Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Dorota Przepiórka"'
Autor:
Marcin Grzesiak, Mariusz Pożoga, Barbara Matyjasiak, Dorota Przepiórka, Katarzyna Beser, Lukasz Tomasik, Hanna Rothkaehl, Helena Ciechowska
Publikováno v:
Remote Sensing, Vol 14, Iss 18, p 4655 (2022)
We try to assess the validity of assumptions taken when deriving drift velocity. We give simple formulas for characteristics of the spatiotemporal correlation function of the observed diffraction pattern for the frozen flow and the more general Brigg
Externí odkaz:
https://doaj.org/article/052e3f259cbf44cb90ad73bba5e39c46
The Earth's ionosphere is a coupled system affected by interactions with precipitating energetic particles and electrical currents from the Earth's magnetosphere, and in addition by upward propagating disturbances from lower atmospheric layers. Geoma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a0f4045f32c944138554f9ac75453c4f
https://doi.org/10.5194/egusphere-egu22-12910
https://doi.org/10.5194/egusphere-egu22-12910
Publikováno v:
2021 Signal Processing Symposium (SPSympo).
We take the frozen-in assumption of the scatter evolution and derive simple formulas for characteristics of the spatiotemporal correlation function of the observed diffraction pattern. Using Low-Frequency Array (LOFAR) Cassiopeia intensity observatio
Autor:
Barbara Atamaniuk, Hanna Rothkaehl, Mariusz Pozoga, Katarzyna Budzińska, Marcin Grzesiak, Dorota Przepiórka, Barbara Matyjasiak
Scintillation of beacon satellite signals or distant cosmic radio emissions can provide interesting information on the cosmic medium itself, its internal spatial structure and basic evolution characteristics. LOFAR network gives consistent scintillat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::13fcdad38bd98a64295f3595ccf59783
https://doi.org/10.5194/egusphere-egu21-6582
https://doi.org/10.5194/egusphere-egu21-6582
Mid-latitude trough (MIT) is the distinct structure observed in Earth’s ionosphere at high latitudes especially at the nighttimes. The phenomenon is observed at both hemispheres. As it resides at the topside ionosphere in the sub-auroral region, it
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ded5c5c122f77411020f4504031ff560
https://doi.org/10.5194/egusphere-egu2020-18228
https://doi.org/10.5194/egusphere-egu2020-18228
The sub-auroral region of the main ionospheric trough is a very unique area strongly affected by different type of instabilities coming from both the bottom (Earth's atmosphere) and the top (Earth's magnetosphere) neighbouring regions. The main ionos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::67a428cb401fe235a9b5a423239ed089
https://doi.org/10.5194/egusphere-egu2020-8427
https://doi.org/10.5194/egusphere-egu2020-8427
Autor:
Dorota Przepiórka, Agata Chuchra, Hanna Rothkaehl, Barbara Matyjasiak, Michał Marek, Roman Schreiber
The Earth’s auroral region and its close neighbourhood is the origin of strong radio emissions caused by complex physical plasma processes. Among them we can list auroral hiss, auroral roar, auroral medium frequency (MF) burst, and auroral kilometr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f4b4506de1c4efbc64fc06c876320c68
https://doi.org/10.5194/egusphere-egu2020-18465
https://doi.org/10.5194/egusphere-egu2020-18465
Autor:
Dorota Przepiórka, Barbara Matyjasiak, Hanna Rothkaehl, C. Y. Chen, Kwangsun Ryu, Loren C. Chang, I. T. Lee, Tiger J.Y. Liu, Koichiro Oyama
Publikováno v:
Journal of Geophysical Research: Space Physics. 123:5917-5932
Publikováno v:
Journal of Geophysical Research: Space Physics. 121:2390-2406
Autor:
Marek Strumik, Dorota Przepiórka, Krzysztof Stasiewicz, H. Karimabadi, Marcin Grzesiak, Vadim Roytershteyn
Publikováno v:
Geophysical Research Letters. 42:5109-5116
We discuss mechanisms of the generation of ultralow frequency (ULF) upstream waves in the terrestrial foreshock that are essential for the acceleration of ions in space plasmas. The analysis is based on global hybrid kinetic simulations of the magnet