Media education and the formation of the legal culture of society

The development of legal culture and a culture of human rights in the modern world through media technologies, is acquiring special significance in connection with the processes of globalization and the spread of media in recent decades. The purpose of the article is to study the prospects for the use of media education in the formation of the legal social culture and a culture of human rights. © 2020 LLC Ecological Help. All rights reserved.The reported study was funded by RFBR, project number 20-013-00813 “Educational potential of the media sphere as a space for the development of legal culture and human rights culture in modern Russia”

О качестве контента блогов в контексте формирования правовой культуры

Introduction. The relevance of the study is caused by the development of digital technologies, their increasingly active influence on all aspects of society and human life and, consequently, the need of forming the individual's legal culture using the media sphere's resources. The purpose of the study is to analyze the main characteristics and quality of legal Instagram blog content as one of the dynamically developing applications with a multi-million audience of users. Materials and research methods. The research methodology consists of an integrative approach. Information and target analysis of texts and discourse analysis were used to interpret blog content in the context of specific cultural and historical factors. The results of the study and the discussion. The Top Instagram bloggers was compiled using the hashtag #lawyer, blog content studied. Based on the development of quality content criteria - relevance, social significance, completeness, accessibility, practice orientation, personalization, infoesthetics, multi-factor, literacy, and subscriber response-were developed, according to which the analysis of legal content was carried out. The study identified the content of bloggers who position themselves on Instagram as legal experts, analyzed the content of bloggers with more than ten thousand subscribers based on the developed quality criteria. It is identified that high-quality content causes an adequate reaction of users, contains a knowledge component endowed with legal content and aimed at improving the legal culture of the individual Conclusions. Despite the fact that Instagram, like other apps, has more entertainment content, however, users feel the need for knowledges that will let them to constructively solve situation in the legal sphere. It was revealed that high-quality content as socially significant knowledge has an adequate response of Instagram users. This contributes to the development of the individual's legal culture in the context of socio-cultural transformations, when a modern person increasingly has to solve non-standard objectives in a dynamically developing environment, including changes in the legal framework in various fields of activity. © 2020 LLC Ecological Help. All rights reserved.The reported study was funded by RFBR, project number 20-013-00813 "Educational potential of the media sphere as a space for the development of legal culture and human rights culture in modern Russia"

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VIII: The Eighth Year (2015-2016)

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 128 SU UMa-type dwarf novae observed mainly during the 2015-2016 season and characterized these objects. The data have improved the distribution of orbital periods, the relation between the orbital period and the variation of superhumps, the relation between period variations and the rebrightening type in WZ Sge-type objects. Coupled with new measurements of mass ratios using growing stages of superhumps, we now have a clearer and statistically greatly improved evolutionary path near the terminal stage of evolution of cataclysmic variables. Three objects (V452 Cas, KK Tel, ASASSN-15cl) appear to have slowly growing superhumps, which is proposed to reflect the slow growth of the 3:1 resonance near the stability border. ASASSN-15sl, ASASSN-15ux, SDSS J074859.55+312512.6 and CRTS J200331.3-284941 are newly identified eclipsing SU UMa-type (or WZ Sge-type) dwarf novae. ASASSN-15cy has a short (~0.050 d) superhump period and appears to belong to EI Psc-type objects with compact secondaries having an evolved core. ASASSN-15gn, ASASSN-15hn, ASASSN-15kh and ASASSN-16bu are candidate period bouncers with superhump periods longer than 0.06 d. We have newly obtained superhump periods for 79 objects and 13 orbital periods, including periods from early superhumps. In order that the future observations will be more astrophysically beneficial and rewarding to observers, we propose guidelines how to organize observations of various superoutbursts.Comment: 123 pages, 162 figures, 119 tables, accepted for publication in PASJ (including supplementary information

Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. the seventh year (2014-2015)

© The Author 2015. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved. Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 102 SU UMa-type dwarf novae, observed mainly during the 2014-2015 season, and characterized these objects. Our project has greatly improved the statistics of the distribution of orbital periods, which is a good approximation of the distribution of cataclysmic variables at the terminal evolutionary stage, and has confirmed the presence of a period minimum at a period of 0.053 d and a period spike just above this period. The number density monotonically decreased toward the longer period and there was no strong indication of a period gap. We detected possible negative superhumps in Z Cha. It is possible that normal outbursts are also suppressed by the presence of a disk tilt in this system. There was no indication of enhanced orbital humps just preceding the superoutburst, and this result favors the thermal-tidal disk instability as the origin of superoutbursts. We detected superhumps in three AM CVn-type dwarf novae. Our observations and recent other detections suggest that 8% of objects showing dwarf nova-type outbursts are AM CVn-type objects. AM CVn-type objects and EI Psc-type objects may be more abundant than previously recognized. OT J213806, a WZ Sge-type object, exhibited remarkably different features between the 2010 and 2014 superoutbursts. Although the 2014 superoutburst was much fainter, the plateau phase was shorter than the 2010 one, and the course of the rebrightening phase was similar. This object indicates that the O - C diagrams of superhumps can indeed be variable, at least in WZ Sge-type objects. Four deeply eclipsing SU UMa-type dwarf novae (ASASSN-13cx, ASASSN-14ag, ASASSN-15bu, and NSV 4618) were identified. We studied long-term trends in supercycles in MM Hya and CY UMa and found systematic variations of supercycles of ∼20%

Class I methanol masers in low-mass star formation regions

We present a review of the properties of Class I methanol masers detected in low-mass star forming regions (LMSFRs). These masers, henceforth called LMMIs, are associated with postshock gas in the lobes of chemically active outflows in LMSFRs NGC1333, NGC2023, HH25, and L1157. LMMIs share the main properties with powerful masers in regions of massive star formation and are a low-luminosity edge of the total Class I maser population. However, the exploration of just these objects may push forward the exploration of Class I masers, since many LMSFRs are located only 200-300 pc from the Sun, making it possible to study associated objects in detail. EVLA observations with a 0.2″ spatial resolution show that the maser images consist of unresolved or barely resolved spots with brightness temperatures up to 5 7 105 K. The results are marginally consistent with the turbulent model of maser emission

EFFICIENCY OF PREVENTION AND MANAGEMENT OF VITAMIN D DEFICIENCY IN YOUNG CHILDREN IN RUSSIA DEPENDING ON THE REGION OF RESIDENCE (BASED ON THE RESULTS OF RODNICHOK-2 STUDY)

Medical examination of 360 children from four regions of Russia (Moscow, Astrakhan, Stavropol, Kazan) showed significant regional differences in the sufficiency and compensation of vitamin D deficiency at the baseline (Day 0) and established factors associated with vitamin D sufficiency on Day 0. The established interregional differences in vitamin D levels were not due to insolation, but primarily to adequate vitamin D supplementation received at the baseline. Vitamin D supplementation (an average of 894 ± 632.6 IU/day) significantly reduced the risk of vitamin D deficiency (RR 0.15, 95% CI 0.09–0.26, P = 5.7 x 10–14). The study included the analysis of factors associated with the increase in 25(OH)D levels during the administration of Aquadetrim, identification of predictors of patient’s response and the analysis of identified predictors. The most important factor determining the patient’s response was the dose of vitamin D taken by the patient: 25(OH)D levels increased by 1 ng/ml with an increase in the dose of vitamin D by 90 IU per day. As can be seen from the above, the study results indicate that the vitamin D deficiency requires a long-term preventive therapy (for at least several months) with adequate doses of vitamin D (1000–2000 IU/day)