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The 20 cm radio continuum fluxes of 91 HII regions in a previously compiled catalog have been determined. The spectral types of the ionizing stars in 42 regions with known distances are estimated. These spectral types range from B0.5 to O7,…

星系天体物理 · 物理学 2018-11-27 A. P. Topchieva , M. S. Kirsanova , A. M. Sobolev

The heat flux mitigation during the Thermal Quench (TQ) by the Shattered Pellet Injection (SPI) is one of the major elements of disruption mitigation strategy for ITER. It's efficiency greatly depends on the SPI and the target plasma, and…

等离子体物理 · 物理学 2024-06-10 D. Hu , F. J. Artola , E. Nardon , M. Lehnen , M. Kong , D. Bonfiglio , M. Hoelzl , G. T. A. Huijsmans , JOREK Team

Purpose: To theoretically and experimentally study implant lead tip heating caused by radiofrequency (RF) power deposition in different wire configurations that contain loop(s). Methods: Maximum temperature rise caused by RF heating was…

医学物理 · 物理学 2024-12-20 Lydia J Bardwell Speltz , Seung-Kyun Lee , Yunhong Shu , Matt A Bernstein

Using a limited, but representative sample of sources in the ISM of our Galaxy with published spectra from the Infrared Space Observatory, we analyze flux ratios between the major mid-IR emission features (EFs) centered around 6.2, 7.7, 8.6…

天体物理学 · 物理学 2016-08-30 Nanyao Y. Lu

Infra-red (IR) thermography is an essential diagnostic tool for understanding the edge plasma behavior in fusion devices. In this work, we present a new in-house numerical tool, Functional Analysis of Heat Flux (FAHF), for IR thermographic…

Heavy (O+) ion energization and field-aligned motion in and near the ionosphere are still not well understood. Based on observations from the CASSIOPE Enhanced Polar Outflow Probe (e-POP) at altitudes between 325 km and 730 km over one…

Nonlinear simulation model for radio frequency (RF) waves in fusion plasmas has been developed and verified using fully kinetic ion and drift kinetic electron. Ion cyclotron motion in the toroidal geometry is implemented using Boris push in…

等离子体物理 · 物理学 2017-09-19 A. Kuley , Z. Lin , J. Bao , X. S. Wei , Y. Xiao , W. Zhang , G. Y. Sun , N. J. Fisch

The principal objective of this work is to report on the power coupled to a tungsten target in the Proto-MPEX device during oblique injection of a microwave beam (< 70 kW at 28 GHz) into a high-power (~100 kW at 13.56 MHz) over-dense…

等离子体物理 · 物理学 2022-01-10 J. F. Caneses Marin , C. L. Lau , R. H. Goulding , T. Bigelow , T. Biewer , J. B. O. Caughman , J. Rapp

Heat flux suppression in collisionless plasmas for a large range of plasma $\beta$ is explored using two-dimensional particle-in-cell simulations with a strong, sustained thermal gradient. We find that a transition takes place between…

高能天体物理现象 · 物理学 2018-11-14 G. T. Roberg-Clark , J. F. Drake , M. Swisdak , C. S. Reynolds

In the innermost regions of low-luminosity accretion flows, including Sgr A* at the center of our Galaxy, the frequency of Coulomb collisions is so low that the plasma is two-temperature, with the ions substantially hotter than the…

高能天体物理现象 · 物理学 2015-06-23 Lorenzo Sironi

The two-frequency heating technique was studied to increase the beam intensities of highly charged ions provided by the high-voltage extraction configuration (HEC) ion source at the National Institute of Radiological Sciences (NIRS). The…

等离子体物理 · 物理学 2015-01-29 S. Biri , A. Kitagawa , M. Muramatsu , A. G. Drentje , R. Rácz , K. Yano , Y. Kato , N. Sasaki , W. Takasugi

The possibility of using Infrared Lock-In Thermography (LIT) to estimate the thickness of a sample was assessed and shown to be accurate up to 1.8mm. LIT is a technique involving heating samples with halogen lamps with varying intensity…

应用物理 · 物理学 2018-10-15 Ming Hin Wong , Kok Hin Henry Goh

Turbulent transport is known to limit the plasma confinement of present-day optimized stellarators. To address this issue, a novel method to strongly suppress turbulence in such devices is proposed, namely the resonant wave-particle…

等离子体物理 · 物理学 2020-09-09 Alessandro Di Siena , Alejandro Banon Navarro , Frank Jenko

We show the evidence of ion-cyclotron dissipation mechanism in solar wind plasma using Helios data. From our statistical analysis we found that the wave power of high-frequency transverse waves (having frequencies between 0.01 and 1…

太阳与恒星天体物理 · 物理学 2010-09-27 Sofiane Bourouaine , Eckart Marsch , Fritz M. Neubauer

ITER's large and powerful neutral beam injection system is based on an ion source utilizing a modular concept, where eight cylindrical drivers are attached to one common expansion and extraction region. In each driver, a plasma is sustained…

等离子体物理 · 物理学 2022-11-21 Dominikus Zielke , Stefan Briefi , Ursel Fantz

The study examines the heating profile of hot solar transition region loops, particularly focusing on transient brightenings observed in IRIS 1400{\AA} slit-jaw images. The findings challenge the adequacy of simplistic, singular heating…

太阳与恒星天体物理 · 物理学 2024-05-15 Shah Mohammad Bahauddin , Stephen J Bradshaw

A fusion reactor requires plasma pre-heating before the rate of deuterium-tritium fusion reactions becomes significant. In ITER, radiofrequency (RF) heating of 3He ions, additionally puffed into the plasma, is one of the main options…

等离子体物理 · 物理学 2015-07-27 Y. O. Kazakov , J. Ongena , D. Van Eester , R. Bilato , R. Dumont , E. Lerche , M. Mantsinen , A. Messiaen

A load-tolerant External Conjugate-T (ECT) impedance matching system for two A2 Ion Cyclotron Resonance Heating (ICRH) antennas has been successfully put into operation at JET. The system allows continuous injection of the RF power into…

Time dependent numerical simulations of the K ALPHA complex of Fe XXV are carried out as a function of temperature/density/radiation field variations in high-temperature astrophysical and laboratory plasmas. In addition to several well…

天体物理学 · 物理学 2008-11-26 Justin Oelgoetz , Anil K. Pradhan

Multi-machine empirical scaling predicts an extremely narrow heat exhaust layer in future high magnetic field tokamaks, producing high power densities that require mitigation. In the experiments presented, the width of this exhaust layer is…