Planetary Radio Emissions VII

1 - FOREWORD [Seite 6]
2 - SPONSORS [Seite 8]
3 - CONTENTS [Seite 10]
4 - SATURN'S RADIO EMISSIONS AND THEIR RELATION TO MAGNETOSPHERIC DYNAMICS [Seite 20]
4.1 - 1 Introduction [Seite 20]
4.2 - 2 Solar Wind Influence on Saturn'sMagnetospheric Radio Emis-sions [Seite 21]
4.3 - 3 Magnetotail Reconnection and Radio Emissions: Terrestrial Review [Seite 22]
4.4 - 4 Magnetotail Reconnection at Saturn and Link to Radio Emis-sions [Seite 24]
4.5 - 5 Conclusion [Seite 27]
4.6 - References [Seite 28]
5 - DIRECTION FINDING AND POLARIZATION MEASUREMENTS OF SKR [Seite 32]
5.1 - 1 Introduction [Seite 32]
5.2 - 2 How the RPWS Instrument Works [Seite 33]
5.3 - 3 Some Already Published DF&Pol Results on SKR [Seite 34]
5.4 - 4 Improving DF&pol Retrieval Technique [Seite 35]
5.5 - 5 Some Improved Results on SKR [Seite 45]
5.6 - 6 Summary [Seite 51]
5.7 - References [Seite 52]
6 - AN OVERVIEW OF THE TIME-DEPENDENT ROTATIONAL MODULATION OF SATURNIAN RADIO EMISSIONS [Seite 56]
7 - VARIABILITY OF SOUTHERN AND NORTHERN SKR PERIODICITIES [Seite 58]
7.1 - 1 Introduction [Seite 58]
7.2 - 2 Radio Observations and Harmonic Analysis [Seite 59]
7.3 - 3 Variability of SKR Periodicities [Seite 61]
7.4 - 4 Nature of the SKR Diurnal Modulation [Seite 65]
7.5 - 5 Conclusions [Seite 67]
7.6 - References [Seite 67]
8 - AN SLS4 LONGITUDE SYSTEM BASED ON A TRACKING FILTER ANALYSIS OF THE ROTATIONAL MODULATION OF SATURN KILOMETRIC RADIATION [Seite 70]
8.1 - 1 Introduction [Seite 71]
8.2 - 2 SKR Modulation Spectrum [Seite 73]
8.3 - 3 Phase and Longitude Analysis [Seite 77]
8.4 - 4 The SLS4-N and SLS4-S Longitude Systems [Seite 80]
8.5 - 5 Accessing the SLS4 Longitude System [Seite 80]
8.6 - References [Seite 82]
9 - IS A RIKITAKE DYNAMO IN SATURN'S INTERIOR AT THE ORIGIN OF THE VARIABILITY OF THE RADIO ROTATION PERIODS? [Seite 84]
9.1 - 1 Introduction [Seite 84]
9.2 - 2 Particularity of Saturn's Magnetic Field [Seite 85]
9.3 - 3 Dynamo Effect in Saturn's Interior [Seite 86]
9.4 - 4 Results and Conclusion [Seite 89]
9.5 - References [Seite 90]
10 - SOLAR WIND AND SATURNIAN MOONS SIGNATURES IN THE LONG-PERIODIC MODULATIONS OF SKR [Seite 92]
11 - A CLOSE ENCOUNTER WITH A SATURN KILOMETRIC RADIATION SOURCE REGION [Seite 94]
11.1 - 1 Introduction [Seite 94]
11.2 - 2 Observations [Seite 95]
11.3 - 3 Discussion [Seite 99]
11.4 - References [Seite 101]
12 - SATURN KILOMETRIC RADIATION NEAR A SOURCE CENTER ON DAY 73, 2008 [Seite 106]
12.1 - 1 Introduction [Seite 106]
12.2 - 2 Instrumentation, Observations, and Analysis [Seite 107]
12.3 - 3 Summary and Conclusions [Seite 112]
12.4 - References [Seite 112]
13 - PROPERTIES OF SATURN KILOMETRIC RADIATION MEASURED WITHIN ITS SOURCE REGION [Seite 116]
14 - AN OVERVIEW OF SATURN NARROWBAND RADIO EMISSIONS OBSERVED BY CASSINI RPWS [Seite 118]
14.1 - 1 Introduction [Seite 119]
14.2 - 2 Source Mechanism [Seite 119]
