PDF (for b&w printout) - Living Reviews in Solar Physics
PDF (for b&w printout) - Living Reviews in Solar Physics
PDF (for b&w printout) - Living Reviews in Solar Physics
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6 Further Back <strong>in</strong> Time: The Pre-Ma<strong>in</strong> Sequence Sun 61<br />
6.1 Where was the cradle of the Sun? . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61<br />
6.2 New features <strong>in</strong> the pre-ma<strong>in</strong> sequence Sun . . . . . . . . . . . . . . . . . . . . . . 61<br />
6.2.1 Evolutionary stages: Overview . . . . . . . . . . . . . . . . . . . . . . . . . 61<br />
6.2.2 New features: Accretion, disks, and jets . . . . . . . . . . . . . . . . . . . . 62<br />
6.2.3 New emission properties: <strong>Solar</strong>-like or not? . . . . . . . . . . . . . . . . . . 62<br />
6.3 The T Tauri Sun . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63<br />
6.3.1 The magnetic field of the T Tauri Sun . . . . . . . . . . . . . . . . . . . . . 63<br />
6.3.2 The ultraviolet T Tauri Sun . . . . . . . . . . . . . . . . . . . . . . . . . . . 65<br />
6.3.3 The X-ray T Tauri Sun <strong>in</strong> time . . . . . . . . . . . . . . . . . . . . . . . . . 66<br />
6.3.4 Coronal excesses and deficits <strong>in</strong>duced by activity? . . . . . . . . . . . . . . 68<br />
6.3.5 X-ray flar<strong>in</strong>g of the T Tauri Sun . . . . . . . . . . . . . . . . . . . . . . . . 70<br />
6.3.6 The radio T Tauri Sun <strong>in</strong> time . . . . . . . . . . . . . . . . . . . . . . . . . 70<br />
6.3.7 The composition of the T Tauri Sun’s corona . . . . . . . . . . . . . . . . . 71<br />
6.4 The protostellar Sun . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72<br />
6.4.1 Magnetic activity <strong>in</strong> the protostellar Sun . . . . . . . . . . . . . . . . . . . 72<br />
6.4.2 Magnetic flar<strong>in</strong>g of the protostellar Sun . . . . . . . . . . . . . . . . . . . . 73<br />
6.4.3 Radio emission from the protostellar Sun . . . . . . . . . . . . . . . . . . . 73<br />
6.5 The pre-ma<strong>in</strong> sequence Sun’s environment <strong>in</strong> time . . . . . . . . . . . . . . . . . . 73<br />
6.5.1 Circumstellar disk ionization . . . . . . . . . . . . . . . . . . . . . . . . . . 73<br />
6.5.2 Circumstellar disk heat<strong>in</strong>g . . . . . . . . . . . . . . . . . . . . . . . . . . . . 74<br />
6.5.3 Observational evidence of disk irradiation . . . . . . . . . . . . . . . . . . . 76<br />
6.6 The T Tauri Sun’s activity and meteoritics . . . . . . . . . . . . . . . . . . . . . . 77<br />
6.7 Summary: The violent pre-ma<strong>in</strong> sequence Sun . . . . . . . . . . . . . . . . . . . . . 79<br />
7 The <strong>Solar</strong> System <strong>in</strong> Time: <strong>Solar</strong> Activity and Planetary Atmospheres 80<br />
7.1 The Fa<strong>in</strong>t Young Sun Paradox: Greenhouse or deep freeze? . . . . . . . . . . . . . 80<br />
7.1.1 The relevance of greenhouse gases . . . . . . . . . . . . . . . . . . . . . . . 81<br />
7.1.2 A bright young Sun? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82<br />
7.1.3 Cosmic rays and a stronger solar w<strong>in</strong>d . . . . . . . . . . . . . . . . . . . . . 84<br />
7.2 The Sun’s activity <strong>in</strong> the young solar system . . . . . . . . . . . . . . . . . . . . . 84<br />
7.2.1 Planetary atmospheric chemistry <strong>in</strong>duced by high-energy radiation . . . . . 84<br />
7.2.2 High-energy radiation and the planetary biospheres <strong>in</strong> habitable zones . . . 86<br />
7.2.3 Planetary atmospheric loss and high-energy radiation and particles . . . . . 87<br />
7.2.4 Mercury: Erosion of atmosphere and mantle? . . . . . . . . . . . . . . . . . 89<br />
7.2.5 Venus: Where has the water gone? . . . . . . . . . . . . . . . . . . . . . . . 89<br />
7.2.6 Earth: A CO2 atmosphere and magnetic protection . . . . . . . . . . . . . 90<br />
7.2.7 Mars: Once warmer and wetter? . . . . . . . . . . . . . . . . . . . . . . . . 91<br />
7.2.8 Venus, Earth, Mars: Similar start, different results? . . . . . . . . . . . . . 92<br />
7.2.9 Titan: Early atmospheric blow-off? . . . . . . . . . . . . . . . . . . . . . . . 93<br />
7.2.10 Hot Jupiters: Mass evolution by evaporation? . . . . . . . . . . . . . . . . . 94<br />
7.3 Summary: The high-energy young solar system . . . . . . . . . . . . . . . . . . . . 95<br />
8 Summary and Conclusions 96<br />
9 Acknowledgements 99<br />
References 100