Titlebook: Characterizing Stellar and Exoplanetary Environments; Helmut Lammer,Maxim Khodachenko Book 2015 The Editor(s) (if applicable) and The Auth

本土

Leaven

Energierechtliche Rahmenbedingungen,he different ways in which a planetary magnetic field may modify the planetary evolution and reviews the different methods that have been suggested to detect these fields. These methods are compared and we evaluate which techniques have the highest potential for future detection of exoplanetary magnetic fields.

钱财

Dislocation

Detection Methods and Relevance of Exoplanetary Magnetic Fieldshe different ways in which a planetary magnetic field may modify the planetary evolution and reviews the different methods that have been suggested to detect these fields. These methods are compared and we evaluate which techniques have the highest potential for future detection of exoplanetary magnetic fields.

生气的边缘

Alfvén Radius: A Key Parameter for Astrophysical Magnetospheresf its origin, direction of motion and material in it) in the presence of a strong magnetic field is located close to the Alfvén radius. For magnetized planets a concept of Alfvén radius is important as for the interaction with the solar/stellar wind, either for the inter-magnetospheric processes.

Ballad

FELON

Stellar Winds in Timedge of how they evolve with time. Determining this empirically requires the ability to study the winds of stars of various ages and activity levels, but this is not easy to do as the coronal winds of solar-like stars are very hard to detect. Relevant observations are here reviewed, as well as more t

经典

杀人

饰带