14.3 - 3 Polarization and Intensity Measurements [Seite 120]
14.4 - 4 Direction Finding Results [Seite 123]
14.5 - 5 Z-mode Narrowband Emissions Below fce [Seite 124]
14.6 - 6 Rotational Modulation [Seite 126]
14.7 - 7 Conclusion [Seite 128]
14.8 - References [Seite 129]
15 - SATURNIAN LOW FREQUENCY DRIFTING RADIO BURSTS: STATISTICAL PROPERTIES AND POLARIZATION [Seite 134]
15.1 - 1 Introduction [Seite 134]
15.2 - 2 Spectral Characteristics [Seite 135]
15.3 - 3 Visibility Depending on Cassini's Position [Seite 137]
15.4 - 4 Polarization [Seite 138]
15.5 - 5 Summary and Conclusions [Seite 140]
15.6 - References [Seite 141]
16 - ANALYSIS OF LATITUDINAL DEPENDENCE OF SATURNIAN RADIO EMISSIONS [Seite 144]
17 - OBSERVATIONS OF CHORUS AT SATURN BY CASSINI [Seite 146]
18 - THE LOCATION OF THE HIGH-DENSITY BOUNDARY IN SATURN'S INNER MAGNETOSPHERE [Seite 148]
18.1 - References [Seite 150]
19 - DENSITY AND TEMPERATURE OF THE ELECTRON CORE IN THE INNER MAGNETOSPHERE OF SATURN FROM CASSINI/RPWS ANTENNAS [Seite 152]
20 - OVERVIEW OF SATURN LIGHTNING OBSERVATIONS [Seite 154]
20.1 - 1 Radio Observations of SEDs by Cassini RPWS [Seite 154]
20.2 - 2 Ground-based Radio Observations of SEDs [Seite 155]
20.3 - 3 Direct Optical Observations of Saturn Lightning Flashes [Seite 156]
20.4 - 4 Optical Observations of Storm Clouds [Seite 156]
20.5 - 5 Other Observations by Cassini VIMS and CIRS [Seite 160]
20.6 - 6 Comparison of lightning on Saturn, Jupiter, and Earth [Seite 161]
20.7 - 7 Summary and Conclusions [Seite 162]
20.8 - References [Seite 162]
21 - GROUND-BASED STUDY OF SATURN LIGHTNING [Seite 164]
21.1 - 1 Introduction [Seite 164]
21.2 - 2 The Complementarity of Ground-based and Space-based Ob-servations [Seite 165]
21.3 - 3 Saturn Observations with UTR-2 [Seite 166]
21.4 - 4 Saturn Observations with WSRT [Seite 168]
21.5 - 5 First Saturn Observations with LOFAR [Seite 169]
21.6 - 6 Planned Observations [Seite 171]
21.7 - 7 Conclusion [Seite 171]
21.8 - References [Seite 172]
22 - ELECTRIC FIELD TRANSIENTS OBSERVED BY THE HUYGENS PROBE IN THE ATMOSPHERE OF TITAN: ATMOSPHERIC ELECTRICITY PHENOMENA OR ARTEFACTS? [Seite 174]
23 - NEW TYPE OF PERIODIC BURSTS OF NON-IO JOVIAN DECAMETRIC RADIO EMISSION [Seite 176]
23.1 - 1 Introduction [Seite 176]
23.2 - 2 Periodic non-Io DAM Radio Bursts and its Properties [Seite 177]
23.3 - 3 Discussion [Seite 183]
23.4 - 4 Summary [Seite 183]
23.5 - References [Seite 184]
24 - JUPITER'S DECAMETRIC AND HECTOMETRIC RADIO EMISSIONS OBSERVED BY CASSINI RPWS AND VOYAGER PRA [Seite 186]
24.1 - 1 Introduction [Seite 186]
24.2 - 2 Observations and Analysis [Seite 187]
24.3 - 3 Discussion [Seite 189]
24.4 - 4 Summary [Seite 192]
24.5 - References [Seite 193]
25 - IO-JUPITER ELECTRODYNAMIC INTERACTION, ELECTRON ACCELERATION AND RADIO BURSTS GENERATION [Seite 196]
26 - A MODEL OF JUPITER'S DECAMETRIC RADIO EMISSIONS AS A SEARCHLIGHT BEAM [Seite 198]
26.1 - 1 Introduction [Seite 198]
