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標(biāo)題: Titlebook: Helioseismic Diagnostics of Solar Convection and Activity; Thomas L. Duvall,John W. Harvey,Zdeněk ?vestka Book 2001 Springer Science+Busin [打印本頁]

作者: FERAL    時間: 2025-3-21 16:52
書目名稱Helioseismic Diagnostics of Solar Convection and Activity影響因子(影響力)




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書目名稱Helioseismic Diagnostics of Solar Convection and Activity網(wǎng)絡(luò)公開度學(xué)科排名




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書目名稱Helioseismic Diagnostics of Solar Convection and Activity讀者反饋




書目名稱Helioseismic Diagnostics of Solar Convection and Activity讀者反饋學(xué)科排名





作者: NATTY    時間: 2025-3-22 00:13
Peter A. Gilmanculations and, avoiding the condensed style frequently found in textbooks, explains these ideas without parsimony of words. The French edition in four volumes, published from 1998, has met with resounding success: the first two volumes are now available in English..978-3-540-20921-8978-3-540-29926-4Series ISSN 0172-5939 Series E-ISSN 2191-6675
作者: 進(jìn)步    時間: 2025-3-22 01:23
Alexander Ruzmaikinculations and, avoiding the condensed style frequently found in textbooks, explains these ideas without parsimony of words. The French edition in four volumes, published from 1998, has met with resounding success: the first two volumes are now available in English..978-3-540-20921-8978-3-540-29926-4Series ISSN 0172-5939 Series E-ISSN 2191-6675
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作者: Exposition    時間: 2025-3-22 18:54
G. H. Fisher,Y. Fan,D. W. Longcope,M. G. Linton,A. A. Pevtsovculations and, avoiding the condensed style frequently found in textbooks, explains these ideas without parsimony of words. The French edition in four volumes, published from 1998, has met with resounding success: the first two volumes are now available in English..978-3-540-20921-8978-3-540-29926-4Series ISSN 0172-5939 Series E-ISSN 2191-6675
作者: Lipoprotein    時間: 2025-3-22 22:46

作者: 類型    時間: 2025-3-23 02:09

作者: Arthritis    時間: 2025-3-23 09:36

作者: 依法逮捕    時間: 2025-3-23 13:40
C. Lindsey,D. C. Braunaluable suggestions for improvement, contributed essentially to the final version. We also extend great thanks to our staff for their careful perusal of the entire manuscript and for tracking errata and inaccuracies. Our most heartfelt thank extends again to our “typesetting perfectionist”, 1 withou
作者: triptans    時間: 2025-3-23 16:36

作者: 放縱    時間: 2025-3-23 21:22
Helioseismic Diagnostics of Solar Convection and Activity978-94-011-4377-6
作者: EVADE    時間: 2025-3-23 22:11
Book 2001e deep structure of large-scale convection and flows, emerging active regions, and sunspots. Along with the traditional ‘global‘ helioseismology based on frequencies of resonant oscillation modes, the local-area techniques have become increasingly important for studying the solar interior and the me
作者: 灰心喪氣    時間: 2025-3-24 06:11
ults on the deep structure of large-scale convection and flows, emerging active regions, and sunspots. Along with the traditional ‘global‘ helioseismology based on frequencies of resonant oscillation modes, the local-area techniques have become increasingly important for studying the solar interior and the me978-94-010-5882-7978-94-011-4377-6
作者: Osteons    時間: 2025-3-24 08:07
Can We Get the Bottom B?istribution of emerging photospheric magnetic fields can give us information about the magnetic field strength at the bottom of the convection zone. Distinguishing between the modes of emerging field requires simultaneous magnetic imaging of both sides of the Sun. Correlation of simultaneous Doppler
作者: 道學(xué)氣    時間: 2025-3-24 11:24
The Coupling of Solar Convection and Rotation (Invited Review)ut more recent investigations have begun to explore the distinct nature of turbulent convection. After a brief overview of empirical and numerical results on the related Rayleigh-Bernard system, I will outline the current state of numerical modeling of turbulent convection in rotating, stratified fl
作者: padding    時間: 2025-3-24 16:12
The Solar Dynamo and Emerging Flux (Invited Review)large poleward drift of active regions as they emerge. The time scale for emergence of an active region from the base of the convection zone to the surface is typically 2-4 months. The equatorial gap in the distribution of active regions has two possible origins; if the toroidal field strength is cl
作者: synovial-joint    時間: 2025-3-24 21:00
On the Twist of Emerging Flux Loops in the Solar Convection Zonelux tubes at the base of the solar convection zone. We find that: (1) In the northern hemisphere, a left-handed twist is generated in the flux tubes as a result of the right-handed tilt or writhe of the emerging loops induced by the Coriolis force. The generated twist increases with the latitude of
作者: 黃瓜    時間: 2025-3-24 23:11
Time-Distance Inversion Methods and Results (Invited Review) in January 1998, was studied from SOHO/MDI for eight days, both before and after its emergence at the surface. The results show a complicated structure of the emerging region in the interior, and suggest that the emerging flux ropes travel very quickly through the depth range of our observations. T
作者: SKIFF    時間: 2025-3-25 04:16
Acoustic Imaging of Solar Active Regions (Invited Review)s. The perturbed physical conditions caused by the magnetic fields of active regions manifest in these maps. The outgoing intensity is lower in magnetic regions than the quiet Sun. The group travel time and phase travel time are smaller in magnetic regions than in the quiet Sun. In this paper, we re
作者: 小官    時間: 2025-3-25 09:14
Basic Principles of Solar Acoustic Holography (Invited Review)epresents. Computational holography was proposed as the optimum approach whereby to address the severe diffraction effects that confront standard tomography in the solar .-mode environment. It has given us a number of remarkable discoveries in the last two years and now promises a new insight into s
作者: 博識    時間: 2025-3-25 12:08

