cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
АНАЛИЗ РАЗВИТИЯ МАГНИТНЫХ БУРЬ, ИНИЦИИРОВАННЫХ РАЗЛИЧНЫМИ СТРУКТУРАМИ СОЛНЕЧНОГО ВЕТРА
Creators: name: Дремухина, Л.А.
name: Ермолаев, Ю.И.
name: Лодкина, И.Г.
Publisher: name: Кольский научный центр Российской академии наук
Year: 2019

description: В работе анализируются характеристики главных фаз магнитных бурь, индуцированных различными типами солнечного ветра (СВ), и их связь с электрическим полем СВ Ey=-V∙Bz. На основании каталога идентифицированных крупномасштабных типов СВ (ftp://ftp.iki.rssi.ru/pub/omni/) и базы данных OMNIза 1995-2016 гг. было отобрано 230 изолированных магнитных бурь и их межпланетные источники: выбросы корональной массы ICME, включающие магнитные облака MCи поршни Ejecta, области компрессии перед ICMESheathи области взаимодействия разно-скоростных потоков СВ CIR. Из-за небольшой статистики не проводилось разделение на Sheathперед MCи SheathпередEjecta, а также учет наличия или отсутствия ударной волны перед драйверами. Проведенный корреляционный анализ показал, что минимальные значения индекса Dstmin(максимальная интенсивность бури) тесно коррелируют (cкоэффициентами корреляции > 0.6) со средними за период главной фазы значениями поля Eyдля всех типов бурь, однако для Sheath-и CIR-индуцированных бурь эта связь наиболее сильная. Тесная корреляция между Dstminи интегралом Eyза период главной фазы характерна для CIR-, Sheath-и Ejecta-бурь, в то время как для MC-бурь она практически отсутствует (коэффициент корреляции < 0.5). Корреляционная связь между средней скоростью развития бури на главной фазе |ΔDst|/ΔTи средними значениями Eyсильна для бурь, вызванных CIRи Sheath, ослабевает для MC, и практически отсутствует (коэффициент корреляции <0.6) для Ejecta-индуцированных бурь. Полученные результаты указывают на тенденцию зависимости развития магнитной бури (ее интенсивности и скорости роста) от типа ее межпланетного источника.
Additional file 2 of Will fire-smart landscape management buffer the effects of climate and land-use changes on fire regimes?
Creators: name: Sil, Ângelo
name: Azevedo, João C.
name: Fernandes, Paulo M.
name: Honrado, João P.
Publisher: name: figshare
Year: 2024
Subjects: Space Science
Medicine
Environmental Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Cancer
Science Policy
Computational Biology

description: Supplementary Material 2.
Mean-field electrostatics beyond the point-charge description
Creators: name: Frydel, Derek
Publisher: name: arXiv
Year: 2014
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: This review explores the number of mean-field constructions for ions whose structure goes beyond the point-charge description, a representation used in the standard Poisson-Boltzmann equation. The exploration is motivated by a body of experimental work which indicates that ion-specific effects play a significant role, where ions of the same valence charge but different size, polarizability, or shape yield quite different, and sometimes surprising results. Furthermore, there are many large ions encountered in soft-matter and biophysics that do not fit into a point-charge description, and their extension in space and shape must be taken into account of any reasonable representation.
title: Η εξέλιξη του λιανικού εμπορίου στην Ελλάδα εν μέσω της πανδημίας του Covid-19 και του ψηφιακού μετασχηματισμού
title: The evolution of the retail sector in Greece during the pandemic of Covid-19 and the digital transformation
titleType: AlternativeTitle
Creators: name: Κοιλάκου, Μαρία-Άννα
Publisher: name: Πανεπιστήμιο Δυτικής Αττικής
Year: 2022
Subjects: Λιανικό εμπόριο
Μικρομεσαίες επιχειρήσεις
Covid-19
Digital Economy and Society Index
DESI
Ελλάδα
Ευρωπαϊκή Ένωση
Εξέλιξη
Ιστορική αναδρομή