26.2 - 2 TheDE Effect [Seite 199]
26.3 - 3 Model of a Searchlight Beam [Seite 200]
26.4 - 4 Delta Zone Effect [Seite 203]
26.5 - 5 Conclusion [Seite 204]
26.6 - References [Seite 205]
27 - JOVIAN DAM "ARCS" AND AURORAL CONTEXT [Seite 206]
28 - ON THE ORIGIN OF IO'S ULTRAVIOLET AURORA [Seite 208]
28.1 - 1 Introduction [Seite 208]
28.2 - 2 Heating Mechanism of Ionospheric Electrons and Generation of UV Emission [Seite 210]
28.3 - 3 Discussion [Seite 213]
28.4 - References [Seite 214]
29 - BEAMING CONE OF IO-CONTROLLED JOVIAN DECAMETER RADIO EMISSION AND EXISTENCE OF LOCALIZED ACTIVE LONGITUDE [Seite 216]
29.1 - 1 Introduction [Seite 216]
29.2 - 2 Polar Distribution of the Source Regions [Seite 218]
29.3 - 3 Polar Distribution in Elliptic Coordinates [Seite 219]
29.4 - 4 Conclusions [Seite 222]
29.5 - References [Seite 223]
30 - ANALYSIS OF THE S-COMPONENTS FEATURES OF THE JOVIAN DAM EMISSION OBTAINED FOR THE IO-DEPENDENT SOURCES [Seite 224]
30.1 - References [Seite 227]
31 - CONSIDERATION OF THE JOVIAN S-BURSTS AND NB-EMISSION BASED ON THE PARAMETRIC MODEL [Seite 228]
31.1 - 1 Introduction [Seite 228]
31.2 - 2 Propagation of the Extraordinary Electromagnetic Wave in a Magnetized Plasma with Non-stationary Disturbances of the Magnetic Field [Seite 230]
31.3 - 3 Conclusion [Seite 233]
31.4 - References [Seite 234]
32 - S/NB-EVENTS OF JOVIAN DECAMETRIC EMISSION [Seite 238]
32.1 - 1 Introduction [Seite 238]
32.2 - 2 Motion of an Emitter [Seite 239]
32.3 - 3 Dispersion Delay [Seite 241]
32.4 - 4 Shadow Effect [Seite 242]
32.5 - 5 Synthetic and Real Spectra [Seite 242]
32.6 - 6 Conclusions [Seite 244]
32.7 - References [Seite 245]
33 - JOVIAN RADIO EMISSIONS MODELING AND THEIR FUTURE INVESTIGATION WITH EJSM [Seite 246]
34 - EXPLORATION OF JUPITER'S POLAR MAGNETOSPHERE AND RADIO EMISSIONS WITH THE JUNO MISSION [Seite 248]
35 - VARIABILITY OF JUPITER'S SYNCHROTRON EMISSION IN MID-2009 [Seite 250]
35.1 - 1 Introduction [Seite 250]
35.2 - 2 Observation and Data Reduction [Seite 251]
35.3 - 3 Brightness Distribution at 6 cm [Seite 252]
35.4 - 4 Response to a Comet-like Impact [Seite 254]
35.5 - 5 Conclusion [Seite 256]
35.6 - References [Seite 257]
36 - RX AND Z-MODE GROWTH RATES AND PROPAGATION AT CAVITY BOUNDARIES [Seite 260]
36.1 - 1 Introduction [Seite 260]
36.2 - 2 Wave Modes in a Cold Magnetized Plasma [Seite 261]
36.3 - 3 Cluster Observations of RX and Z ModeWaves in the Earth's Auroral Acceleration Region [Seite 263]
36.4 - References [Seite 270]
37 - WAVEGUIDE MODES IN THE AKR SOURCE [Seite 272]
37.1 - 1 Introduction [Seite 272]
37.2 - 2 Measurements and the Analysis [Seite 273]
37.3 - 3 Discussion [Seite 276]
37.4 - 4 Conclusion [Seite 277]
37.5 - References [Seite 278]
38 - AKR SOURCES POSITIONS - INTERBALL-2 VS CLUSTER OBSERVATIONS [Seite 280]
38.1 - 1 Introduction [Seite 280]
38.2 - 2 Tangent Plane Beaming Model [Seite 281]
