Ecotoxicological assessment of mineralized stratum water as an environmentally friendly substitute for agrochemicals

Received: May 2nd, 2022 ; Accepted: July 17th, 2022 ; Published: July 28th, 2022 ; Correspondence: [email protected]; [email protected] a result of military operations on the territory of Ukraine, sown areas are reduced, the cost of plant protection products and fertilizers increases which emphasizes the problem of obtaining maximum yields from a smaller area of farmland. Given that a shortage of food grains can cause a global food crisis, research on the use of MSW as an environmentally friendly substitute for agrochemicals is relevant today. The aim of the research was to assess the ecotoxicological properties of MSW as an environmentally friendly substitute for synthetic agrochemicals. The impact of MSW as a fertilizer on soil chemical properties and assessment of MSW phytotoxicity as an herbicide for weeds and productivity of winter wheat were studied under field conditions. Toxicological assessment of MSW under laboratory conditions was carried out according to the following parameters: acute oral toxicity and resorptive-toxic effect of MSW. As a result of the assessment of MSW impact on soil chemical properties, it was found that significant soil acidification occurs only when MSW dose of more than 2,400 L ha-1 is used. The content of nitrates and oil products did not increase and there was no soil salinity when the MSW was used in doses of 300–1,200 L ha-1 . It was determined that the greatest decrease in weed plant biomass (85.5%) was observed when 100% concentration of MSW was used in a dose of 350 L ha-1 . As a consequence, with reduced weed infestation, there was a 21.5% increase in winter wheat yield if 100% MSW was used and a 19.1% increase if 75% MSW was used. As a result of the toxicological assessment of MSW, it was found that it belongs to low-toxic compounds. These results of ecotoxicological investigation of MSW make it possible to assert that its use is safe in agriculture, in particular as an environmentally safe organomineral fertilizer and herbicide

70. Meningiomas treated in Greatpoland Cancer Center between 1990–1997

IntroductionWe analyzed correlation between age of patient with anaplastic meningiomas, extension of tumor excision, histopatological recognition and time to recurrence and survival.Material and methodsBetween 1990–1997 7 patients with anaplastic meningioma, 3 patients with haemangiopericytoma, 2 patients with sarcoma meningeum (6 women and 6 men) have been irradiated. 7 patients underwent radical excision of the tumor, 5 patients non radical. The patients were irradiated from limited fields to total dose 56–60 Gy/T mostly by energy Co-60 (9 patients) and photons 9 MV (3 patients).ResultsThere are 6 patients with anaplasticum meningioma still alive. 3 patients living 96–108 months, 3 other 30–39 months. Recurrence was confirmed in two male participants who underwent radical surgery in 12 and 29 month from the start of treatment. The first patient died after 16 months with recurrence of the disease. One patient (39 years old) with heamangiopericytoma lives 40 months after radical surgery without evidence of recurrence. Two patients died – one 11 months after radical surgery (41 years old) and the other one (42 years old) 21 months after non radical surgery. Both patients (24 and 59 years old) with sarcoma died (one after 8 months, and the other one after 21 months).ConclusionsPatient with anaplastic meningiomas have long survival. The extension of tumor excision didn’t influence on survival

Large halloween asteroid at lunar distance

The near-Earth asteroid (NEA) 2015 TB had a very close encounter with Earth at 1.3 lunar distances on October 31, 2015. We obtained 3-band mid-infrared observations of this asteroid with the ESO VLT-VISIR instrument covering approximately four hours in total. We also monitored the visual lightcurve during the close-encounter phase. The NEA has a (most likely) rotation period of 2.939 ± 0.005 h and the visual lightcurve shows a peak-to-peak amplitude of approximately 0.12 ± 0.02 mag. A second rotation period of 4.779 ± 0.012 h, with an amplitude of the Fourier fit of 0.10 ± 0.02 mag, also seems compatible with the available lightcurve measurements. We estimate a V-R colour of 0.56 ± 0.05 mag from different entries in the MPC database. A reliable determination of the object's absolute magnitude was not possible. Applying different phase relations to the available R-/V-band observations produced H = 18.6 mag (standard H-G calculations) or H = 19.2 mag and H = 19.8 mag (via the H-G procedure for sparse and low-quality data), with large uncertainties of approximately 1 mag. We performed a detailed thermophysical model analysis by using spherical and partially also ellipsoidal shape models. The thermal properties are best explained by an equator-on (± 30°) viewing geometry during our measurements with a thermal inertia in the range 250-700 J m s K (retrograde rotation) or above 500 J m s K (prograde rotation). We find that the NEA has a minimum size of approximately 625 m, a maximum size of just below 700 m, and a slightly elongated shape with a/b 1.1. The best match to all thermal measurements is found for: (i) thermal inertia Γ = 900 J m s K; D = 644 m, p = 5.5% (prograde rotation with 2.939 h); regolith grain sizes of 50-100 mm; (ii) thermal inertia Γ = 400 J m s K; D = 667 m, p = 5.1% (retrograde rotation with 2.939 h); regolith grain sizes of 10-20 mm. A near-Earth asteroid model (NEATM) confirms an object size well above 600 m (best NEATM solution at 690 m, beaming parameter η = 1.95), significantly larger than early estimates based on radar measurements. In general, a high-quality physical and thermal characterisation of a close-encounter object from two-week apparition data is not easily possible. We give recommendations for improved observing strategies for similar events in the future. © ESO, 2017.The research leading to these results has received funding from the European Union's Horizon 2020 Research and Innovation Programme, under Grant Agreement No. 687378. Funding from Spanish grant AYA-2014-56637-C2-1-P is acknowledged. Hungarian funding from the NKFIH grant GINOP-2.3.2-15-2016-00003 is also acknowledged. R.D. acknowledges the support of MINECO for his Ramon y Cajal Contract.Peer Reviewe