description: Πρωτογενής έρευνα / Ποιοτική έρευνα σε Key Persons του κλάδου του λιανικού εμπορίου
description: Η ζωή και η καθημερινότητα των ανθρώπων έχει αλλάξει. Ο τρόπος που επικοινωνούμε, ο τρόπος που εργαζόμαστε, ο τρόπος που κάνουμε αγορές έχει επηρεαστεί άμεσα από τις ψηφιακές τεχνολογίες που χρόνο με τον χρόνο αλλάζουν και εξελίσσονται. Κατά την περίοδο της πανδημίας του Covid-19 η στροφή προς την ψηφιοποίηση έπαιξε κρίσιμο ρόλο και δημιουργήθηκε έντονα η ανάγκη για επέκταση της χρήσης των τεχνολογικών επιτευγμάτων. Το λιανικό εμπόριο είναι από εκείνους τους κλάδους που επηρεάστηκε σημαντικά και που ανέδειξε την ανάγκη για μετασχηματισμό. Η παρούσα μελέτη εξετάζει το κατά πόσον ο κλάδος του εμπορίου στην Ελλάδα και ειδικά η μικρομεσαία επιχείρηση είναι έτοιμη να δεχθεί τον ψηφιακό μετασχηματισμό και τι απαιτείται τελικά για την επίτευξή του. Όλα τα παραπάνω συνδέονται άρρηκτα και με τους στόχους που έχει θέσει η Ευρωπαϊκή Επιτροπή, οι οποίοι τοποθετούνται χρονικά έως το 2030. Μια από τις βασικότερες προτάσεις στρατηγικής της Ευρωπαϊκής Επιτροπής είναι η «Ψηφιακή Πυξίδα: 20301». Στο πλαίσιο αυτό εξετάζουμε ως εξαρτημένη μεταβλητή το κατά πόσον μια μικρομεσαία επιχείρηση στην Ελλάδα, που δραστηριοποιείται στο λιανικό εμπόριο, μπορεί να προσαρμοστεί και να επιβιώσει στις νέες συνθήκες, τη στιγμή μάλιστα που η Ελλάδα φαίνεται να καθυστερεί να εξελιχθεί σε σχέση με άλλες χώρες, ενώ ως επεξηγηματικές μεταβλητές, που παίζουν πολύ σημαντικό ρόλο για την προσέγγιση του θέματος, είναι οι υποδομές, ο ψηφιακός αναλφαβητισμός – τα skills που έχει το προσωπικό μιας επιχείρησης/ο ιδιοκτήτης. Τέλος, η εμπιστοσύνη που φαίνεται να δείχνει ο επιχειρηματικός κόσμος στο κράτος και στους Ευρωπαϊκούς θεσμούς και φυσικά οι ρυθμοί με τους οποίους φαίνεται να εξελίσσεται το λιανικό εμπόριο στην χώρα μέσα στα χρόνια. Μεθοδολογικά, θα πραγματοποιηθεί αρχικά βιβλιογραφική επισκόπηση με βάση την οποία θα καταλήξουμε σε κάποιες υποθέσεις. Στη συνέχεια θα γίνει πρωτογενής έρευνα με την μορφή μη δομημένων συνεντεύξεων, έτσι ώστε τα πιθανά αποτελέσματα από την περιγραφική ανάλυση να απαντήσουν στο βασικό ερώτημα: Τελικά κατά πόσον η μικρομεσαία επιχείρηση στην Ελλάδα είναι έτοιμη να προσαρμοστεί στις νέες συνθήκες και πως θα καταφέρει να επιβιώσει εν όψει των αλλαγών που επέρχονται;
Accretion and ejection in black-hole X-ray transients
Creators: name: Kylafis, N. D.
name: Belloni, T. M.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Aims: We summarize the current observational picture of the outbursts of black-hole X-ray transients (BHTs), based on the evolution traced in a hardness-luminosity diagram (HLD), and we offer a physical interpretation. Methods: The basic ingredient in our interpretation is the Poynting-Robertson Cosmic Battery (PRCB, Contopoulos & Kazanas 1998), which provides locally the poloidal magnetic field needed for the ejection of the jet. In addition, we make two assumptions, easily justifiable. The first is that the mass-accretion rate to the black hole in a BHT outburst has a generic bell-shaped form. This is guaranteed by the observational fact that all BHTs start their outburst and end it at the quiescent state. The second assumption is that at low accretion rates the accretion flow is geometrically thick, ADAF-like, while at high accretion rates it is geometrically thin. Results: Both, at the beginning and the end of an outburst, the PRCB establishes a strong poloidal magnetic field in the ADAF-like part of the accretion flow, and this explains naturally why a jet is always present in the right part of the HLD. In the left part of the HLD, the accretion flow is in the form of a thin disk, and such a disk cannot sustain a strong poloidal magnetic filed. Thus, no jet is expected in this part of the HLD. The counterclockwise traversal of the HLD is explained as follows: the poloidal magnetic field in the ADAF forces the flow to remain ADAF and the source to move upwards in the HLD rather than to turn left. Thus, the history of the system determines the counterclockwise traversal of the HLD. As a result, no BHT is expected to ever traverse the entire HLD curve in the clockwise direction. Conclusions: We offer a physical interpretation of accretion and ejection in BHTs with only one parameter, the mass transfer rate.
description: Accepted for publication in A&A
HOOP D8.3 Guidance for the organisation of National Replication Workshops
Creators: name: Lisai, Serena
name: Bel, Jean-Benoit
Publisher: name: Zenodo
Year: 2021

description: The HOOP project aims to unlock bio-based investments and deploy local bio economies in Europe through a systemic and cross-cutting approach. It will offer project development assistance to a group of 8 Lighthouse Cities and Regions (from now on Lighthouses) to build the technical, economic, financial and legal expertise needed to develop concrete investments to valorise biowaste and wastewater, with the aim of obtaining safe and sustainable bio-based products.

This report is one of the outputs of the HOOP project and it aims at guiding the Lighthouses involved in the in the organisation of National Replication Workshops (NRW). Each lighthouse is in charge of organising at least one NRW over the course of the project to promote the replication of the HOOP findings to other cities and regions at national level, and push forward innovative solutions for local bioeconomy strategies. This how-to guide will be a tool to inspire methodologies and activities for the organisation of NRW, yet Lighthouses will be given flexibility to make it relevant and effective. Transforming an idea in reality is the goal of the HOOP project and the NRW represents a key element to demonstrate how local bioeconomy concept can be turned into actual projects.

The first part of this report is a short introduction about the HOOP project and the National Replication Workshops, the goals to achieve and how they should be inserted in the project activities. Then, a how-to guide is provided to define step-by-step the elements that should be considered in advance for the organisation of such an event. The guide provides suggestions and inspirations to organise the workshops keeping in mind that the approach chosen needs to be adapted to the national context. Therefore, this guide is more a source of inspiration listing various possibilities and approaches that can be then selected to make the most of the event. The guide can be adapted and replicated in every context and sector.