38.3 - 3 Interball-2 Observations - Direction Finding [Seite 281]
38.4 - 4 AKR Visibility Maps and Results [Seite 282]
38.5 - 5 Conclusions [Seite 284]
38.6 - References [Seite 285]
39 - CAN THE RELATIVISTIC MASER MECHANISM CAUSE THE STRONG EMISSIONS REGISTERED BY CLUSTER AND DEMETER SATELLITES IN THE POLAR CUSP? [Seite 288]
40 - MEDIUM FREQUENCY BURST EMISSIONS: A TERRESTRIAL ANALOG TO SOLAR TYPE III BURSTS? [Seite 290]
40.1 - 1 Introduction [Seite 290]
40.2 - 2 Review of Recent Observational Work [Seite 291]
40.3 - 3 Review of Recent Theoretical Work [Seite 294]
40.4 - 4 Conclusions [Seite 298]
40.5 - References [Seite 299]
41 - AKR DIURNAL, SEMI-DIURNAL AND SHORTER TERM MODULATIONS DISENTANGLED BY CASSINI/RPWS OBSERVATIONS [Seite 302]
42 - GROUND-LEVEL DETECTION OF AURORAL KILOMETRIC RADIATION [Seite 304]
43 - THE SEARCH FOR EXOPLANETARY RADIO EMISSIONS [Seite 306]
43.1 - 1 Historical Landmarks [Seite 306]
43.2 - 2 Theoretical Predictions [Seite 307]
43.3 - 3 Early Low-frequency Observations [Seite 308]
43.4 - 4 Tentative Optical Detection and More Theoretical Work [Seite 310]
43.5 - 5 Recent Low-frequency Observations [Seite 312]
43.6 - 6 Method and Motivations [Seite 313]
43.7 - 7 Perspectives [Seite 314]
43.8 - References [Seite 316]
44 - EXOPLANET MAGNETIC FIELD ESTIMATION VIA ENERGETIC NEUTRAL ATOMS (ENAS) AND HYDROGEN CLOUD OBSERVATIONS AND MODELLING [Seite 322]
44.1 - 1 Introduction [Seite 323]
44.2 - 2 Expanding Thermospheres of "Hot Jupiters" [Seite 324]
44.3 - 3 Stellar Wind Interaction with HD 209458b and Production of Hydrogen and ENA-Clouds [Seite 324]
44.4 - 4 Conclusion [Seite 328]
44.5 - References [Seite 329]
45 - RADIO EMISSION FROM MAGNETIC EXOPLANETS: PROGRESS REPORT ON GMRT OBSERVATIONS AND RESULTS [Seite 332]
46 - ON THE POSSIBILITY OF RADIO EMISSION OF PLANETS AROUND PULSARS [Seite 334]
46.1 - 1 Exoplanets Around Pulsars [Seite 334]
46.2 - 2 Alfv´en Wings [Seite 336]
46.3 - 3 Radio Emissions from the Alfv´en Wings [Seite 338]
46.4 - 4 Characteristics of the Radio Emissions from a Planet Around a Pulsar [Seite 340]
46.5 - 5 Conclusion [Seite 340]
46.6 - References [Seite 342]
47 - CORONAL MASS EJECTIONS AND SOLAR RADIO EMISSIONS [Seite 344]
47.1 - 1 Introduction [Seite 344]
47.2 - 2 Type III Bursts [Seite 346]
47.3 - 3 TypeIIBursts [Seite 349]
47.4 - 4 TypeIVBursts [Seite 355]
47.5 - 5 Conclusions [Seite 357]
47.6 - References [Seite 357]
48 - DECAMETER RADIO EMISSION OF THE SUN: RECENT OBSERVATIONS [Seite 362]
48.1 - 1 Introduction [Seite 362]
48.2 - 2 Type III-like Bursts [Seite 363]
48.3 - 3 Powerful Type III Bursts [Seite 364]
48.4 - 4 Decameter Type IIIb Bursts [Seite 364]
48.5 - 5 Inverted Decameter U- and J-bursts [Seite 365]
48.6 - 6 Dog-leg Type III Bursts [Seite 366]
48.7 - 7 TypeIVBursts [Seite 366]
48.8 - 8 Decameter Spikes [Seite 367]
48.9 - 9 S-bursts [Seite 367]
48.10 - 10 Conclusion [Seite 367]
48.11 - References [Seite 369]
