66 citations · 157 across the 7 of their papers we have counts for
7 papers
Radio signature of a distant behind-the-limb CME on 2017 September 6
V. N. Melnik, H. O. Rucker, A. I. Brazhenko +5
We discuss properties of a Type IV burst, which was observed on 2017 September 6, as a result of the powerful flare X 9.3. At decameter wavelengths this burst was observed by the r…
Digital receivers for low-frequency radio telescopes UTR-2, URAN, GURT
V. Zakharenko, A. Konovalenko, P. Zarka +49
This paper describes digital radio astronomical receivers used for decameter and meter wavelength observations. This paper describes digital radio astronomical receivers used for d…
Beaming structures of Jupiter's decametric common S-bursts observed from LWA1, NDA, and URAN2 radio telescopes
Masafumi Imai, Alain Lecacheux, Tracy E. Clarke +7
On 2015 February 21, simultaneous observations of Jupiter's decametric radio emission between 10 and 33 MHz were carried out using three powerful low-frequency radio telescopes: Lo…
Fine and superfine structure of Decameter-Hectometer type II burst on 2011 June 7
V. V. Dorovskyy, V. N. Melnik, A. A. Konovalenko +4
The characteristics of the type II bursts with herringbone structure observed both by ground based radio telescopes (UTR-2, URAN-2) and spaceborn spectrometers (STEREO A-B) are dis…
In-flight calibration of STEREO-B/WAVES antenna system
M. Panchenko, W. Macher, H. O. Rucker +4
The STEREO/WAVES (SWAVES) experiment on board the two STEREO spacecraft (Solar Terrestrial Relations Observatory) launched on 25 October 2006 is dedicated to the measurement of the…
Radio seismology of the outer solar corona
T. V. Zaqarashvili, V. N. Melnik, A. I. Brazhenko +5
Observed oscillations of coronal loops in EUV lines have been successfully used to estimate plasma parameters in the inner corona (< 0.2 R_0, where R_0 is the solar radius). Howeve…
XUV exposed, non-hydrostatic hydrogen-rich upper atmospheres of terrestrial planets II: Hydrogen coronae and ion escape
K. G. Kislyakova, H. Lammer, M. Holmström +8
We study the interactions between the stellar wind plasma flow of a typical M star, such as GJ 436, and hydrogen-rich upper atmospheres of an Earth-like planet and a "super-Earth"…