The report also contains a ready-to-use toolkit as annexes: a checklist of the activities to implement, with a reference to the time, the people to involve and the status.
ГЕЛИОГЕОФИЗИЧЕСКИЕ ФАКТОРЫ, ВЛИЯНИЕ КОТОРЫХ МОГЛО ОБУСЛОВИТЬ ОШИБКИ В РАБОТЕ GPSВ ПЕРИОД ВОЕННЫХ УЧЕНИЙ НАТО «TRIDENTJUNCTURE» С 25/10/2018 ПО 7/11/2018
Creators: name: Козелов, Б.В.
name: Черноус, С.А.
name: Шагимуратов, И.И.
name: Филатов, М.В.
name: Ефишов, И.И.
name: Тепеницина, Н.Ю.
name: Федоренко, Ю.В.
name: Пильгаев, С.В.
Publisher: name: Кольский научный центр Российской академии наук
Year: 2019

description: Крупнейшие маневры НАТО со времен холодной войны под кодовым названием «Трайдент юнктер» (United Trident) проводились на территории Евроарктики с 25 октября по 7 ноября 2018 года. Солдаты из 32 стран принимали участие в маневрах на территории Норвегии, в Балтийском море и Северной Атлантике. Как сообщали различные источники, во время учений были отмечены нарушения работы Глобальной системы позиционирования (GPS). В этой работе мы представляем, какой отклик эти события нашли в официальной прессе Финляндии, Норвегии, Швеции и России. Даем объяснение почему эти сбои могли быть вызваны непредсказуемыми естественными гелиогеофизическими факторами. Для анализа были использованы данные полученные сети GPS в западной части Арктики и субарктической зоне отНью-Олесунна до Апатитов и Калининграда. Проводим оценку отклонений позиционирования во время учений.
Fusion of O16 + Ca40 at Elab(16O)=13.4 MeV/nucleon
Creators: name: Wang, T.F.
name: Prosser, F.W.
name: Beck, C.
name: Vineyard, M.F.
name: Kovar, D.G.
name: Ma, W.C.
name: Henderson, D.J.
name: Janssens, R.V.F.
name: Maguire, C.F.
name: Wilkins, B.D.
name: Rosner, G.
name: Sanders, S.J.
Publisher: name: American Physical Society
Year: 1989

description: Mass and velocity distributions have been measured for the evaporation residue and fusion-fission products from the O16+40Ca reaction at 214 MeV. Comparisons of Monte Carlo statistical evaporation simulations to the observed angle and mass dependences of the evaporation-residue velocity distributions were used to set limits on the maximum complete-fusion cross section and to extract information about the magnitude and character of incomplete-fusion processes. The extracted value of the complete fusion evaporation-residue cross section is discussed in the framework of previous results and existing models.
Additional file 1 of Annelid methylomes reveal ancestral developmental and aging-associated epigenetic erosion across Bilateria
Creators: name: Guynes, Kero
name: Sarre, Luke A.
name: Carrillo-Baltodano, Allan M.
name: Davies, Billie E.
name: Xu, Lan
name: Liang, Yan
name: Martín-Zamora, Francisco M.
name: Hurd, Paul J.
name: de Mendoza, Alex
name: Martín-Durán, José M.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Supplementary Figures. Figures S1 to S19.
title: Ο ρόλος των μέσων κοινωνικής δικτύωσης στη διαμόρφωση της αξίας της επωνυμίας (brand) εταιρειών
title: Brand equity and the role of social media
titleType: AlternativeTitle
Creators: name: Ατσάρος, Λάμπρος
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2022
Subjects: subject: Brand equity
subject: Βranding
subject: Social media
subject: Communication
subject: Μέσα κοινωνικής δικτύωσης

description: Η παρούσα εργασία πραγματεύεται την έννοια του Brand Equity και τον ρόλο που αναλαμβάνουν τα μέσα κοινωνικής δικτύωσης στη προώθηση της αξίας της σύγχρονης επιχείρησης. Θα γίνει αναφορά στους παράγοντες που διαμορφώνουν το Brand Equity ανάλογα με τα χαρακτηριστικά της επιχείρησης, των προϊόντων και της αγοράς. Επιπλέον θα γίνει ανάλυση σε βάθος στους τρόπους που μια επωνυμία μπορεί να εκσυγχρονιστεί με τα δεδομένα που διαρκώς αλλάζουν και εξελίσσονται. Ακόμη θα γίνει σύνδεση της στρατηγικής που ακολουθεί η επιχείρηση με σκοπό να περιλαμβάνει το Brand Equity και πως αυτά συνδέονται με την εισαγωγή καινοτομίας, της επικοινωνίας εντός και εκτός της επιχείρησης, την αναγνωσιμότητα και την αξία της. Στη συνέχεια θα γίνει μελέτη των μέσων κοινωνικής δικτύωσης που είναι διαθέσιμα στο χώρο του διαδικτύου για να αξιοποιηθούν από τις επιχειρήσεις με τον καλύτερο δυνατό τρόπο και ποια τα οφέλη και οι αδυναμίες που συνδέονται με τη χρήση αυτών των μέσων. Τέλος θα γίνει ανάλυση της περίπτωσης της αλυσίδας καταστημάτων καφέ Starbucks και του τρόπου που αυτή επωφελείται και εκμεταλλεύεται προς όφελός της τα διαθέσιμα διαδικτυακά μέσα επικοινωνίας.
Review of Some Promising Fractional Physical Models
Creators: name: Tarasov, Vasily E.
Publisher: name: arXiv
Year: 2015
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Fractional dynamics is a field of study in physics and mechanics investigating the behavior of objects and systems that are characterized by power-law non-locality, power-law long-term memory or fractal properties by using integrations and differentiation of non-integer orders, i.e., by methods of the fractional calculus. This paper is a review of physical models that look very promising for future development of fractional dynamics. We suggest a short introduction to fractional calculus as a theory of integration and differentiation of non-integer order. Some applications of integro-differentiations of fractional orders in physics are discussed. Models of discrete systems with memory, lattice with long-range inter-particle interaction, dynamics of fractal media are presented. Quantum analogs of fractional derivatives and model of open nano-system systems with memory are also discussed.
description: 38 pages, LaTeX
G factor of the 59/2 - isomer in Gd147
Creators: name: Dafni, E.
name: Wolfs, F.H.L.
name: Janssens, R.V.F.
name: Moore, E.F.
name: Khoo, T.L.
name: Beard, K.
name: Garg, U.
name: Benczer-Koller, N.
name: Piiparinen, M.
name: Ahmad, I.
name: Hass, M.
name: Körner, H.J.
name: Daly, P.J.
Publisher: name: American Physical Society
Year: 1989

