August 2018) and in the spring (from 27th March to 14th April 2019). The subject in our research were walnut trees (Juglans regia) situated in the private orchard in Nové Zámky area in Slovak Republic. The sap flow values in summer were on average range of 90 g.h-1, with maximum measured values above 160 g.h-1 measured after the precipitation events. After increasing of soil moisture on 1st and 2nd August 2018, it was detected the branches diameter expansion up to 0,05 mm. However, the other spring values were much lower. The sap flow reached less than 35 g.h-1 what was one third values in summer 2018. This phenomenon is a result of the low transpiration intensity of transpiration or a leafless state of trees. Although the changes in diameter were not significant in the early vegetation stage, there were monitored some fluctuation causing the diameter was shrinked by 0,2 mm due to a negative average air temperature.

Municipalities in Slovakia have a duty to separate biodegradable municipal waste (BDMW) from family houses. This duty can be achieved by home composting or by collection of green waste in bio-bins, which are regularly emptied by a collection company. Collected waste is recycled in a composting plant. Our research was focused on identifying the composition of collected green waste and comparing the environmental behaviour of residents in villages and towns. The analyses made by us showed that separated BDMW from urban population has a higher rate of contamination, but a lower rate of compostable kitchen waste compared to residents in villages.

In this work, we investigate the possibility of transporting material to the NEO region via the 8:3 MMR with Jupiter, potentially even material released from the dwarf planet Ceres. By applying the FLI map method to the 8:3 MMR region in the orbital plane of Ceres, we were able to distinguish between stable and unstable orbits. Subsequently, based on the FLI maps (for mean anomaly M = 60° and also M = 30°), 500 of the most stable and 500 of the most unstable particles were integrated for $15\, \mathrm{Myr}$ for each map. Long-term integration in the case of M = 60° showed that most of the stable particles evolved, in general, in uneventful ways with only 0.8 per cent of particles reaching the limit of q ≤ 1.3 au . However, in the case of M = 30°, a stable evolution was not confirmed. Over 40 per cent of particles reached orbits with q ≤ 1.3 au and numerous particles were ejected to hyperbolic orbits or orbits with a > 100 au. The results for stable particles indicate that short-term FLI maps are more suitable for finding chaotic orbits, than for detecting the stable ones. A rough estimate shows that it is possible for material released from Ceres to get to the region of 8:3 MMR with Jupiter. A long-term integration of unstable particles in both cases showed that transportation of material via 8:3 MMR close to the Earth is possible.

Changes in the distribution of annual rainfall totals, together with the increase in temperature over the last 40 years, are causing more frequent periods of drought, and plants are more often exposed to water stress. The aim of this study was to monitor the effect of different water regimes (irrigated and non-irrigated) of individuals of walnut tree (Juglans regia L.) in a private orchard located in the West of Slovakia. Our research was focused on dendrometric and sap flow measurements in the period from 28 March to 2 June 2019. The results showed differences in the sap flow of walnut trees during the budbreak period: when trees were irrigated, sap flow in the diurnal cycle was around 130 g·h−1 (20.48%), higher than in the non-irrigated treatment. Dendrometric differences between the irrigated and non-irrigated treatments were not significant. The sap flow data in the flowering period of the irrigated variant were slightly higher at 150 g·h−1 (35.62%) than non-irrigated. Dendrometric differences were more significant when the difference between the variants was more than 1.5 mm. Continuation of this research and analysis of the data obtained in the coming years will allow us to evaluate the effects of the environment on fruit trees in the long term.

Koncatinovocievna arteriova ischemicka choroba (periferne arteriove ochorenie dolných koncatin - PAO DK) je doležitou manifestaciou systemovej aterosklerozy a iných arteriových chorob cievneho systemu. Cim nižsi je clenkovo-ramenový tlakový index, tým vacsie je riziko vzniku zavažných akutnych instabilných organovaskularnych prihod (napr. akutneho infarktu myokardu, nahlej cievnej mozgovej prihody). V praci sa rozobera komplexna prevencia a liecba koncatinovocievnej arteriovej choroby. Angiologia/vaskularna medicina je najrýchlejsie sa rozvijajucou specializaciou internej mediciny.

Apollo-type asteroids Bennu and Ryugu are currently targets of sample-return missions. The goal of OSIRIS-REx mission (NASA) is to explore asteroid Bennu and Ryugu is being probed by JAXA’s Hayabusa2 mission. Observations of Bennu in January 2019 revealed ejecting material in the close proximity of the asteroid. Here we peresent our results of studying orbital evolution of potential meteoroid streams along the orbits of Bennu and Ryugu by integrating over 5000 test particles each for 1000 yr. We searched for their approaches to the Earth and we were also interested in evolution of their Earth MOIDs in order to estimate possible activity of potential meteor showers. Our results indicate possible observability from the Earth approximately for next 400 - 500 yr in both cases. Theoretical radiants for both asteroids and their potential meteor showers were also calculated.

