標(biāo)題: Titlebook: Dynamics of the Sun and Stars; Honoring the Life an Mário J. P. F. G. Monteiro,Rafael A. García,Scott Conference proceedings 2020 The Edit [打印本頁] 作者: Remodeling 時間: 2025-3-21 19:42
書目名稱Dynamics of the Sun and Stars影響因子(影響力)
書目名稱Dynamics of the Sun and Stars影響因子(影響力)學(xué)科排名
書目名稱Dynamics of the Sun and Stars網(wǎng)絡(luò)公開度
書目名稱Dynamics of the Sun and Stars網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Dynamics of the Sun and Stars被引頻次
書目名稱Dynamics of the Sun and Stars被引頻次學(xué)科排名
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書目名稱Dynamics of the Sun and Stars讀者反饋學(xué)科排名
作者: 滔滔不絕的人 時間: 2025-3-21 20:13
Assessing the Threat of Major Outbreaks of Vector-Borne Diseases Under a Changing Climatepresent results from a collaboration that was set up following Michael’s untimely death in October 2018, between climate scientists (Jim Hurrell and Lantao Sun) and mathematical epidemiologists (Robin Thompson and Uri Obolski). Specifically, we propose a framework for studying the effect of climate 作者: 反感 時間: 2025-3-22 04:22 作者: antidote 時間: 2025-3-22 04:55
1570-6591 becoming feasible. Combining observations, seismic analysis, and modelling the meeting and this book serve as a fitting memorial to a close colleague and friend, much missed..978-3-030-55338-8978-3-030-55336-4Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: Nibble 時間: 2025-3-22 12:48
https://doi.org/10.1007/978-1-4612-5823-0present results from a collaboration that was set up following Michael’s untimely death in October 2018, between climate scientists (Jim Hurrell and Lantao Sun) and mathematical epidemiologists (Robin Thompson and Uri Obolski). Specifically, we propose a framework for studying the effect of climate 作者: instulate 時間: 2025-3-22 13:10 作者: instulate 時間: 2025-3-22 19:30
Dynamics of the Sun and Stars978-3-030-55336-4Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: COKE 時間: 2025-3-23 01:13 作者: Canyon 時間: 2025-3-23 02:00 作者: 膝蓋 時間: 2025-3-23 05:56 作者: 新鮮 時間: 2025-3-23 10:09 作者: infatuation 時間: 2025-3-23 17:25 作者: INCUR 時間: 2025-3-23 18:30 作者: 蛤肉 時間: 2025-3-24 02:09
On Solar and Solar-Like Stars Convection, Rotation and Magnetismibutions have impacted or challenged the current state of our understanding and guided the development of advanced numerical simulations of the magnetohydrodynamics (MHD) of the Sun and Sun-like stars.作者: atopic-rhinitis 時間: 2025-3-24 03:42 作者: 詞根詞綴法 時間: 2025-3-24 06:57 作者: LIMN 時間: 2025-3-24 12:38
Writing Patient Education Materialsw ideas. He spent six years in Sheffield after being appointed as the Head of Applied Mathematics Department in the University of Sheffield (UK) where colleagues hold fond memories of him, both as a committed academic and a very effective leader. His hard work and sincere approach was infectious to 作者: Rankle 時間: 2025-3-24 15:09 作者: 使習(xí)慣于 時間: 2025-3-24 20:30 作者: Diatribe 時間: 2025-3-25 01:40
Response to Bryan and Beauchampeismic data forthcoming from the GONG, MDI (on SOHO) and HMI (on SDO) observational projects. This has enabled major discoveries about the internal differential rotation of the Sun, revealing both a tachocline of shear at the base of its convection zone and a near-surface shear layer near its surfac作者: Morose 時間: 2025-3-25 06:12 作者: HALO 時間: 2025-3-25 08:26 作者: Free-Radical 時間: 2025-3-25 14:19 作者: Affable 時間: 2025-3-25 19:32 作者: lanugo 時間: 2025-3-25 21:30
Michael Indergaard,Michael CushionTime-distance helioseismic studies of the deep structure of MC, however, have yielded conflicting inferences. Here, following a summary of existing results we show how a large center-to-limb systematics (CLS) in the measured travel times of acoustic waves affects the inferences through an analysis o作者: Condescending 時間: 2025-3-26 03:03
Developments in Hematology and Immunologyrather easily. Here we show the result of the measurement of rotation periods for a large number of . solar-like stars along with their level of magnetic activity. We also study solar-like stars for which oscillations have not been detected using 1 month of . data in order to understand what can be 作者: 樹木心 時間: 2025-3-26 04:47
Platelet Functions and Platelet Transfusionrted in time–distance helioseismic measurements. Meanwhile, another travel-time asymmetry between waves traveling away from and into sunspots is well known. It is possible that both of the travel-time asymmetries are partially, albeit not entirely, due to different atmospheric heights where oscillat作者: subacute 時間: 2025-3-26 11:29 作者: Canopy 時間: 2025-3-26 13:38
https://doi.org/10.1007/978-1-4613-3458-34). Optimization procedures that rely on matrix inversions may suffer from numerical instabilities caused by ill-conditioned matrices. Markov Chain Monte Carlo (MCMC) methods sample the parameter space, independent of its complexity, while Bayesian methods are powerful ways of of understanding the p作者: Vertical 時間: 2025-3-26 18:53 作者: 脆弱么 時間: 2025-3-27 00:03
https://doi.org/10.1007/978-3-030-55336-4Michael J; Thompson; Measuring stellar oscillations - Asteroseismology; Measuring solar oscillations -作者: 連累 時間: 2025-3-27 02:37 作者: 運動吧 時間: 2025-3-27 06:11 作者: Diuretic 時間: 2025-3-27 09:58 作者: interrupt 時間: 2025-3-27 17:24
