Identification of Saturn Lightnings Recorded by the UTR-2 Radio Telescope and Cassini Spacecraft

Identification of Saturn Lightnings Recorded by the UTR-2 Radio Telescope and Cassini Spacecraft

The Saturn electrostatic discharges (SED) simultaneously recorded in the initial period of storm F at the UTR-2 radio telescope and Cassini spacecraft are investigated. The UTR-2 used the FFT-spectral receiver operating 12÷33 MHz, while the Cassini the serial spectrum analyser RPWS (Radio Plasma Wav...

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Bibliographic Details
Date:2012
Main Authors: Zakharenko, V. V., Mylostna, K. Y., Fischer, G., Konovalenko, O. O., Zarka, P., Grießmeier, J.–M., Ryabov, B. P., Vavriv, D. M., Ryabov, V. B., Rucker, H. O., Ravier, P., Sidorchuk, M. A., Cecconi, B., Coffre, A., Denis, L., Fabrice, C., Kozhyn, R. V., Mukha, D. V., Pallier, L., Schneider, J., Shevchenko, V. A., Vynogradov, V. V., Weber, R., Nikolaenko, V. S.
Format: Article
Language:Russian
Published: Видавничий дім «Академперіодика» 2012
Online Access:http://rpra-journal.org.ua/index.php/ra/article/view/458
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Journal Title:Radio physics and radio astronomy

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Radio physics and radio astronomy
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Summary:The Saturn electrostatic discharges (SED) simultaneously recorded in the initial period of storm F at the UTR-2 radio telescope and Cassini spacecraft are investigated. The UTR-2 used the FFT-spectral receiver operating 12÷33 MHz, while the Cassini the serial spectrum analyser RPWS (Radio Plasma Wave Science) operating 1.8÷16 MHz. The ground and space data processed have shown very good agreement. E-folding time of SED and its dependence on episode intensity in the initial period of storm F were determined.

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