description: The g factor of the 10 995 keV, Je=(59/2-, and T1/2=0.8 ns level in Gd147 has been determined by the transient field method for ions recoiling through a magnetized Gd foil at a temperature of 100 K. The Ge76(76Ge,5n)147Gd reaction at E(76Ge)=310 MeV was used to provide high recoil velocity. A 100 ps flight time in vacuum between the target and the ferromagnet of 100 ps ensured that the -ray cascades fed the (59/2 level before the recoil ions traversed the Gd foil. The g factor was extracted from standard double ratios with the known parametrization of the transient field, yielding g=0.38(7). This value is in agreement with the predicted wave function and experimental single-particle moments in this mass region. Results for levels in 146,148Gd were also obtained.
Photometric brown-dwarf classification. I. A method to identify and accurately classify large samples of brown dwarfs without spectroscopy
Creators: name: Skrzypek, Nathalie
name: Warren, Stephen J.
name: Faherty, Jacqueline K.
name: Mortlock, Daniel J.
name: Burgasser, Adam J.
name: Hewett, Paul C.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims. We present a method, named photo-type, to identify and accurately classify L and T dwarfs onto the standard spectral classification system using photometry alone. This enables the creation of large and deep homogeneous samples of these objects efficiently, without the need for spectroscopy. Methods. We created a catalogue of point sources with photometry in 8 bands, ranging from 0.75 to 4.6 microns, selected from an area of 3344 deg^2, by combining SDSS, UKIDSS LAS, and WISE data. Sources with 13.0 < J < 17.5, and Y - J > 0.8, were then classified by comparison against template colours of quasars, stars, and brown dwarfs. The L and T templates, spectral types L0 to T8, were created by identifying previously known sources with spectroscopic classifications, and fitting polynomial relations between colour and spectral type. Results. Of the 192 known L and T dwarfs with reliable photometry in the surveyed area and magnitude range, 189 are recovered by our selection and classification method. We have quantified the accuracy of the classification method both externally, with spectroscopy, and internally, by creating synthetic catalogues and accounting for the uncertainties. We find that, brighter than J = 17.5, photo-type classifications are accurate to one spectral sub-type, and are therefore competitive with spectroscopic classifications. The resultant catalogue of 1157 L and T dwarfs will be presented in a companion paper.
description: 15 pages, 12 figures, Accepted for publication in A & A
Towards DIB mapping in galaxies beyond 100 Mpc. A radial profile of the $λ$5780.5 diffuse interstellar band in AM 1353-272 B
Creators: name: Monreal-Ibero, Ana
name: Weilbacher, Peter M.
name: Wendt, Martin
name: Selman, Fernando
name: Lallement, Rosine
name: Brinchmann, Jarle
name: Kamann, Sebastian
name: Sandin, Christer
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Diffuse Interstellar Bands (DIBs) are non-stellar weak absorption features of unknown origin found in the spectra of stars viewed through one or several clouds of Interstellar Medium (ISM). Research of DIBs outside the Milky Way is currently very limited. Specifically spatially resolved investigations of DIBs outside of the Local Group is, to our knowledge, inexistent. Here, we explore the capability of the high sensitivity Integral Field Spectrograph, MUSE, as a tool to map diffuse interstellar bands at distances larger than 100 Mpc. We use MUSE commissioning data for AM 1353-272 B, the member with highest extinction of the "The Dentist's Chair", an interacting system of two spiral galaxies. High signal-to-noise spectra were created by co-adding the signal of many spatial elements distributed in a geometry of concentric elliptical half-rings. We derived decreasing radial profiles for the equivalent width of the $λ$5780.5 DIB both in the receding and approaching side of the companion galaxy up to distances of $\sim$4.6 kpc from the center of the galaxy. Likewise, interstellar extinction, as derived from the Halpha/Hbeta line ratio displays a similar trend, with decreasing values towards the external parts. This translates into an intrinsic correlation between the strength of the DIB and the extinction within AM 1353-272 B consistent with the current existing global trend between these quantities when using measurements for both Galactic and extragalactic sight lines. Mapping of DIB strength in the Local Universe as up to now only done for the Milky Way seems feasible. This offers a new approach to study the relationship between DIBs and other characteristics and species of the ISM in different conditions as those found in our Galaxy to the use of galaxies in the Local Group and/or single sightlines towards supernovae, quasars and galaxies outside the Local Group.
description: 4 pages, 4 figures, accepted for publication as a Letter in Astronomy and Astrophysics; Received 10 February 2015 / Accepted 20 February 2015 ; English corrections included
Additional file 2 of Annelid methylomes reveal ancestral developmental and aging-associated epigenetic erosion across Bilateria
Creators: name: Guynes, Kero
name: Sarre, Luke A.
name: Carrillo-Baltodano, Allan M.
name: Davies, Billie E.
name: Xu, Lan
name: Liang, Yan
name: Martín-Zamora, Francisco M.
name: Hurd, Paul J.
name: de Mendoza, Alex
name: Martín-Durán, José M.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Supplementary Tables.
PERFORMANCE EVALUATION OF MAINTENANCE IN A MANUFACTURING INDUSTRY
Creators: name: Onyejaka, Chidi Maurice
name: Prof. Ike, Oluka
Publisher: name: SADI Journals
Year: 2023
Subjects: Evaluation
Maintenance
Manufacturing Industry
Performance

