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Solar noise storms /
Solar Noise Storms examines the properties and features of solar noise storm phenomenon. The book also presents some theories that can be used to gain a better understanding of the phenomenon. The coverage of the text includes topics that cover the features and behavior of noise storms, such as the...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Oxford ; New York :
Pergamon Press,
1977.
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| Edición: | 1st ed. |
| Colección: | International series in natural philosophy ;
v. 90. |
| Temas: | |
| Acceso en línea: | Texto completo |
Tabla de Contenidos:
- Front Cover; Solar Noise Storms; Copyright Page; Table of Contents; PREFACE; INTRODUCTION; ACKNOWLEDGEMENTS; Chapter 1. RELATIONS BETWEEN NOISE STORMS AND OPTICALLY OBSERVABLE FEATURES ON THE SUN; 1.1. THE ONSET OF NOISE STORMS; 1.2. RELATION BETWEEN NOISE STORMS AND FLARES; 1.3. NOISE STORMS AND SUNSPOTS; 1.4. RELATIVE POSITION OF NOISE STORM CENTRES AND OPTICALCENTRES OF ACTIVITY; 1.5. THE HEIGHT OF THE STORM CENTRES; 1.6. DOUBLE AND MULTIPLE SOURCES; 1.7. TYPE I BURST SOURCES; 1.8. VARIATIONS IN THE SOURCE POSITION; Chapter 2. THE SPECTRUM OF NOISE STORMS; 2.1. BACKGROUND CONTINUUM.
- 2.2. STORM BURSTS2.3. DURATION OF STORM BURSTS; 2.4. THE BANDWIDTH; Chapter 3. POLARIZATION OF NOISESTORM EMISSION; 3.1. POLARIZATION OF CONTINUUM; 3.2. POLARIZATION OF STORM BURSTS; 3.3. POLARIZATION OBSERVATIONS WITH HIGH SPATIAL AND TIME RESOLUTION; 3.4. THE EFFECT OF FARADAY ROTATION ON THE OBSERVED POLARIZATION; 3.5. MAGNETO-IONIC MODE COUPLING IN THE SOLAR CORONA; 3.6. MODE COUPLING AND POLARIZATION OF NOISE STORMS; 3.7. CONCLUDING REMARKS ON POLARIZATION; 3.8. SOME MODELS OF CORONAL MAGNETIC FIELDS AS DEDUCEDFROM STORM OBSERVATIONS; Chapter 4. DIRECTIVITY; 4.1. INTRODUCTION.
- 4.2. LONGITUDE EFFECTS4.3. OBSERVATIONS OF THE DIRECTIVITY OF INDIVIDUAL BURSTS; 4.4. EAST
- WEST ASYMMETRY OF NOISE STORMS; Chapter 5. CORONAL SCATTERING OF RADIATION FROM NOISE STORM SOURCES; 5.1. THE CORONA AS AN INHOMOGENEOUS MEDIUM; 5.2. COMPUTATION OF CORONAL SCATTERING OF RADIO WAVES IN THE SMALL ANGLE APPROXIMATION; 5.3. SCATTERING AS DETERMINED BY RAY TRACING; 5.4. OBSERVED FEATURES OF STORM EMISSION AS COMPARED WITH PREDICTIONS FROM SCATTERING THEORY; Chapter 6. ORDERED BEHAVIOUR OF STORM BURSTS IN THE TIME-FREQUENCY PLANE; 6.1. LARGE-SCALE FEATURES IN BURST ACTIVITY.
- 6.2. CHAINS OF TYPE I SOLAR RADIO BURSTS6.3. TIME SPLITTING OF BURSTS; 6.4. FREQUENCY SPLITTING; Chapter 7. PERIODIC AND QUASI-PERIODIC PHENOMENA; 7.1. INTENSITY VARIATIONS IN THE BACKGROUND CONTINUUM; 7.2. RELATIONS BETWEEN CONTINUUM FLUCTUATIONS AND OTHER VARIABLE PHENOMENA; 7.3. EXTREMELY RAPID, PERIODIC VARIATIONS; Chapter 8. METRIC NOISE STORMS AND RELATED PHENOMENA; 8.1. METRIC AND DECAMETRIC NOISE STORMS; 8.2. TYPE I STORM ACTIVITY AND EMISSION AT SHORT WAVELENGTHS; 8.3. TYPE I STORMS AND STATIONARY TYPE IV BURSTS; 8.4. RELATION BETWEEN TYPE I STORMS AND TYPE III BURSTS.
- 8.5. METRIC TYPE I STORMS AND ENERGETIC ELECTRONS IN THE INTERPLANETARY SPACE8.6. ACTIVE REGIONS AND INTERPLANETARY SECTOR STRUCTURE; Chapter 9. DISCUSSION OF SOME OBSERVEDFEATURES OF NOISE STORMS; 9.1. INTRODUCTION; 9.2. BURSTS AND BACKGROUND CONTINUUM; 9.3. ENERGIES INVOLVED IN NOISE STORM RADIATION; 9.4. DURATION OF TYPE I BURSTS; 9.5. BANDWIDTH OF TYPE I BURSTS; 9.6. FREQUENCY SPLITTING; Chapter 10. INTRODUCTION TO NOISESTORM THEORIES; 10.1. EARLY WORK; 10.2. MODELS OF STORM REGIONS; 10.3. SOME THEORETICAL CONCEPTS; Chapter 11. PLASMA WAVE THEORIES OF TYPE I BURSTS.