The polar caps
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概要
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In the past we have somewhat slighted upper atmospheric phenomena in the area bounded approximately by the auroral oval because our main interests have traditionally been concentrated on understanding magneto-spheric substorms along the auroral oval; substorms are due primarily to the southward component of the interplanetary magnetic field (IMF). However, it has recently become clear that a great variety of fascinating phenomena take place in this highest latitude region of the earth when the IMF has an appreciable northward component. The importance of those phenomena in understanding basic magnetospheric processes is emphasized. Systematic observational programs specifically designed to study those phenomena in the Antarctic region could make significant contributions to upper atmospheric physics and magnetospheric physics.
- 国立極地研究所の論文
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関連論文
- Effects of the interplanetary magnetic field on the characteristics of Pc 3-4 pulsations at globally coordinated stations
- Polar cap arcs and their relationship to IMF and geomagnetic activity
- The polar caps
- Coordinated observations of ionosphere-atmosphere coupling in the arctic using an HF Doppler system and an infrasonic wave detector