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作者: 立即    時間: 2025-3-25 22:46
tics skilfully with didactical and historical considerations.Functions in R and C, including the theory of Fourier series, Fourier integrals and part of that of holomorphic functions, form the focal topic of these two volumes. Based on a course given by the author to large audiences at Paris VII Uni
作者: 不自然    時間: 2025-3-26 04:12

作者: 職業(yè)拳擊手    時間: 2025-3-26 05:39

作者: floaters    時間: 2025-3-26 12:00
Alexander Ruzmaikintics skilfully with didactical and historical considerations.Functions in R and C, including the theory of Fourier series, Fourier integrals and part of that of holomorphic functions, form the focal topic of these two volumes. Based on a course given by the author to large audiences at Paris VII Uni
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作者: arterioles    時間: 2025-3-26 19:22
Robert F. Stein,?ke Nordlundtics skilfully with didactical and historical considerations.Functions in R and C, including the theory of Fourier series, Fourier integrals and part of that of holomorphic functions, form the focal topic of these two volumes. Based on a course given by the author to large audiences at Paris VII Uni
作者: 雄辯    時間: 2025-3-26 22:59

作者: 熱情贊揚(yáng)    時間: 2025-3-27 04:30

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作者: cumulative    時間: 2025-3-27 13:05

作者: 緊張過度    時間: 2025-3-27 14:59
T. L. Duvall Jr.,L. Gizonese two volumes. Based on a course given by the author to large audiences at Paris VII University for many years, the exposition proceeds somewhat nonlinearly, blending rigorous mathematics skilfully with didactical and historical considerations. It sets out to illustrate the variety of possible app
作者: 我還要背著他    時間: 2025-3-27 17:48
A. C. Birch,A. G. Kosovichevtics skilfully with didactical and historical considerations.Functions in R and C, including the theory of Fourier series, Fourier integrals and part of that of holomorphic functions, form the focal topic of these two volumes. Based on a course given by the author to large audiences at Paris VII Uni
作者: 向下    時間: 2025-3-28 00:26
J. E. Rickett,J. F. Claerbouttics skilfully with didactical and historical considerations.Functions in R and C, including the theory of Fourier series, Fourier integrals and part of that of holomorphic functions, form the focal topic of these two volumes. Based on a course given by the author to large audiences at Paris VII Uni
作者: SEVER    時間: 2025-3-28 03:18
Gary H. Pricetics skilfully with didactical and historical considerations.Functions in R and C, including the theory of Fourier series, Fourier integrals and part of that of holomorphic functions, form the focal topic of these two volumes. Based on a course given by the author to large audiences at Paris VII Uni
作者: 并置    時間: 2025-3-28 07:46
Marcus Brüggen eine Funktion als einen Punkt in einem Funktionenraum anzusehen?.Zwei Problemkreise bildeten die treibende Kraft für die Entwicklung dieser Konzepte: Zum einen handelte es sich um Integralgleichungen der Form . für gegebene Funktionen . und rechte Seiten . mit dem Ziel, eine L?sung . zu finden. Zum
作者: 搜尋    時間: 2025-3-28 13:17
Jesper Munk Jensen,Bo Holm Jacobsen,J?Rgen Christensen-Dalsgaard eine Funktion als einen Punkt in einem Funktionenraum anzusehen?.Zwei Problemkreise bildeten die treibende Kraft für die Entwicklung dieser Konzepte: Zum einen handelte es sich um Integralgleichungen der Form . für gegebene Funktionen . und rechte Seiten . mit dem Ziel, eine L?sung . zu finden. Zum
作者: 偽書    時間: 2025-3-28 17:08
C. Lindsey,D. C. Braunutiful and well-grounded applications which connect broadly to many areas of mathematics. We of course hope that students will pursue this material independently; teachers may find it useful for undergraduate seminars. For an overview of the material presented, consult the table of contents and the
作者: Addictive    時間: 2025-3-28 20:34

