Zobrazeno 1 - 10
of 53
pro vyhledávání: '"solar emission"'
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
Publikováno v:
In Nuclear and Particle Physics Proceedings October-November 2017 291-293:36-39
Publikováno v:
Atmosphere, Vol 6, Iss 1, Pp 50-59 (2014)
The electromagnetic power that arrives from the Sun in the C-band has been used to check the quality of the polarimetric, Doppler weather radar network that has recently been installed in Switzerland. The operational monitoring of this network is bas
Externí odkaz:
https://doaj.org/article/214e60ca2e494ba7bb074496cf6bd8ab
Publikováno v:
Atmosphere, Vol 7, Iss 6, p 76 (2016)
The electromagnetic power that comes from the Sun has been proved to be an effective reference for checking the quality of dual-polarization weather radar receiver. Operational monitoring methods have been developed and implemented for determining th
Externí odkaz:
https://doaj.org/article/acecb562b6514d5f8534d65821d87316
Publikováno v:
Nuclear and Particle Physics Proceedings. :36-39
The high energy gamma-ray emission from the Sun is due to the interactions of cosmic ray (CR) protons and electrons with matter and photons in the solar environment. Such interactions lead to two component gamma-ray emission: a disk-like emission due
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eaaa199a5772c608a93510df0ae64da6
https://doi.org/10.1016/j.nuclphysbps.2017.06.008
https://doi.org/10.1016/j.nuclphysbps.2017.06.008
Autor:
Andreas Leuenberger, Marco Gabella
Publikováno v:
Sensors (Basel, Switzerland)
The radio noise that comes from the Sun has been reported in literature as a reference signal to check the quality of dual-polarization weather radar receivers for the S-band and C-band. In most cases, the focus was on relative calibration: horizonta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4aa0b7df8e83820948557bd4b7c1693d
https://pubmed.ncbi.nlm.nih.gov/28531164
https://pubmed.ncbi.nlm.nih.gov/28531164
Publikováno v:
Atmosphere, Vol 6, Iss 1, Pp 50-59 (2014)
The electromagnetic power that arrives from the Sun in the C-band has been used to check the quality of the polarimetric, Doppler weather radar network that has recently been installed in Switzerland. The operational monitoring of this network is bas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ac0c9fbe7030f8a8e017b3863f3d136
https://doi.org/10.3390/atmos6010050
https://doi.org/10.3390/atmos6010050
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer
In this paper we present the high resolution spectral observations of the fragment of lunar surface during the total lunar eclipse of December 10, 2011. The observations were carried out with the fiber-fed echelle spectrograph at 1.2-m telescope in K
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0deb7611e8a94bdccb7fb2c936408b25
https://doi.org/10.1016/j.jqsrt.2012.11.013
https://doi.org/10.1016/j.jqsrt.2012.11.013
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