267 research outputs found
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
Constitutional mutations of cancer susceptibility genes in the health workers professionally exposed to cytostatic drugs
Applying the product lines paradigm to the quantitative analysis of collective adaptive systems
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 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 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
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