49 - PROPERTIES OF DECAMETER SPIKES [Seite 370]
49.1 - 1 Introduction [Seite 370]
49.2 - 2 Observations [Seite 371]
49.3 - 3 Discussion [Seite 375]
49.4 - 4 Conclusion [Seite 376]
49.5 - References [Seite 376]
50 - UNUSUAL TYPE III BURSTS AT THE DECAMETRE WAVELENGTHS [Seite 378]
50.1 - 1 Introduction [Seite 378]
50.2 - 2 Instruments [Seite 380]
50.3 - 3 Observations [Seite 380]
50.4 - 4 Discussion [Seite 383]
50.5 - 5 Conclusion [Seite 384]
50.6 - References [Seite 384]
51 - PROPERTIES OF POWERFUL SOLAR TYPE III BURSTS IN THE FREQUENCY RANGE OF 10-30 MHZ [Seite 386]
51.1 - 1 Introduction [Seite 386]
51.2 - 2 Observations [Seite 387]
51.3 - 3 Conclusion [Seite 390]
51.4 - References [Seite 391]
52 - PROPAGATION OF ENERGETIC ELECTRONS FROM THE CORONA INTO INTERPLANETARY SPACE AND TYPE III RADIO EMISSION [Seite 392]
52.1 - 1 Introduction [Seite 392]
52.2 - 2 Drift Rates and Radial Propagation Velocity [Seite 394]
52.3 - 3 Density Model for the Interplanetary Space [Seite 395]
52.4 - 4 Results [Seite 397]
52.5 - 5 Conclusion [Seite 398]
52.6 - References [Seite 398]
53 - LOCAL TIME OCCURRENCE OF SOLAR TYPE III BURSTS AT SATURN'S ORBIT [Seite 400]
53.1 - 1 Introduction [Seite 400]
53.2 - 2 Type III Burst Occurrence [Seite 401]
53.3 - 3 Discussion and Conclusion [Seite 403]
53.4 - References [Seite 405]
54 - AN INFLUENCE OF ANTENNA TILT ANGLE TO THE RPW/SOLAR ORBITER DIRECTION FINDING [Seite 408]
54.1 - References [Seite 409]
55 - NUMERICAL SIMULATION OF THE PROPAGATION OF TYPE III RADIO EMISSION [Seite 410]
55.1 - 1 Introduction [Seite 410]
55.2 - 2 The Model [Seite 411]
55.3 - 3 Results [Seite 414]
55.4 - 4 Conclusion [Seite 416]
55.5 - References [Seite 416]
56 - LOCALIZED LANGMUIR EIGENMODES AND SOLAR RADIO BURSTS [Seite 418]
56.1 - 1 Introduction [Seite 418]
56.2 - 2 Langmuir-eigenmode Modulation [Seite 419]
56.3 - 3 Langmuir-eigenmode Radiation [Seite 421]
56.4 - 4 Interactions with Density Turbulence [Seite 423]
56.5 - 5 Conclusions [Seite 424]
56.6 - References [Seite 425]
57 - COMPLEX ZEBRA PATTERNS IN SOLAR RADIO EMISSION AND GENERATION MECHANISMS [Seite 426]
57.1 - 1 Introduction [Seite 426]
57.2 - 2 Generation Mechanisms [Seite 427]
57.3 - 3 NewObservation [Seite 428]
57.4 - 4 OtherMechanisms [Seite 430]
57.5 - 5 The New Alternative Mechanism of the ZP due to Develop-ment of Explosive Instability in the System Beam-plasma [Seite 431]
57.6 - 6 Conclusion [Seite 433]
57.7 - References [Seite 433]
58 - SOLAR RADIO EMISSIONS IN VIEW OF THE SOLAR ORBITER MISSION [Seite 436]
59 - MILLIMETER RADIO ASTRONOMY AND THE SOLAR CONVECTION ZONE [Seite 438]
59.1 - 1 Introduction [Seite 438]
59.2 - 2 Turbulence in Large-scale Pattern of Active Regions [Seite 439]
59.3 - 3 Gigantic Convection Cells and Preferred Scales [Seite 441]
59.4 - 4 What Can be Seen at Millimeter Wavelengths? [Seite 443]
59.5 - 5 Conclusions [Seite 444]
59.6 - References [Seite 445]
