Zobrazeno 1 - 10
of 2 520
pro vyhledávání: '"A, Rakhmanova"'
Autor:
Yermolaev, Yuri I., Lodkina, Irina G., Khokhlachev, Alexander A., Yermolaev, Michael Yu., Riazantseva, Maria O., Rakhmanova, Liudmila S., Borodkova, Natalia L., Sapunova, Olga V., Moskaleva, Anastasiia V.
Solar activity and solar wind parameters decreased significantly in solar cycles (SCs) 23-24. In this paper, we analyze solar wind measurements at the rising phase of SC 25 and compare them with similar data from the previous cycles. For this purpose
Externí odkaz:
http://arxiv.org/abs/2304.14707
Publikováno v:
Solar-Terrestrial Physics, Vol 10, Iss 2, Pp 13-25 (2024)
Magnetosheath is a transition layer between the solar wind and the magnetosphere and may contribute to the geoeffectiveness of various large-scale interplanetary phenomena. In this paper, we examine the dynamics of the turbulent fluctuation spectra b
Externí odkaz:
https://doaj.org/article/4bb6fe7f0d0945dba0f0b09ee502dc3c
Autor:
Tuganova, Regina, Permyakova, Anna, Kuznetsova, Anna, Rakhmanova, Karina, Monzul, Natalia, Uvarov, Roman, Kovtun, Elizaveta, Budennyy, Semen
Green technology is viewed as a means of creating a sustainable society and a catalyst for sustainable development by the global community. It is responsible for both the potential reduction of production waste and the reduction of carbon footprint a
Externí odkaz:
http://arxiv.org/abs/2210.09611
Autor:
Yermolaev, Yuri I., Lodkina, Irina G., Khokhlachev, Alexander A., Yermolaev, Michael Yu., Riazantseva, Maria O., Rakhmanova, Liudmila S., Borodkova, Natalia L., Sapunova, Olga V., Moskaleva, Anastasiia V.
Publikováno v:
Universe. 2022; 8(9):472
In solar cycles 23-24, solar activity noticeably decreased, and, as a result, solar wind parameters decreased. Based on the measurements of the OMNI base for the period 1976-2019, the time profiles of the main solar wind parameters and magnetospheric
Externí odkaz:
http://arxiv.org/abs/2208.04849
Autor:
Liudmila Rakhmanova, Alexander Khokhlachev, Maria Riazantseva, Yuri Yermolaev, Georgy Zastenker
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
Turbulent solar wind is known to be a main driver of the processes inside the magnetosphere, including geomagnetic storms and substorms. Experimental studies of the last decade demonstrate additional ways of interplanetary plasma transport to the mag
Externí odkaz:
https://doaj.org/article/8340f4149bde42129bf1b8182cde1098
Autor:
Kostyukov, Anton I., Kostyukova, Nadezhda Y., Nashivochnikov, Aleksandr A., Rakhmanova, Mariana I., Suprun, Evgenii A.
Publikováno v:
In Optical Materials November 2024 157 Part 1
Publikováno v:
In Journal of Luminescence November 2024 275
Autor:
Omelchenko, A.N., Okotrub, K.A., Igonina, T.N., Rakhmanova, T.A., Okotrub, S.V., Rozhkova, I.N., Kozeneva, V.S., Amstislavsky, S.Ya., Surovtsev, N.V.
Publikováno v:
In Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy 15 January 2025 325
Autor:
Yermolaev Y. I., Lodkina I. G., Khokhlachev A. A., Yermolaev M. Y., Riazantseva M. O., Rakhmanova L. S., Borodkova N. L., Sapunova O. V., Moskaleva A. V.
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 4, Pp 55-62 (2023)
Solar activity and solar wind parameters decreased significantly in solar cycles (SCs) 23–24. In this paper, we analyze solar wind measurements at the rising phase of SC 25 and compare them with similar data from the previous cycles. For this purpo
Externí odkaz:
https://doaj.org/article/046253339960425ebc0973672abf12b1
Autor:
Rakhmanova, Liudmila1 rakhlud@gmail.com, Khokhlachev, Alexander1, Riazantseva, Maria1, Yermolaev, Yuri1, Zastenker, Georgy1, Alexandrova, Olga, Safrankova, Jana
Publikováno v:
Frontiers in Astronomy & Space Sciences. 2024, p1-15. 15p.