Results 161 to 170 of about 17,830 (208)
Nonbacterial Thrombotic Endocarditis and Mechanical Valve Thrombosis in a Patient with Antiphospholipid Syndrome. [PDF]
Bravo F +6 more
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Small left ventricular size as a predictor for incident type 2 diabetes: insights from the UK biobank cardiovascular magnetic resonance substudy. [PDF]
Hu G +6 more
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Renal artery pulsatility index and myocardial performance index are not related with adverse perinatal outcome in late onset fetal growth restriction. [PDF]
Dur R, Eroglu H, Pektas MK, Yilmazer M.
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Hearing the Hoofbeats of Pheochromocytoma in New-Onset Cardiomyopathy Leads to Success Instead of Failure. [PDF]
Dimza M +4 more
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Space Science Reviews, 2006
A Brief History of CME Science.- Coronal Mass Ejections: Overview of Observations.- In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections.- An Introduction to CMEs and Energetic Particles.- An Introduction to Theory and Models of CMEs, Shocks, and Solar Energetic Particles.- An Introduction to the pre-CME Corona ...
H. Kunow +4 more
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A Brief History of CME Science.- Coronal Mass Ejections: Overview of Observations.- In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections.- An Introduction to CMEs and Energetic Particles.- An Introduction to Theory and Models of CMEs, Shocks, and Solar Energetic Particles.- An Introduction to the pre-CME Corona ...
H. Kunow +4 more
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Annual Review of Astronomy and Astrophysics, 1984
Sudden expulsions of dense clouds of plasma from the outer atmosphere of the Sun, termed "coronal mass ejections" (CMEs), are the focus of intense observational and theoretical efforts. CMEs are a type of coronal transient, the general name given the disruption of coronal structure.
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Sudden expulsions of dense clouds of plasma from the outer atmosphere of the Sun, termed "coronal mass ejections" (CMEs), are the focus of intense observational and theoretical efforts. CMEs are a type of coronal transient, the general name given the disruption of coronal structure.
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AIP Conference Proceedings, 2000
The most dramatic changes in the solar corona occur during coronal mass ejections, or CMEs, during which solar material is propelled outward into the heliosphere from regions in the corona not previously participating in the solar wind expansion. These ejections often produce major solar wind disturbances, large geomagnetic storms, enhancements of ...
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The most dramatic changes in the solar corona occur during coronal mass ejections, or CMEs, during which solar material is propelled outward into the heliosphere from regions in the corona not previously participating in the solar wind expansion. These ejections often produce major solar wind disturbances, large geomagnetic storms, enhancements of ...
openaire +1 more source