作者: FLAIL    時間: 2025-3-29 02:00
D. C. Braun,C. Lindsey mathematicians (and very many practitioners) must have the skills to work with convex sets and functions, and extremal problems, since convexity continually crops up in the investigation of very diverse problems in mathematics and the natural sciences. It seems that some of the elements of convex a
作者: Resistance    時間: 2025-3-29 06:36

作者: 莊嚴(yán)    時間: 2025-3-29 11:03
Fluid Dynamics and MHD of the Solar Convection Zone and Tachocline: Current Understanding and Unsolvnetic structures; global convection and circulation; the rise of magnetic flux tubes to the photosphere, and their injection into the base of the convection zone; tachocline fluid dynamics and MHD; and the solar dynamo. We close with a set of observational’ targets’ for helioseismologists to aim for
作者: 高度贊揚(yáng)    時間: 2025-3-29 14:53

作者: jabber    時間: 2025-3-29 16:44
The Coupling of Solar Convection and Rotation (Invited Review) tremendous advances in high-performance computing technology, prompting increasingly sophisticated and realistic numerical models of solar convection. Among the most important helioseismic constraints on global-scale convection models is the mean differential rotation profile of the solar envelope,
作者: arboretum    時間: 2025-3-29 23:47
Realistic Solar Convection Simulationsate and radiative energy exchange. The simulation results are compared quantitatively with observations. Excellent agreement is obtained for the distribution of the emergent continuum intensity, the profiles of weak photospheric lines, the .mode frequencies, the asymmetrical shape of the mode veloci
作者: 驚呼    時間: 2025-3-30 00:08

作者: DEFT    時間: 2025-3-30 05:24

作者: 要素    時間: 2025-3-30 10:28
On the Twist of Emerging Flux Loops in the Solar Convection Zoneed by Longcope and Klapper, generalizing the original formulation for the dynamics of untwisted thin flux tubes by Spruit. The generalized formulation includes the description of torsional Alf vén waves and takes into account the coupling of the writhing motion of the tube axis to the change in the
作者: 明確    時間: 2025-3-30 14:45

作者: Locale    時間: 2025-3-30 19:13
Time-Distance Helioseismology With , Modes as a Method for Measurement of Near-Surface Flowsc field. Previous flow measurements of Doppler surface rotation, small magnetic feature rotation, supergranular pattern rotation, and surface meridional circulation have been confirmed. In addition, the flow in supergranules due to Coriolis forces has been measured. The spatial and temporal power sp
作者: 怪物    時間: 2025-3-30 23:11

作者: 清唱劇    時間: 2025-3-31 00:52
Calculation of the Sun’s Acoustic Impulse Response by Multi-dimensional Spectral Factorizationtion in one-dimensional space is Kolmogorov’s Fourier domain spectral-factorization method. The helical coordinate system maps two-dimensions to one. Likewise a three-dimensional volume is representable as a concatenation of many one-dimensional signals. Thus concatenating a cube of helioseismic dat
作者: 個人長篇演說    時間: 2025-3-31 05:08
Ray Travel Time and Distance for the Planar Polytropeound that an adiabatically stratified polytrope yields non-dispersed wave fields for a full circuit of a ray through a trapping region. Non-adiabacity, however, leads to dispersion, and a consequent loss of correlation with successive circuits of the trapping region. An acoustic waveguide with fixed
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作者: 的是兄弟    時間: 2025-3-31 14:11

作者: 蚊帳    時間: 2025-3-31 17:39
Acoustic Imaging of Solar Active Regions (Invited Review)t the solar surface. The constructed signals contain both intensity information and phase information. The intensity is computed by summing the squared amplitude of the constructed signal over time. The phase of constructed signals can be studied by the cross-correlation function between the time se
作者: Stress-Fracture    時間: 2025-3-31 21:42

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作者: Banquet    時間: 2025-4-1 06:42

作者: NOMAD    時間: 2025-4-1 10:16
Fluid Dynamics and MHD of the Solar Convection Zone and Tachocline: Current Understanding and Unsolvnetic structures; global convection and circulation; the rise of magnetic flux tubes to the photosphere, and their injection into the base of the convection zone; tachocline fluid dynamics and MHD; and the solar dynamo. We close with a set of observational’ targets’ for helioseismologists to aim for.
作者: 作繭自縛    時間: 2025-4-1 15:25

作者: 空洞    時間: 2025-4-1 20:11
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