Plasma waves in the Hermean magnetosphere

被引：12

作者：

Blomberg, L. G. ^{[1
]}

Cumnock, J. A. ^{[1
]}

Glassmeier, K. -H. ^{[2
]}

Treumann, R. A. ^{[3
]}

机构：

[1] Royal Inst Technol, Sch Elect Engn, Stockholm, Sweden

[2] Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, Braunschweig, Germany

[3] Univ Munich, Dept Geophys & Environm Phys, Geophys Sect, Munich, Germany

来源：

SPACE SCIENCE REVIEWS | 2007年 / 132卷 / 2-4期

关键词：

Mercury; magnetosphere; plasma waves; pulsations; magnetospheric radiation;

D O I：

10.1007/s11214-007-9282-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Hermean magnetosphere is likely to contain a number of wave phenomena. We briefly review what little is known so far about fields and waves around Mercury. We further discuss a number of possible phenomena, including ULF pulsations, acceleration-related radiation, bow shock waves, bremsstrahlung (or braking radiation), and synchrotron radiation. Finally, some predictions are made as to the likelihood that some of these types of wave emission exist.

引用

页码：575 / 591

页数：17

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