Evaluating the usability of a visual feature modeling notation

International audienceFeature modeling is a popular Software Product Line Engineering (SPLE) technique used to describe variability in a product family. A usable feature modeling tool environment should enable SPLE practitioners to produce good quality models, in particular, models that effectively communicate modeled information. FAMILIAR is a text-based environment for manipulating and composing Feature Models (FMs). In this paper we present extensions we made to FAMILIAR to enhance its usability. The extensions include a visualization of FMs, or more precisely , a feature diagram rendering mechanism that supports the use of a combination of text and graphics to describe FMs, their configurations, and the results of FM analyses. We also present the results of a preliminary evaluation of the environment's usability. The evaluation involves comparing the use of the extended environment with the previous text-based console-driven version. The preliminary experiment provides some evidence that use of the new environment results in increased cognitive effectiveness of novice users and improved quality of new FMs

70 Wyniki leczenia chorych na raka sutka w stadium rozsiewu w materiale Wielkopolskiego Centrum Onkologii

WstępLeczenie chorych na raka sutka w stadium rozsiewu (M1) ma charakter paliatywny. Metody leczenia obejmują radioterapię, chemioterapię, hormonoterapię w monoterapii lub jako leczenie skojarzone. Wyniki leczenia są najczęściej złe. Przedstawiamy wyniki leczenia chorych na raka sutka w stadium rozsiewu leczonych w Wielkopolskim Centrum Onkologii.Materiał i metody95 chorych na raka sutka w stadium M1 leczono w latach 1983–1987 w Wielkopolskim Centrum Onkologii. Wiek chorych wahał się od 29 do 74 lat, średnio 51,5 lat. W grupie 65 chorych pierwszym umiejscowieniem przerzutów był kościec, w dalszej kolejności płuca i wątroba. Większość chorych leczona była cytostatykami lub hormonami, u części zastosowano paliatywną radioterapię. Wyniki leczenia opracowano na podstawie historii chorób i przeprowadzonej katamnezie. Grupę badaną poddano 5-letniej obserwacji.Wyniki8 chorych (8,4%) przeżyło 5 lat od momentu rozpoczęcia leczenia zmian przerzutowych. Średni okres przeżycia w całej grupie wyniósł 13,5 miesiąca.WnioskiPomimo złego rokowania leczeniem systemowym udaje się przedłużyć życie części chorych na raka sutka, u których wystąpiły przerzuty odległe

Thermal properties of large main-belt asteroids observed by Herschel PACS

Non-resolved thermal infrared observations enable studies of thermal and physical properties of asteroid surfaces provided the shape and rotational properties of the target are well determined via thermo-physical models. We used calibration-programme Herschel PACS data (70, 100, 160 $\mu$m) and state-of-the-art shape models derived from adaptive-optics observations and/or optical light curves to constrain for the first time the thermal inertia of twelve large main-belt asteroids. We also modelled previously well-characterised targets such as (1) Ceres or (4) Vesta as they constitute important benchmarks. Using the scale as a free parameter, most targets required a re-scaling $\sim$5\% consistent with what would be expected given the absolute calibration error bars. This constitutes a good cross-validation of the scaled shape models, although some targets required larger re-scaling to reproduce the IR data. We obtained low thermal inertias typical of large main belt asteroids studied before, which continues to give support to the notion that these surfaces are covered by fine-grained insulating regolith. Although the wavelengths at which PACS observed are longwards of the emission peak for main-belt asteroids, they proved to be extremely valuable to constrain size and thermal inertia and not too sensitive to surface roughness. Finally, we also propose a graphical approach to help examine how different values of the exponent used for scaling the thermal inertia as a function of heliocentric distance (i.e. temperature) affect our interpretation of the results.Comment: Accepted for publication in Astronomy & Astrophysics (preprint version