| FOREWORD | 6 |
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| SPONSORS | 8 |
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| CONTENTS | 10 |
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| SATURN’S RADIO EMISSIONS AND THEIR RELATION TO MAGNETOSPHERIC DYNAMICS | 20 |
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| 1 Introduction | 20 |
| 2 Solar Wind Influence on Saturn’sMagnetospheric Radio Emis-sions | 21 |
| 3 Magnetotail Reconnection and Radio Emissions: Terrestrial Review | 22 |
| 4 Magnetotail Reconnection at Saturn and Link to Radio Emis-sions | 24 |
| 5 Conclusion | 27 |
| References | 28 |
| DIRECTION FINDING AND POLARIZATION MEASUREMENTS OF SKR | 32 |
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| 1 Introduction | 32 |
| 2 How the RPWS Instrument Works | 33 |
| 3 Some Already Published DF | 33 |
| 34 | 33 |
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| 4 Improving DF | 33 |
| 35 | 33 |
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| 5 Some Improved Results on SKR | 45 |
| 6 Summary | 51 |
| References | 52 |
| AN OVERVIEW OF THE TIME-DEPENDENT ROTATIONAL MODULATION OF SATURNIAN RADIO EMISSIONS | 56 |
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| VARIABILITY OF SOUTHERN AND NORTHERN SKR PERIODICITIES | 58 |
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| 1 Introduction | 58 |
| 2 Radio Observations and Harmonic Analysis | 59 |
| 3 Variability of SKR Periodicities | 61 |
| 4 Nature of the SKR Diurnal Modulation | 65 |
| 5 Conclusions | 67 |
| References | 67 |
| AN SLS4 LONGITUDE SYSTEM BASED ON A TRACKING FILTER ANALYSIS OF THE ROTATIONAL MODULATION OF SATURN KILOMETRIC RADIATION | 70 |
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| 1 Introduction | 71 |
| 2 SKR Modulation Spectrum | 73 |
| 3 Phase and Longitude Analysis | 77 |
| 4 The SLS4-N and SLS4-S Longitude Systems | 80 |
| 5 Accessing the SLS4 Longitude System | 80 |
| References | 82 |
| IS A RIKITAKE DYNAMO IN SATURN’S INTERIOR AT THE ORIGIN OF THE VARIABILITY OF THE RADIO ROTATION PERIODS? | 84 |
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| 1 Introduction | 84 |
| 2 Particularity of Saturn’s Magnetic Field | 85 |
| 3 Dynamo Effect in Saturn’s Interior | 86 |
| 4 Results and Conclusion | 89 |
| References | 90 |
| SOLAR WIND AND SATURNIAN MOONS SIGNATURES IN THE LONG-PERIODIC MODULATIONS OF SKR | 92 |
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| A CLOSE ENCOUNTER WITH A SATURN KILOMETRIC RADIATION SOURCE REGION | 94 |
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| 1 Introduction | 94 |
| 2 Observations | 95 |
| 3 Discussion | 99 |
| References | 101 |
| SATURN KILOMETRIC RADIATION NEAR A SOURCE CENTER ON DAY 73, 2008 | 106 |
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| 1 Introduction | 106 |
| 2 Instrumentation, Observations, and Analysis | 107 |
| 3 Summary and Conclusions | 112 |
| References | 112 |
| PROPERTIES OF SATURN KILOMETRIC RADIATION MEASURED WITHIN ITS SOURCE REGION | 116 |
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| AN OVERVIEW OF SATURN NARROWBAND RADIO EMISSIONS OBSERVED BY CASSINI RPWS | 118 |
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| 1 Introduction | 119 |
| 2 Source Mechanism | 119 |
| 3 Polarization and Intensity Measurements | 120 |
| 4 Direction Finding Results | 123 |
| 5 Z–mode Narrowband Emissions Below fce | 124 |
| 6 Rotational Modulation | 126 |
| 7 Conclusion | 128 |
| References | 129 |
| SATURNIAN LOW FREQUENCY DRIFTING RADIO BURSTS: STATISTICAL PROPERTIES AND POLARIZATION | 134 |
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| 1 Introduction | 134 |
| 2 Spectral Characteristics | 135 |
| 3 Visibility Depending on Cassini’s Position | 137 |
| 4 Polarization | 138 |
| 5 Summary and Conclusions | 140 |
| References | 141 |
| ANALYSIS OF LATITUDINAL DEPENDENCE OF SATURNIAN RADIO EMISSIONS | 144 |