60 - UNUSUAL SPECTRA OF POLARISED RADIO EMISSION OF ACTIVE REGIONS ON THE SUN [Seite 446]
60.1 - 1 Introduction [Seite 446]
60.2 - 2 Observations [Seite 446]
60.3 - 3 Model [Seite 447]
60.4 - 4 Model Calculations [Seite 448]
60.5 - 5 Estimations of Physical Conditions in a Loop [Seite 450]
60.6 - 6 Conclusions [Seite 451]
60.7 - References [Seite 451]
61 - LONG-PERIODIC TRANSVERSE OSCILLATIONS OF CORONAL LOOPS AND MODULATIONS OF SOLAR MICROWAVE RADIATION [Seite 454]
61.1 - 1 Introduction [Seite 454]
61.2 - 2 Diagnostics of Oscillating Coronal Loops via VLF Modula-tions of mm-Radiation [Seite 456]
61.3 - 3 Magnetic Field Variations, Estimated from VLF Spectra [Seite 460]
61.4 - 4 Conclusions [Seite 460]
61.5 - References [Seite 461]
62 - PLASMA HEATING BY THE PARAMETRIC EXCITATION OF ACOUSTIC WAVES IN CORONAL MAGNETIC LOOPS [Seite 464]
62.1 - 1 Introduction [Seite 464]
62.2 - 2 Parametric Resonance [Seite 465]
62.3 - 3 Energy of the Acoustic Waves [Seite 466]
62.4 - 4 Dissipation of the Acoustic Waves or the Heating Rate [Seite 468]
62.5 - 5 Heating of Coronal Magnetic Loops [Seite 469]
62.6 - 6 Discussion [Seite 470]
62.7 - 7 Conclusions [Seite 470]
62.8 - References [Seite 471]
63 - CORONAL MAGNETIC FIELD STRUCTURE IN SOLAR ACTIVE REGIONS [Seite 474]
63.1 - 1 Introduction [Seite 474]
63.2 - 2 Method of the Magnetic Field Determination [Seite 475]
63.3 - 3 Calculation Results [Seite 476]
63.4 - 4 Discussion and Conclusions [Seite 478]
63.5 - References [Seite 481]
64 - MAGNETOHYDRODYNAMIC SHOCKS AND SOLITONS IN THE SOLAR ATMOSPHERE: RECENT CHALLENGES IN OBSERVATIONS AND THEORY [Seite 484]
64.1 - 1 Introduction [Seite 484]
64.2 - 2 First Observation of Slow Sausage Soliton in the Solar Atmo-sphere [Seite 485]
64.3 - 3 Shock Waves as Important Part of Spicule Formation Mech-anism in the Solar Atmosphere [Seite 485]
64.4 - 4 Results and Conclusions [Seite 488]
64.5 - References [Seite 489]
65 - STEREO OBSERVATIONS OF LARGE-SCALE WAVES IN THE SOLAR CORONA [Seite 490]
66 - STUDY OF THE KINEMATICS, DRIVER OF THE GLOBAL MORETON WAVE OBSERVED ON 28-10-2003 [Seite 492]
67 - IMPLICATIONS OF ANTENNA SYSTEM CALIBRATION ON SPACECRAFT DESIGN AND RADIO DATA ANALYSIS [Seite 494]
67.1 - 1 The Concept of Effective Length Vector of an Antenna [Seite 494]
67.2 - 2 Antenna System Calibration Methods [Seite 495]
67.3 - 3 Numerical Computer Simulation of Antenna System Calibra-tion [Seite 497]
67.4 - 4 Conclusions [Seite 500]
67.5 - References [Seite 501]
68 - NUMERICAL SIMULATIONS OF THE SOLAR ORBITER ANTENNA SYSTEM RPW ANT [Seite 506]
68.1 - 1 Introduction [Seite 506]
68.2 - 2 Spacecraft Modeling [Seite 508]
68.3 - 3 Numerical Simulations [Seite 509]
68.4 - 4 Results [Seite 509]
68.5 - 5 Conclusions [Seite 512]
68.6 - References [Seite 512]
69 - ANTENNA DESIGN AND DISTRIBUTION FOR A LOFAR SUPER STATION IN NANC¸AY [Seite 514]
69.1 - 1 Introduction [Seite 514]
69.2 - 2 The LOFAR Super Station [Seite 515]
