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H

H. Lühr

Researcher at Braunschweig University of Technology

Publications -  116
Citations -  8917

H. Lühr is an academic researcher from Braunschweig University of Technology. The author has contributed to research in topics: Solar wind & Magnetosphere. The author has an hindex of 45, co-authored 116 publications receiving 8464 citations.

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Journal ArticleDOI

Bursty Bulk Flows in the Inner Central Plasma Sheet

TL;DR: In this article, high-speed flows in the inner central plasma sheet are studied, together with the concurrent behavior of the plasma and magnetic field, by using AMPTE/IRM data from about 9 to 19 R(E) in the earth magnetotail.

Bursty bulk flows in the inner central plasma sheet: An effective means of earthward transport in the magnetotail

TL;DR: In this paper, the importance of different flow magnitude samples for Earthward transport in the ICPS are statistically evaluated and several representative Bursty Bulk Flow (BBF) events and their relevance to Earth-ward transport are discussed.
Journal ArticleDOI

The magnetopause for large magnetic shear: AMPTE/IRM observations

TL;DR: In this paper, the authors used the improved accuracy and time resolution of the IRM plasma measurements to reexamine the occurrence of high-speed flows as signatures of the reconnection process at the magnetopause.
Book ChapterDOI

The cluster magnetic field investigation

TL;DR: The Cluster mission as mentioned in this paper provides a new opportunity to study plasma processes and structures in the near-Earth plasma environment using four-point measurements of the magnetic field, which can enable the analysis of the three dimensional structure and dynamics of a range of phenomena which shape the macroscopic properties of the magnetosphere.
Journal ArticleDOI

The magnetosheath region adjacent to the dayside magnetopause: AMPTE/IRM observations

TL;DR: In this paper, the magnetic shear across the magnetopause has been investigated and the magnetic field in the magnetosheath region adjacent to the dayside magnetosphere has been found to depend strongly on the angle between the magnetoheath magnetic field and the geomagnetic field.