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| OBSERVATIONS OF CHORUS AT SATURN BY CASSINI | 146 |
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| THE LOCATION OF THE HIGH-DENSITY BOUNDARY IN SATURN’S INNER MAGNETOSPHERE | 148 |
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| References | 150 |
| DENSITY AND TEMPERATURE OF THE ELECTRON CORE IN THE INNER MAGNETOSPHERE OF SATURN FROM CASSINI/RPWS ANTENNAS | 152 |
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| OVERVIEW OF SATURN LIGHTNING OBSERVATIONS | 154 |
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| 1 Radio Observations of SEDs by Cassini RPWS | 154 |
| 2 Ground–based Radio Observations of SEDs | 155 |
| 3 Direct Optical Observations of Saturn Lightning Flashes | 156 |
| 4 Optical Observations of Storm Clouds | 156 |
| 5 Other Observations by Cassini VIMS and CIRS | 160 |
| 6 Comparison of lightning on Saturn, Jupiter, and Earth | 161 |
| 7 Summary and Conclusions | 162 |
| References | 162 |
| GROUND-BASED STUDY OF SATURN LIGHTNING | 164 |
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| 1 Introduction | 164 |
| 2 The Complementarity of Ground-based and Space-based Ob-servations | 165 |
| 3 Saturn Observations with UTR-2 | 166 |
| 4 Saturn Observations with WSRT | 168 |
| 5 First Saturn Observations with LOFAR | 169 |
| 6 Planned Observations | 171 |
| 7 Conclusion | 171 |
| References | 172 |
| ELECTRIC FIELD TRANSIENTS OBSERVED BY THE HUYGENS PROBE IN THE ATMOSPHERE OF TITAN: ATMOSPHERIC ELECTRICITY PHENOMENA OR ARTEFACTS? | 174 |
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| NEW TYPE OF PERIODIC BURSTS OF NON-IO JOVIAN DECAMETRIC RADIO EMISSION | 176 |
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| 1 Introduction | 176 |
| 2 Periodic non-Io DAM Radio Bursts and its Properties | 177 |
| 3 Discussion | 183 |
| 4 Summary | 183 |
| References | 184 |
| JUPITER’S DECAMETRIC AND HECTOMETRIC RADIO EMISSIONS OBSERVED BY CASSINI RPWS AND VOYAGER PRA | 186 |
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| 1 Introduction | 186 |
| 2 Observations and Analysis | 187 |
| 3 Discussion | 189 |
| 4 Summary | 192 |
| References | 193 |
| IO-JUPITER ELECTRODYNAMIC INTERACTION, ELECTRON ACCELERATION AND RADIO BURSTS GENERATION | 196 |
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| A MODEL OF JUPITER’S DECAMETRIC RADIO EMISSIONS AS A SEARCHLIGHT BEAM | 198 |
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| 1 Introduction | 198 |
| 2 TheDE Effect | 199 |
| 3 Model of a Searchlight Beam | 200 |
| 4 Delta Zone Effect | 203 |
| 5 Conclusion | 204 |
| References | 205 |
| JOVIAN DAM “ARCS” AND AURORAL CONTEXT | 206 |
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| ON THE ORIGIN OF IO’S ULTRAVIOLET AURORA | 208 |
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| 1 Introduction | 208 |
| 2 Heating Mechanism of Ionospheric Electrons and Generation of UV Emission | 210 |
| 3 Discussion | 213 |
| References | 214 |
| BEAMING CONE OF IO-CONTROLLED JOVIAN DECAMETER RADIO EMISSION AND EXISTENCE OF LOCALIZED ACTIVE LONGITUDE | 216 |
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| 1 Introduction | 216 |
| 2 Polar Distribution of the Source Regions | 218 |
| 3 Polar Distribution in Elliptic Coordinates | 219 |
| 4 Conclusions | 222 |
| References | 223 |
| ANALYSIS OF THE S-COMPONENTS FEATURES OF THE JOVIAN DAM EMISSION OBTAINED FOR THE IO-DEPENDENT SOURCES | 224 |
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| References | 227 |
| CONSIDERATION OF THE JOVIAN S-BURSTS AND NB-EMISSION BASED ON THE PARAMETRIC MODEL | 228 |
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| 1 Introduction | 228 |
| 2 Propagation of the Extraordinary Electromagnetic Wave in a Magnetized Plasma with Non-stationary Disturbances of the Magnetic Field | 230 |
| 3 Conc
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