MichaelI was very sorry that I could not attend the conference to help celebrate Michael’s life. I certainly would have come had I been able.作者: 盡忠 時間: 2025-3-27 18:58 作者: justify 時間: 2025-3-28 01:27
Michael Thompson’s Legacy in Solar and Stellar Physicsrch pioneer in the field of solar and stellar astrophysics and as an administrator who held major leadership positions in the UK and the USA. In this review we summarize his outstanding contributions to research.作者: Explosive 時間: 2025-3-28 03:34 作者: Water-Brash 時間: 2025-3-28 06:24
Michael J. Thompson: A Remarkable Scientist, Leader, and Friends that Michael J. Thompson passed away unexpectedly. Michael was an outstanding solar physicist, known for his exceptional accomplishments in advancing the understanding of the structure and dynamics of the solar interior. Michael was an internationally recognized leader in the field of helioseismol作者: Aromatic 時間: 2025-3-28 13:20
Assessing the Threat of Major Outbreaks of Vector-Borne Diseases Under a Changing Climateo, where he was also a Senior Scientist. In September 2013, Michael became the Deputy Director and Chief Operating Officer of NCAR, enjoying a very close working relationship with Director Jim Hurrell. During this time, Michael oversaw an organisation conducting research in a range of fields, includ作者: 首創(chuàng)精神 時間: 2025-3-28 15:45 作者: 祖?zhèn)髫敭a(chǎn) 時間: 2025-3-28 20:50
Uncovering the Hidden Layers of the Sunve allowed us to determine the structure of the inner layers of the Sun. This in turn has led to tests of solar models, and perhaps more importantly, tests of the properties of stellar material. I review some of the interesting results that helioseismic structure inversions have revealed and how tod作者: gustation 時間: 2025-3-29 02:56
Solar Rotationt challenged modellers—such as the nearly-radial profile of the lines of constant rotation in the convection zone, the thin shear layer or tachocline at its base, and the nearly-rigid rotation in the radiative interior. This review will highlight Michael Thompson’s important contributions to techniq作者: DECRY 時間: 2025-3-29 05:45 作者: 綠州 時間: 2025-3-29 10:09 作者: upstart 時間: 2025-3-29 14:54
Time-Distance Helioseismology of Deep Meridional CirculationTime-distance helioseismic studies of the deep structure of MC, however, have yielded conflicting inferences. Here, following a summary of existing results we show how a large center-to-limb systematics (CLS) in the measured travel times of acoustic waves affects the inferences through an analysis o作者: 豐富 時間: 2025-3-29 16:07
Surface Rotation and Magnetic Activity of Solar-Like Stars: Impact on Seismic Detectionsrather easily. Here we show the result of the measurement of rotation periods for a large number of . solar-like stars along with their level of magnetic activity. We also study solar-like stars for which oscillations have not been detected using 1 month of . data in order to understand what can be 作者: 多嘴 時間: 2025-3-29 22:35 作者: 省略 時間: 2025-3-30 03:34 作者: 使激動 時間: 2025-3-30 05:57
New Inversion Scheme for Time-Distance Helioseismology4). Optimization procedures that rely on matrix inversions may suffer from numerical instabilities caused by ill-conditioned matrices. Markov Chain Monte Carlo (MCMC) methods sample the parameter space, independent of its complexity, while Bayesian methods are powerful ways of of understanding the p作者: GRIN 時間: 2025-3-30 10:07 作者: AMEND 時間: 2025-3-30 12:38
https://doi.org/10.1007/978-1-4612-5248-1cument. Dynamics of the Sun & Stars: Honoring the Life & Work of Michael Thompson was a wonderful gathering of Michael’s family, friends and colleagues to discuss the science that was his passion and to commemorate his many professional achievements.作者: paroxysm 時間: 2025-3-30 19:42
Workers, Managers, and Technological Changervations but which helioseismology reveals to penetrate deep into the convection zone. Finally, I briefly mention the collaborative effort that was initiated by Michael in 2017 with the aim of taking advantage of more than twenty years of high-quality helioseismic observations to refine our picture of the interior rotation profile.作者: Fantasy 時間: 2025-3-30 21:41 作者: NEX 時間: 2025-3-31 04:04 作者: inhibit 時間: 2025-3-31 08:47 作者: 羞辱 時間: 2025-3-31 09:22 作者: Bmd955 時間: 2025-3-31 16:46
Surface Rotation and Magnetic Activity of Solar-Like Stars: Impact on Seismic Detectionstic activity. We also study solar-like stars for which oscillations have not been detected using 1 month of . data in order to understand what can be the reason behind these non-detections. Surprisingly the conclusion of our analysis is that magnetic activity is not the main reason for not detecting acoustic modes in those stars.作者: 混雜人 時間: 2025-3-31 19:31
Michael Indergaard,Michael Cushionf frequency dependence of CLS, using data from the Helioseismic and Doppler Imager (HMI) onboard Solar Dynamics Observatory (SDO). Our results point to the residual systematics in travel times as a major cause of differing inferences on the deep structure of MC.