description: The performance evaluation of maintenance practices in a manufacturing industry (Nigerian bottling company Benin Plant) was carried out. This was a retrospective study on the performance evaluation of maintenance in a manufacturing industry. Records on maintenance of filler machine was collected for a period of five years from 2017-2021 using a questionnaire. This questionnaire was designed to capture the cumulative end of the year production and maintenance parameters/data for the industry which includes; year of manufacture of equipment, year of installation, types of maintenance done on the machine, total hours of failure for the year, year product target, year actual volume of product produced and the quantity of defective product etc. The machine was obtained and installed in 2008, the world class OEE (Overall Equipment Effectiveness) mathematical model was used to evaluate the maintenance performance. The availability rate ranged from 93.0% - 96.9%, Performance rate ranged from 66.2% - 129.3% while the quality rate was 99.9% for all the years. The approaches used for the maintenance of the filler machine in this manufacturing company were preventive and usage-based approaches. The availability rate, performance rate and quality rate where high however performance rate was lower in the year 2020.
ЭКСТРЕМАЛЬНЫЕ ВЕЛИЧИНЫ ГЕОИНДУКТИРОВАННЫХ ТОКОВ В РЕГИОНАЛЬНОЙ ЭНЕРГОСИСТЕМЕ
Creators: name: Сахаров, Я.А.
name: Селиванов, В.Н.
name: Билин, В.А.
name: Николаев, В.Г.
Publisher: name: Кольский научный центр Российской академии наук
Year: 2019

description: Более десяти лет ведется непрерывная регистрация геоиндуктированных токов (ГИТ) на подстанциях магистральных электрических сетей на Северо-Западе России. Анализ амплитудных значений ГИТ в узлах энергосистемы позволяет на фоне относительно гладких закономерностей выделить случаи с максимальными амплитудами токов, экстремальные события. С точки зрения обеспечения стабильной работыэлектрической сети именно эти, экстремальные события, могут оказаться наиболее опасными. В работе рассмотрены случаи развития геоиндуктированных токов максимальных амплитуд в узлах магистральной линии электропередачи «Северный транзит» при различных геомагнитных возмущениях. Обсуждается связь событий ГИТ с условиями, влияющими на генерациютоков в энергосистеме, а именно величиной геомагнитного возмущения, скоростью изменения горизонтальной компоненты геомагнитного поля, параметрами и расположением линий электропередачи.
Role of p-induced population of medium mass(A $\sim$ 150) neutron rich nuclei
Creators: name: Banerjee, D.
name: Saha, A.
name: Bhattacharjee, T.
name: Guin, R.
name: Das, S. K.
name: Das, P.
name: Pandit, Deepak
name: Mukherjee, A.
name: Chowdhury, A.
name: Bhattacharya, Soumik
name: Gupta, S. Das
name: Bhattacharyya, S.
name: Mukhopadhyay, P.
name: Banerjee, S. R.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Excitation functions were measured by stacked-foil activation technique for the $^{150}$Nd(p, xpyn) reaction using 97.65$%$ enriched $^{150}$Nd target. Measurement up to $\sim$50$%$ above barrier and down to 18$%$ below the barrier was performed using proton beam energy (E$_p$) of 7 - 15 MeV from VECC Cyclotron. The yield of suitable $γ$ rays emitted following the decay of relevant evaporation residues was determined using a 50$%$ High Purity Germanium (HPGe) detector.(p,n) cross section was found to follow the expected trend with a maximum value of 63.7(4.9)mb at E$_p$ $\sim$ 8.6 MeV. (p,2n) cross section gradually increased with E$_p$ and had maximum contribution to the total reaction cross section after E$_p$ $\sim$ 9.0 MeV. (p, p$^{\prime}$n) reaction channel also showed a reasonable yield with a threshold of E$_p$ $\sim$ 12.0 MeV. The experimental data were corroborated with statistical model calculations using different codes, viz., CASCADE, ALICE/91 and EMPIRE3.1. All the calculations using a suitable set of global parameters could reproduce the excitation function fairly well in the present energy range.
External UV Environments and Photoevaporating Protoplanetary Disks: Most Common UV Environment of Stellar Nurseries in the Solar Neighborhood - NGC 1977
Creators: name: Kim, Jinyoung Serena
name: Hartman, Peter
name: Haworth, Thomas
name: Fang, Min
name: Facchini, Stefano
name: Pascucci, Ilaria
name: Heo, Jeong-Eun
Publisher: name: Zenodo
Year: 2023
Subjects: Protoplanetary Disk
External Photoevaporation
Star and Planet Formation
Star Forming Environment

