The bimodal transport in the plasma sheet consists of sunward large‐scale, coherent, and slow motion of charged particles in the closed‐field‐line region as well as meso‐scale, localized, and transient fast flow bursts. It has been found that these earthward moving bursty bulk flows, also called “bubbles,” play a crucial role not only in the transporting mass and energy, but also in resolving the pressure‐balance crisis with their integrated effects. In this study, we examine how bubbles can affect the average configuration of the middle and inner plasma sheet using the Inertialized Rice Convection Model (RCM‐I). Bubbles are sporadically imposed at
Explosive magnetotail activity has long been understood in the context of its auroral manifestations. While global models have been used to interpret and understand many magnetospheric processes, the temporal and spatial scales of some auroral forms have been inaccessible to global modeling creating a gulf between observational and theoretical studies of these phenomena. We present here an important step toward bridging this gulf using a newly developed global magnetosphere‐ionosphere model with resolution capturing
- NSF-PAR ID:
- 10374574
- Publisher / Repository:
- DOI PREFIX: 10.1029
- Date Published:
- Journal Name:
- Geophysical Research Letters
- Volume:
- 47
- Issue:
- 14
- ISSN:
- 0094-8276
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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