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pro vyhledávání: '"Incoherent Scatter Radar"'
Akademický článek
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Publikováno v:
Solar-Terrestrial Physics, Vol 10, Iss 1, Pp 63-67 (2024)
For incoherent scatter measurements, the effective subtraction technique is to alternate the duration of amplitude-modulated signals between a pair of consequently radiated pulses. The resulting gain of spatial resolution enables us to steadily asses
Externí odkaz:
https://doaj.org/article/fc8526faaf51466bb7d811eefc1c7560
Publikováno v:
Earth and Planetary Physics, Vol 8, Iss 2, Pp 408-414 (2024)
During the course of ionospheric heating experiments, researchers at the European Incoherent Scatter Scientific Association (EISCAT) observed an apparent electron density enhancement. The enhancement extended over a wide range of altitudes, above the
Externí odkaz:
https://doaj.org/article/4ed5d000fb3c42788a01f8e02a1b2f05
Publikováno v:
地球与行星物理论评, Vol 55, Iss 1, Pp 66-76 (2024)
Herein, the technical characteristics and programme of Qujing incoherent scatter radar (the first one in China) are described. The measurement ability in the ionosphere, space debris, and the Moon was investigated using the data. The results showed t
Externí odkaz:
https://doaj.org/article/2a86be6fd0e0471abdc423eaa773b591
Autor:
Matvienko, O. V.1,2 matvolegv@mail.ru, Daneyko, O. I.1 olya_dan@mail.ru, Kovalevskaya, T. A.1 takov47@mail.ru
Publikováno v:
Russian Physics Journal. Dec2018, Vol. 61 Issue 8, p1520-1528. 9p.
Publikováno v:
Annales Geophysicae (ANGEO) (09927689). 2018, Vol. 36 Issue 6, p1657-1666. 10p.
Publikováno v:
Earth and Space Science, Vol 11, Iss 4, Pp n/a-n/a (2024)
Abstract Joule heating is one of the main energy inputs into the thermosphere‐ionosphere system. Precise modeling of this process is essential for any space weather application. Existing thermosphere‐ionosphere models tend to underestimate the ac
Externí odkaz:
https://doaj.org/article/7f209b06b7104bbd9dc2d5ab075717c6
Autor:
Setov A. G., Kushnarev D. S.
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 4, Pp 46-54 (2023)
Solar emission in meter waves originates from upper layers of the solar corona. We present absolute measurements of solar flux from Irkutsk Incoherent Scatter Radar (161 MHz frequency) and Learmonth Observatory (245 MHz frequency). We perform correla
Externí odkaz:
https://doaj.org/article/39ed15d99aca474682f0fcfa4b694321