description: Abstract External UV environments play a crucial role in star and planet formation and protoplanetary disk evolution. We discuss ranges of diverse UV environments for star forming regions, then focus on an intermediate UV environment (~3000 G0, where G0~1-2 for the local ISM FUV flux). We present up-to-date census and kinematic studies of photoevaporating protoplanetary disks (proplyds) in an intermediate radiation environment NGC 1977 in the Orion A cloud. Proplyds provide direct evidence of interplay between protoplanetary disks and UV radiation from massive O, B stars. These are excellent laboratories to study the effects radiation environment plays on planet forming disks. Theorists suggest that an intermediate UV environment such as in NGC 1977 is the most “common” star forming environment in the solar neighborhood. NGC 1977 is a sibling of the Orion Nebula Cluster (ONC) in Orion A cloud which has similar ages (1-2 Myr) as young stars in ONC. However, NGC 1977 provide a different star forming environment compared to ONC. NGC 1977 harbors the weakest UV environment to date, where proplyds have been identified around a B1V star, 42 Or. It harbors the second most number of known proplyds, after ONC, where 100s of proplyds have been found around a O6 star. Latest discovery of new proplyds in NGC 2024 covers more embedded and younger star forming region around B0.5 and O9 stars. To date, most known proplyd nurseries (NGC 1977, NGC 2024, ONC) are found in Orion Star Forming Regions. We show preliminary results from the latest spectroscopic observations, which are being analyzed to estimate accretion activity, winds, and jets for three proplyds in NGC 1977. We also used Gaia DR3 data and SDSS/APOGEE-2 radial velocity data to study kinematics of proplyds and YSOs to address lifetime problem of proplyds. In NGC 1977, YSOs and proplyds show similar proper motions, while the proper motion of 42 Ori (B1V) is different from the rest of YSOs suggesting that the ionizing source responsible for external photoevaporation of these proplyds could form more proplyds in the future. We also present that there are extremely low mass proplyds down to a giant planetary mass objects.
description: {"references": ["Baraffe I. et al. (2015), A&A, 577, 6", "Fang, M., Kim, J. S., Pascucci, I. et al. (2016), ApJ, 833, L16", "Fang, M. , Kim, J. S., Pascucci, I. et al. (2017), AJ, 153, 188.", "Hasegawa, Y. et al. (2022), ApJL, 926, L23", "Kim, J. S., Clarke, C., Fang, M. et al. (2016), ApJL, 826, L15", "Haworth. T, J. , Kim, Winter et al. (2022), MNRAS, 512,2,2594", "Winter, A. & Haworth, T., J. (2022), EPJP, 137, 1132 https://arxiv.org/abs/2206.11910"]}
ON THE CORRELATION BETWEEN LUNAR CRUSTAL MAGNETIC FIELDS AND THE SOLAR WIND ION REFLECTION MAP
Creators: name: Belyaev, R.
name: Divin, A.
name: Semenov, V.
name: Kubyshkin, I.
name: Zaytsev, I.
name: Deca, J.
Publisher: name: Кольский научный центр Российской академии наук
Year: 2019

description: The Moon does not have a global magnetic field. However, the lunar crust contains regions of remanent magnetization which are strong enough to deflect and reflect a substantial part of the incoming solar wind ions.Such effects as lunar swirls, limb shocks, minimagnetospheres, low-frequency waves are the global processes induced by the local magnetic fields. In this work we investigate the correlation between local magnetic field data provided by the Tsunakawa model [2015], and the total particle reflectionfunction estimated by Lueet al.[2011]. We find a spatial correlation coefficient between those two up to ~0.7 for the magnetic field model value at 20 km. It was found that an increase in the field leads to a significant increase in reflection and this dependence of the field on the reflection coefficient has a clear nonlinear form, which is consistent with numerical simulation results that show more intense scattering for stronger magnetic anomalies. For low magnetic field regions (<30 nT), the value ofreflection coefficient is ~10-4...10-3which corresponds to direct scattering by the Lunar surface.
Additional file 3 of Annelid methylomes reveal ancestral developmental and aging-associated epigenetic erosion across Bilateria
Creators: name: Guynes, Kero
name: Sarre, Luke A.
name: Carrillo-Baltodano, Allan M.
name: Davies, Billie E.
name: Xu, Lan
name: Liang, Yan
name: Martín-Zamora, Francisco M.
name: Hurd, Paul J.
name: de Mendoza, Alex
name: Martín-Durán, José M.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3. Review history.
Additional file 1 of Identifying complex patients in family medicine for potential benefit from a case manager: a short questionnaire derived from the INTERMED Self-Assessment (IMSA) questionnaire
Creators: name: Cohidon, Christine
name: Gallay, Emilie
name: Wild, Pascal
name: Stiefel, Friedrich
name: Bourquin, Céline
name: Senn, Nicolas
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Supplementary Material 1 - The IMSA questionnaire.
Stability of Hartmann flow with the convective approximation
Creators: name: Kalashnikov, I. Yu.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: This research is focused on linear analysis of a plane-parallel flow stability in a transverse magnetic field (Hartmann flow) within a convective approximation. We derive and solve equations describing the perturbation growth. Perturbation modes and their nonexcitation conditions have been determined. An equation for the instability increment has been derived and it is shown that the equation has an unstable root. Additionally, we show that the resulting instabilities qualitatively agree with the experimental data.
Lifetime measurements of terminating and collective high-spin states in 155DY and 156DY
Creators: name: Ahmad, I.
name: Janssens, R.V.F.
name: Khoo, T.L.
name: Trzaska, W.H.
name: Grabowski, Z.W.
name: Daly, P.J.
name: Dichter, B.K.
name: Quader, M.A.
name: Garg, U.
name: Holzmann, R.
name: Ma, W.C.
name: Piiparinen, M.
name: Ragnarsson, I.
name: Drigert, M.
name: Emling, H.
Publisher: name: Elsevier
Year: 1989

