Comment on “Explanation for MARFE formation and subsequent evolution into a detached symmetric plasma edge” [Phys. Plasmas 3, 2673 (1996)], “MARFE impurity density limits in tokamaks with poloidal asymmetry and rotation” [Phys. Plasmas 3, 3032 (1996)], and “MARFE suppression by external edge heating” [Phys. Plasmas 4, 134 (1997)]

1997 ◽  
Vol 4 (7) ◽  
pp. 2774-2775 ◽  
Author(s):  
A. De Ploey ◽  
R. A. M. Van der Linden ◽  
M. Goossens
Keyword(s):  
Plasma Edge ◽  
Subsequent Evolution ◽  
External Edge ◽  
Impurity Density

scholarly journals Investigation of turbulence rotation and radial electric field in the island divertor and plasma edge at W7-X

2019 ◽  
Vol 61 (5) ◽  
pp. 054003 ◽  
Author(s):  
A Krämer-Flecken ◽  
X Han ◽  
T Windisch ◽  
J Cosfeld ◽  
P Drews ◽  
...  
Keyword(s):  
Electric Field ◽  
Radial Electric Field ◽  
Plasma Edge

scholarly journals Severe tricuspid regurgitation 14 years after diagnosis of “transient neonatal tricuspid regurgitation”

Heart ◽  
2001 ◽  
Vol 86 (1) ◽  
pp. 88-90
Author(s):  
D Boshoff ◽  
L Mertens ◽  
M Gewillig
Keyword(s):  
Tricuspid Regurgitation ◽  
Neonatal Period ◽  
Clinical Course ◽  
Subsequent Evolution ◽  
Severe Tricuspid Regurgitation ◽  
Echocardiographic Examination ◽  
Long Term Follow Up ◽  
Transient Tricuspid Regurgitation

A 14 year old girl presented with severe tricuspid regurgitation after she was diagnosed with “transient tricuspid regurgitation of the newborn”. In the neonatal period she had presented with severe tricuspid regurgitation without an obvious underlying anatomical cause. This spontaneously regressed during the first months of life. She was dismissed from follow up at the age of 5 years after complete normalisation of the clinical and echocardiographic examination. The subsequent evolution and management of the patient, as well as the possible pathogenesis responsible for the unusual clinical course, is discussed. This case stresses the importance of long term follow up of patients with transient tricuspid regurgitation.

Investigation of plasma edge turbulence using a gas-puff imaging system in the reversed-field pinch device TPE-RX

2007 ◽  
Vol 49 (2) ◽  
pp. 129-143 ◽  
Author(s):  
R Cavazzana ◽  
G Serianni ◽  
P Scarin ◽  
M Agostini ◽  
N Vianello ◽  
...  
Keyword(s):  
Imaging System ◽  
Reversed Field Pinch ◽  
Plasma Edge ◽  
Reversed Field

scholarly journals A New View on Young Pulsars in Supernova Remnants: Slow, Radio-quiet & X-ray Bright

2000 ◽  
Vol 177 ◽  
pp. 699-702 ◽  
Author(s):  
E. V. Gotthelf ◽  
G. Vasisht
Keyword(s):  
Magnetic Field ◽  
Neutron Stars ◽  
Supernova Remnants ◽  
Simple Explanation ◽  
Crab Pulsar ◽  
Radio Pulsars ◽  
Substantial Fraction ◽  
Subsequent Evolution ◽  
X Ray ◽  
Field Decay

AbstractWe propose a simple explanation for the apparent dearth of radio pulsars associated with young supernova remnants (SNRs). Recent X-ray observations of young remnants have revealed slowly rotating (P∼ 10s) central pulsars with pulsed emission above 2 keV, lacking in detectable radio emission. Some of these objects apparently have enormous magnetic fields, evolving in a manner distinct from the Crab pulsar. We argue that these X-ray pulsars can account for a substantial fraction of the long sought after neutron stars in SNRs and that Crab-like pulsars are perhaps the rarer, but more highly visible example of these stellar embers. Magnetic field decay likely accounts for their high X-ray luminosity, which cannot be explained as rotational energy loss, as for the Crab-like pulsars. We suggest that the natal magnetic field strength of these objects control their subsequent evolution. There are currently almost a dozen slow X-ray pulsars associated with young SNRs. Remarkably, these objects, taken together, represent at least half of the confirmed pulsars in supernova remnants. This being the case, these pulsars must be the progenitors of a vast population of previously unrecognized neutron stars.

scholarly journals Radiation-Driven Stellar Eruptions

Galaxies ◽  
2020 ◽  
Vol 8 (1) ◽  
pp. 10 ◽  
Author(s):  
Kris Davidson
Keyword(s):  
Mass Loss ◽  
Radiation Pressure ◽  
Central Region ◽  
Massive Stars ◽  
Variable Stars ◽  
Blast Waves ◽  
Subsequent Evolution ◽  
Fundamental Causes ◽  
Radiative Output ◽  
Luminous Blue Variable

Very massive stars occasionally expel material in colossal eruptions, driven by continuum radiation pressure rather than blast waves. Some of them rival supernovae in total radiative output, and the mass loss is crucial for subsequent evolution. Some are supernova impostors, including SN precursor outbursts, while others are true SN events shrouded by material that was ejected earlier. Luminous Blue Variable stars (LBV’s) are traditionally cited in relation with giant eruptions, though this connection is not well established. After four decades of research, the fundamental causes of giant eruptions and LBV events remain elusive. This review outlines the basic relevant physics, with a brief summary of essential observational facts. Reasons are described for the spectrum and emergent radiation temperature of an opaque outflow. Proposed mechanisms are noted for instabilities in the star’s photosphere, in its iron opacity peak zones, and in its central region. Various remarks and conjectures are mentioned, some of them relatively unfamiliar in the published literature.

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