Zobrazeno 1 - 10
of 3 405
pro vyhledávání: '"Getman A."'
Publikováno v:
E3S Web of Conferences, Vol 474, p 01053 (2024)
The paper is devoted to study technological properties of low-melting clay. Research methods of clay properties that affect the technology of ceramic brick production are presented. The clay sample under study is an acid clay of montmorillonite miner
Externí odkaz:
https://doaj.org/article/98884d1cc19548809d68ee4a80af897c
Publikováno v:
E3S Web of Conferences, Vol 474, p 01055 (2024)
The aim of this project is to develop the mass composition and the technology for producing high-alumina chamotte with an Al2O3 content of 65–85% based on technogenic raw materials – fine corundum dust formed during grinding of fused corundum. Fi
Externí odkaz:
https://doaj.org/article/d1739538d14b4ae5a561a9fc3c0824b5
Autor:
Getman, Konstantin V., Kochukhov, Oleg, Ninan, Joe P., Feigelson, Eric D., Airapetian, Vladimir S., Waggoner, Abygail R., Cleeves, L. Ilsedore, Forbrich, Jan, Dzib, Sergio A., Law, Charles J., Rab, Christian, Krolikowski, Daniel M.
We explore the empirical power-law relationship between X-ray luminosity (Lx) and total surface magnetic flux (Phi), established across solar magnetic elements, time- and disk-averaged emission from the Sun, older active stars, and pre-main-sequence
Externí odkaz:
http://arxiv.org/abs/2501.01321
Autor:
Getman, Konstantin V., Feigelson, Eric D., Waggoner, Abygail R., Cleeves, L. Ilsedore, Forbrich, Jan, Ninan, Joe P., Kochukhov, Oleg, Airapetian, Vladimir S., Dzib, Sergio A., Law, Charles J., Rab, Christian
The most powerful stellar flares driven by magnetic energy occur during the early pre-main sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares accessible to a single poi
Externí odkaz:
http://arxiv.org/abs/2410.05126
Publikováno v:
Психологическая наука и образование, Vol 25, Iss 6, Pp 77-87 (2020)
The paper presents results of a comparative study of motivation for studying science in Russia and leading countries in science education. We explored the relationship and its strength between various types of motivation and the level of science lite
Externí odkaz:
https://doaj.org/article/3604c38db3234d34af23b2f519d4af4e
Autor:
Getman, Konstantin V., Kóspál, Ágnes, Arulanantham, Nicole, Semenov, Dmitry A., Smirnov-Pinchukov, Grigorii V., van Terwisga, Sierk E.
DQ Tau is a unique young high-eccentricity binary system that exhibits regular magnetic reconnection flares and pulsed accretion near periastron. We conducted NuSTAR, Swift, and Chandra observations during the July 30, 2022 periastron to characterize
Externí odkaz:
http://arxiv.org/abs/2310.12811
Autor:
Ramirez-Tannus, María Claudia, Bik, Arjan, Cuijpers, Lars, Waters, Rens, Goppl, Christiane, Henning, Thomas, Kamp, Inga, Preibisch, Thomas, Getman, Konstantin V., Chaparro, Germán, Cuartas-Restrepo, Pablo, de Koter, Alex, Feigelson, Eric D., Grant, Sierra L., Haworth, Thomas J., Hernández, Sebastián, Kuhn, Michael A., Perotti, Giulia, Povich, Matthew S., Reiter, Megan, Roccatagliata, Veronica, Sabbi, Elena, Tabone, Benoît, Winter, Andrew J., McLeod, Anna F., van Boekel, Roy, van Terwisga, Sierk E.
We present the first results of the eXtreme UV Environments (XUE) James Webb Space Telescope (JWST) program, that focuses on the characterization of planet forming disks in massive star forming regions. These regions are likely representative of the
Externí odkaz:
http://arxiv.org/abs/2310.11074
Large pre-trained models are essential in paralinguistic systems, demonstrating effectiveness in tasks like emotion recognition and stuttering detection. In this paper, we employ large pre-trained models for the ACM Multimedia Computational Paralingu
Externí odkaz:
http://arxiv.org/abs/2310.10179
Autor:
Punyapu, Venkata Rohit, Zhu, Jiazhou, Meza-Morales, Paul, Chaluvadi, Anish, Mefford, O. Thompson, Getman, Rachel B.
A grand challenge in materials research is identifying the relationship between composition and performance. Herein, we explore this relationship for magnetic properties, specifically magnetic saturation (M$_s$) and magnetic anisotropy energy (MAE) o
Externí odkaz:
http://arxiv.org/abs/2309.09754
We study the four-dimensional relationships between magnetic activity, rotation, mass and age for solar-type stars in the age range 5-25Myr. This is the late-pre-main sequence (l-PMS) evolutionary phase when rapid changes in star's interior may lead
Externí odkaz:
http://arxiv.org/abs/2305.09013