description: Lifetime measurements for the isotopes 155Dy and 156Dy have been extended up to spins around 40h{stroke} by the Doppler shift attenuation method in conjunction with γ-γ-coincidence measurements. Results have been obtained for the yrast band in 156Dy and for three bands in 155Dy. Strong retardations of the E2-strengt were observed for intruding terminating sequences, for which specific single particle configurations are suggested.
Bottomonium in the plasma: lattice results
Creators: name: Aarts, G.
name: Allton, C.
name: Evans, W.
name: Giudice, P.
name: Harris, T.
name: Kelly, A.
name: Kim, S.
name: Lombardo, M. P.
name: Ryan, S.
name: Skullerud, J-I
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present results on the heavy quarkonium spectrum and spectral functions obtained by performing large-scale simulations of QCD for temperatures ranging from about 100 to 500 MeV, in the same range as those explored by LHC experiments. We discuss our method and perspectives for further improvements towards the goal of full control over the many systematic uncertainties of these studies.
description: 8 pages, proceedings of QCD@Work 2014, International Workshop on Quantum Chromodynamics Theory and Experiment Giovinazzo, Bari, Italy, June 16-19, 2014
Additional file 1 of Combinatorial targeting of menin and the histone methyltransferase DOT1L as a novel therapeutic strategy for treatment of chemotherapy-resistant ovarian cancer
Creators: name: Alexandrova, Elena
name: Lamberti, Jessica
name: Memoli, Domenico
name: Quercia, Claudia
name: Melone, Viola
name: Rizzo, Francesca
name: Tarallo, Roberta
name: Giurato, Giorgio
name: Nassa, Giovanni
name: Weisz, Alessandro
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Supplementary Material 1: Figure S1. Impact of menin silencing on proliferation of OC cells. (A) RT-qPCR, (left panel) and western blot (right panel) of MEN1 mRNA and menin expression levels, respectively, in Caov-3, OVCAR-3, PEO1, PEO14 and PEO4 cells. Error bars represent the mean of replicate values ± SD (* p ≤ 0.05). Changes of MEN1 mRNA relative abundance (B), menin protein expression (C) and cell proliferation (D) determined by RT-qPCR, western blot and MTT assay, respectively, in Caov-3 (left), OVCAR-3 (middle) and PEO14 (right) cells 96 hours post transfection with three siRNAs targeting different regions of the MEN1 mRNA. Scramble siRNA (CTRL) was used as the negative control. Error bars represent the mean of replicate values ± SD (* p ≤ 0.05). Figure S2. Validation of menin silencing effects on OC cells. (A) Correlation coefficient between differentially expressed genes following menin silencing obtained from independent experiments performed with two different sequencing approaches. Graph showing differentially expressed genes belonging to Aryl Hydrocarbon receptor (B), Integrin (C) Cyclins and Cell cycle regulation (D) signaling pathways obtained from independent experiments performed with MGI and Illumina sequencing approaches. The dashed orange line marks the Fold change threshold (|FC| ≥ Q1, padj ≤ 0.05). Figure S3. The effects of menin pharmacological inhibition on OC cells proliferation. Caov-3 (left), OVCAR-3 (middle) and PEO14 (right) relative cell viability assessed in cells treated with increasing concentrations of MI-136. Data represent the mean of six independent replicates ± SD (* p ≤ 0.05). Figure S4. The effects of menin pharmacological inhibition on OC cells proliferation. Caov-3, OVCAR-3, PEO1, PEO14, PEO4 relative cell viability assessed in cells treated with increasing concentrations of MI-136. Data represent the mean of six independent replicates ± SD (* p ≤ 0.05). Figure S5. Menin associates with DOT1L in nucleus of OC cells. Immunoprecipitation-western blot showing the presence of DOT1L among proteins, co-precipitated altogether with menin from PEO4 nuclear extracts. IgG was used as negative control. Figure S6. D-R Lowe graph showing the effects of combinatorial treatment with increasing MI-136 and EPZ5676 concentrations on PEO1 (left) and PEO4 (right) cells proliferation after twelve days of treatment
Hagedorn's Hadron Mass Spectrum and the Onset of Deconfinement
Creators: name: Gazdzicki, Marek
name: Gorenstein, Mark I.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A brief history of the observation of the onset of deconfinement - the beginning of the creation of quark gluon plasma in nucleus-nucleus collisions with increasing collision energy - is presented. It starts with the measurement of hadron mass spectrum and the Hagedorn's hypothesis of the limiting temperature of hadronic matter (the Hagedorn temperature). Then the conjecture that the Hagedorn temperature is the phase transition temperature was formulated with the crucial Hagedorn participation. It was confirmed by the observation of the onset of deconfinement in lead-lead collisions at the CERN SPS energies.
description: arXiv admin note: substantial text overlap with arXiv:1201.0485
Metabolic syndrome: a psychiatric outlook
Creators: name: SIDDIQUI, JAVED ATHER
name: QURESHI, SHAZIA FARHEEN
Publisher: name: figshare
Year: 2023
Subjects: Clinical psychology

description: A metabolic syndrome is a cluster of clinical signs that are risk factors for the development of type 2 diabetes mellitus, and cardiovascular disease. This cluster includes obesity, elevated blood sugar, high blood pressure, and high cholesterol. Atypical antipsychotics that are associated with a group of signs and symptoms have resulted in an increased focus on this syndrome. This review included accessible literature, such as review articles and original research articles. It provides useful guidelines for psychiatrists and gives them psycho-education so that they can identify and monitor patients who may have the syndrome and properly manage it.
A new permutation test statistic for complete block designs
Creators: name: Samonenko, Inga
name: Robinson, John
Publisher: name: arXiv
Year: 2014
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics

description: We introduce a nonparametric test statistic for the permutation test in complete block designs. We find the region in which the statistic exists and consider particularly its properties on the boundary of the region. Further, we prove that saddlepoint approximations for tail probabilities can be obtained inside the interior of this region. Finally, numerical examples are given showing that both accuracy and power of the new statistic improves on these properties of the classical $F$-statistic under some non-Gaussian models and equals them for the Gaussian case.
description: Published in at http://dx.doi.org/10.1214/14-AOS1266 the Annals of Statistics (http://www.imstat.org/aos/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Cooking with DAOSPEC
Creators: name: Pancino, Elena
name: Peter B., Stetson
Publisher: name: Zenodo
Year: 2008

description: DAOSPEC is a Fortran program written by Peter B. Stetson at the Dominion Astrophysical Observatory (DAO) of the Herzberg Insti- tute of Astrophysics, National Reasearch Council, in Victoria, Canada in 2008. DAOSPEC automatically finds absorption lines in stellar spectra, fits the continuum, measures equivalent widths and identifies lines with the help of a laboratory linelist, and also provides a radial velocity es- timate. DAOSPEC is designed to work on extracted, one-dimensional spectra that have been binned linearly in wavelength, either in FITS or in IRAF (.imh, .pix) format. This cookbook describes how to obtain, install, configure and use DAOSPEC. This new version includes per- formance considerations and a list of common problems and solutions based on feedback from the users. The software is still widely used today and this manual has not been officially published before.
Ni64 +92Zr fission yields at energies close to the Coulomb barrier
Creators: name: Sanders, S.J.
name: Wolfs, F.L.H.
name: Janssens, R.V.F.
name: Ma, W.C.
name: Holzmann, R.
name: Khoo, T.L.
Publisher: name: American Physical Society
Year: 1989