69.3 - 3 Three Key Design Studies for the LSS [Seite 517]
69.4 - 4 Conclusion [Seite 521]
69.5 - References [Seite 521]
70 - PLANETARY AND EXOPLANETARY STUDIES WITH THE GIANT RADIO TELESCOPE LOFAR [Seite 524]
71 - SOLAR OBSERVATIONS WITH LOFAR [Seite 526]
71.1 - 1 Introduction [Seite 526]
71.2 - 2 Solar Radio Emission [Seite 528]
71.3 - 3 Solar Observation Modes with LOFAR [Seite 530]
71.4 - 4 Concluding Remarks [Seite 530]
71.5 - References [Seite 531]
72 - COMBINED RADIO OBSERVATIONS WITH LOFAR AND THE GIANT UKRAINIAN RADIO TELESCOPE [Seite 532]
72.1 - 1 Introduction [Seite 532]
72.2 - 2 LOFAR [Seite 534]
72.3 - 3 GURT - The Giant Ukrainian Radio Telescope [Seite 535]
72.4 - 4 Joint LOFAR and GURT Observations [Seite 536]
72.5 - 5 Science [Seite 537]
72.6 - 6 DataFormats [Seite 538]
72.7 - 7 Conclusion [Seite 538]
72.8 - References [Seite 538]
73 - NEW ANTENNAS AND METHODS FOR THE LOW FREQUENCY STELLAR AND PLANETARY RADIO ASTRONOMY [Seite 540]
73.1 - 1 Introduction [Seite 540]
73.2 - 2 The Tasks of the Ground-based Low Frequency Radio As-tronomy (10-100 MHz) in the Stellar and Planetary Science [Seite 541]
73.3 - 3 Existing Radio Telescopes and Instrumentation [Seite 541]
73.4 - 4 Some New Examples of the Sun, Stellar, and Planetary Ob-servations [Seite 543]
73.5 - 5 Giant Ukrainian Radio Telescope (GURT) Concept [Seite 547]
73.6 - 6 Conclusion [Seite 548]
73.7 - References [Seite 549]
74 - TESTS OF AN ACTIVE, BROAD-BAND ANTENNA ARRAY [Seite 552]
74.1 - 1 Introduction [Seite 552]
74.2 - 2 The Active Dipole for the Low-frequency Array [Seite 553]
74.3 - 3 Antenna Array [Seite 555]
74.4 - 4 Conclusion [Seite 557]
74.5 - References [Seite 558]
75 - OBSERVING SOLAR RADIO BURSTS FROM THE LUNAR SURFACE [Seite 560]
75.1 - 1 Introduction [Seite 560]
75.2 - 2 ScientificGoals [Seite 561]
75.3 - 3 Implementation [Seite 564]
75.4 - 4 Conclusion [Seite 568]
75.5 - References [Seite 568]
76 - BROADBAND OBSERVATIONS OF RADIO EMISSION OF FLARE STARS [Seite 570]
76.1 - 1 Introduction [Seite 570]
76.2 - 2 Instrumentation [Seite 571]
76.3 - 3 Observations and data processing [Seite 572]
76.4 - 4 Conclusions [Seite 574]
76.5 - References [Seite 574]
77 - ON KINETIC APPROACH TO MODELING OF SOURCES OF ELECTROMAGNETIC RADIATION LOCATED IN PLANET/STELLAR ELECTROMAGNETIC STRUCTURES [Seite 576]
78 - ON DUST KINETIC ALFV ´ EN WAVES AND STREAMING INSTABILITY IN A LORENTZIAN MAGNETOPLASMA [Seite 578]
78.1 - 1 Introduction [Seite 578]
78.2 - 2 BasicEquations [Seite 579]
78.3 - 3 Lorentzian Number Density and Current Density Perturba-tions [Seite 580]
78.4 - 4 Dispersion Relation [Seite 582]
78.5 - 5 Discussions [Seite 584]
78.6 - 6 References [Seite 586]
79 - IMPROVED RADIO STUDIES OF SPACE BY USING NEW EM DEGREES OF FREEDOM [Seite 590]
80 - 101 THINGS THAT YOU MIGHT HAVE WONDERED ABOUT SPACE PLASMA WAVE RESEARCH BUT WERE AFRAID TO ASK! [Seite 592]
81 - Email-List of Participants/Authors: [Seite 593]