Apollo-type asteroids Bennu and Ryugu are currently targets of sample-return missions. The goal of OSIRIS-REx mission (NASA) is to explore asteroid Bennu and Ryugu is being probed by JAXA’s Hayabusa2 mission. Observations of Bennu in January 2019 revealed ejecting material in the close proximity of the asteroid. In this paper, we study orbital evolution of potential meteoroid streams along the orbits of Bennu and Ryugu by integrating over 5000 test particles each for 1000 y r . We searched for their approaches to the Earth and we were also interested in evolution of their Earth MOIDs in order to estimate possible activity of potential meteor showers. Our results indicate possible observability from the Earth approximately for next 400 − 500 y r in both cases. Theoretical radiants for both asteroids and their potential meteor showers were also calculated.

Aims. Prior to 2019, the June epsilon Ophiuchids (JEO) were known as a minor unconfirmed meteor shower with activity that was considered typically moderate for bright fireballs. An unexpected bout of enhanced activity was observed in June 2019, which even raised the possibility that it was linked to the impact of the small asteroid 2019 MO near Puerto Rico. Early reports also point out the similarity of the shower to the orbit of the comet 300P/Catalina. We aim to analyze the orbits, emission spectra, and material strengths of JEO meteoroids to provide a characterization of this stream, identify its parent object, and evaluate its link to the impacting asteroid 2019 MO. Methods. Our analysis is based on a sample of 22 JEO meteor orbits and four emission spectra observed by the AMOS network at the Canary Islands and in Chile. The meteoroid composition was studied by spectral classification based on relative intensity ratios of Na, Mg, and Fe. Heliocentric orbits, trajectory parameters, and material strengths were determined for each meteor and the mean orbit and radiant of the stream were calculated. The link to potential parent objects was evaluated using a combination of orbital-similarity D-criteria and backwards integration of the orbit of comet 300P and the JEO stream. Results. We confirm the reports of an unexpected swarm of meteoroids originating in the JEO stream. JEO meteoroids have low material strengths characteristic for fragile cometary bodies, and they exhibit signs of a porous structure. The emission spectra reveal slightly increased iron content compared to all other measured cometary streams, but they are generally consistent with a primitive chondritic composition. Further dynamical analysis suggests that the JEO stream is likely to originate from comet 300P/Catalina and that it was formed within the last 1000 yr. Over longer timescales, the meteoroids in the stream move to chaotic orbits due to the turbulent orbital evolution of the comet. Our results also suggest that the impact of the small asteroid 2019 MO on June 22 was not connected to the JEO activity.

Organovascular arterial ischemic diseases (cardiovascular, cerebrovascular, extremitovascular, renovascular, genitovascular, pulmovascular, mesenterovascular, dermovascular, oculovascular, otovascular, stomatovascular etc.) are an important manifestations of systemic atherosclerosis and other arterial diseases of vascular system (arteriolosclerosis/arteriolonecrosis; diabetic macroangiopathy; diabetic microangiopathy; Mönckeberg´s mediosclerosis/mediocalcinosis; arteritis - vasculitis; syndromes of arterial compression; fibromuscular dysplasia; cystic adventitial degeneration; arterial thrombosis; arterial embolism/thromboembolism; traumatic and posttraumatic arteriopathies; physical arteriopathies; chemical and toxic arteriopathies; iatrogenic arterial occlusions; dissection of aorta and of arteries; coiling; kinking; complicated arterial aneurysms; arteriovenous fistula, rare vascular diseases). Key clinical-etiology-anatomy-pathophysiology (CEAP) aspects of the mesenteriovascular arterial ischemic diseases are discussed in this article (project Vessels).

We report the presentation and novel therapy of a calcitonin-secreting pancreatic neuroendocrine tumor (PNET) and review the literature on this unusual neoplasm.We cite the history of a 38-year-old male who presented with fatigue, weight loss, and diarrhea and was found to have a pancreatic head mass on cross-sectional imaging, as well as liver metastases.The patient's laboratory evaluation was notable for a100-fold elevation of the peptide hormone calcitonin in serum. As calcitonin is typically secreted by thyroid C-cells, hypercalcitoninemia is considered a marker for medullary thyroid cancer (MTC) or C-cell hyperplasia, but it may be present in several physiologic or pathologic conditions or may be ectopically secreted in rare PNETs. An octreotide scan confirmed the presence of somatostatin (SST) receptors on the pancreatic mass and liver metastases, leading to the diagnosis of a calcitonin-secreting PNET. We initiated treatment with long-acting SST analogs and peptide receptor radionuclide therapy (90Yttrium-DOTATOC) and achieved disease regression while maintaining a high quality of life.Functional PNETs that secrete calcitonin are exceedingly rare, but they are important to consider in the differential diagnosis of nonthyroid-mediated hypercalcitonemia or pancreatic tumors that present with diarrhea, as the management differs markedly from both MTC and other pancreatic malignancies.