description: Fission yields for the Zr64 reaction at laboratory energies between 240 and 300 MeV have been measured. Elastic scattering angular distributions were also obtained and used to deduce the generalized total reaction cross sections. The competition between fission and light-particle evaporation from the compound nucleus is well reproduced by statistical-model calculations. However, the calculated neutron multiplicities for this reaction are larger than those previously measured. Possible reasons for this discrepancy are discussed.
MPEC 2024-R262 : 2009 SL2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Nuclear-structure dependence of heavy-ion-fusion partial-wave distributions
Creators: name: Schwalm, D.
name: Janssens, R.V.F.
name: Kuehn, W.
name: Fischer, R.D.
name: Hennrich, H.J.
name: Khoo, T.L.
name: Breitbach, G.
name: Ruckelshausen, A.
name: Metag, V.
name: Simon, R.S.
name: Novotny, R.
name: Habs, D.
name: Haas, B.
Publisher: name: American Physical Society
Year: 1989

description: Partial-wave cross sections for fusion of Zr64 and Zr64 at energies of 5% and 7% above the Bass-model fusion barrier have been measured with the Darmstadt-Heidelberg Crystal Ball. The distribution for fusion with the more neutron-deficient target Zr92 exhausts the unitarity limit for lower angular momenta. In contrast, fusion with the slightly more neutron-rich target Zr96 yields a broad angular momentum distribution with cross sections well below unitarity even for small partial waves.
Additional file 4 of Combinatorial targeting of menin and the histone methyltransferase DOT1L as a novel therapeutic strategy for treatment of chemotherapy-resistant ovarian cancer
Creators: name: Alexandrova, Elena
name: Lamberti, Jessica
name: Memoli, Domenico
name: Quercia, Claudia
name: Melone, Viola
name: Rizzo, Francesca
name: Tarallo, Roberta
name: Giurato, Giorgio
name: Nassa, Giovanni
name: Weisz, Alessandro
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Supplementary Material 4
Homoclinic orbit and hidden attractor in the Lorenz-like system describing the fluid convection motion in the rotating cavity
Creators: name: Leonov, G. A.
name: Kuznetsov, N. V.
name: Mokaev, T. N.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: In this paper a Lorenz-like system, describing the process of rotating fluid convection, is considered. The present work demonstrates numerically that this system, also like the classical Lorenz system, possesses a homoclinic trajectory and a chaotic self-excited attractor. However, for considered system, unlike the classical Lorenz one, along with self-excited attractor a hidden attractor can be localized. Analytical-numerical localization of hidden attractor is presented.
Additional file 1 of A novel and dual digestive symbiosis scales up the nutrition and immune system of the holobiont Rimicaris exoculata
Creators: name: Aubé, Johanne
name: Cambon-Bonavita, Marie-Anne
name: Velo-Suárez, Lourdes
name: Cueff-Gauchard, Valérie
name: Lesongeur, Françoise
name: Guéganton, Marion
name: Durand, Lucile
name: Reveillaud, Julie
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Supplementary Figure 1. PhyloFlash heatmap of taxonomic assignments (rows, with prokaryotes in blue and eukaryotes in red) for small-subunit rRNA reads in the six individual foregut and midgut metagenomes (columns). The intensity of colors indicates the percentage of reads that mapped to a given taxon. Metagenomes are clustered by their similarity in terms of taxonomic profile and taxa are clustered by their co-occurrence across metagenomes. The Euclidean distance and the Ward's minimum variance method were used for clustering.
Additional file 1 of Multi-locus imprinting disturbance (MLID): interim joint statement for clinical and molecular diagnosis
Creators: name: Mackay, Deborah J. G.
name: Gazdagh, Gabriella
name: Monk, David
name: Brioude, Frederic
name: Giabicani, Eloise
name: Krzyzewska, Izabela M.
name: Kalish, Jennifer M.
name: Maas, Saskia M.
name: Kagami, Masayo
name: Beygo, Jasmin
name: Kahre, Tiina
name: Tenorio-Castano, Jair
name: Ambrozaitytė, Laima
name: Burnytė, Birutė
name: Cerrato, Flavia
name: Davies, Justin H.
name: Ferrero, Giovanni Battista
name: Fjodorova, Olga
name: Manero-Azua, Africa
name: Pereda, Arrate
name: Russo, Silvia
name: Tannorella, Pierpaola
name: Temple, Karen I.
name: Õunap, Katrin
name: Riccio, Andrea
name: de Nanclares, Guiomar Perez
name: Maher, Eamonn R.
name: Lapunzina, Pablo
name: Netchine, Irène
name: Eggermann, Thomas
name: Bliek, Jet
name: Tümer, Zeynep
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1.
The general peakon-antipeakon solution for the Camassa-Holm equation
Creators: name: Grunert, Katrin
name: Holden, Helge
Publisher: name: arXiv
Year: 2015
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35Q53, 35B35, 35Q20

description: We compute explicitly the peakon-antipeakon solution of the Camassa-Holm equation $u_t-u_{txx}+3uu_x-2u_xu_{xx}-uu_{xxx}=0$ in the non-symmetric and $α$-dissipative case. The solution experiences wave breaking in finite time, and the explicit solution illuminates the interplay between the various variables.
description: 23 pages, 5 figures