Origin and dynamics of solar magnetism (Record no. 18175)

MARC details
000 -LEADER
fixed length control field 02733nam a2200349Ia 4500
003 - CONTROL NUMBER IDENTIFIER
control field OSt
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20260115120135.0
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 220909b |||||||| |||| 00| 0 eng d
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9781441902382
037 ## - SOURCE OF ACQUISITION
Terms of availability Textbook
040 ## - CATALOGING SOURCE
Original cataloging agency CSL
Language of cataloging eng
Transcribing agency CSL
041 ## - LANGUAGE CODE
Language code of text/sound track or separate title eng
084 ## - COLON CLASSIFICATION NUMBER
Classification number B93 P9 TC
Assigning agency CSL
100 ## - MAIN ENTRY--PERSONAL NAME
Personal name Thompson, M. J.
9 (RLIN) 875800
245 #0 - TITLE STATEMENT
Title Origin and dynamics of solar magnetism
260 ## - PUBLICATION, DISTRIBUTION, ETC.
Place of publication, distribution, etc. Berlin,
Name of publisher, distributor, etc. Springer:
Date of publication, distribution, etc. 2009.
300 ## - PHYSICAL DESCRIPTION
Extent 428p.
Other physical details : col. ill.
490 ## - SERIES STATEMENT
Series statement Space sciences series of ISSI
500 ## - GENERAL NOTE
General note Includes bibliographical references.
520 ## - SUMMARY, ETC.
Summary, etc. Starting in 1995 numerical modeling of the Earth’s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of approximately the right strength, they show spatial power spectra similar to that of Earth, and the magnetic eld morphology and the temporal var- tion of the eld resembles that of the geomagnetic eld (Christensen and Wicht 2007). Some models show stochastic dipole reversals whose details agree with what has been inferred from paleomagnetic data (Glatzmaier and Roberts 1995; Kutzner and Christensen 2002; Wicht 2005). While these models represent direct numerical simulations of the fundamental MHD equations without parameterized induction effects, they do not match actual pla- tary conditions in a number of respects. Specically, they rotate too slowly, are much less turbulent, and use a viscosity and thermal diffusivity that is far too large in comparison to magnetic diffusivity. Because of these discrepancies, the success of geodynamo models may seem surprising. In order to better understand the extent to which the models are applicable to planetary dynamos, scaling laws that relate basic properties of the dynamo to the fundamental control parameters play an important role. In recent years rst attempts have been made to derive such scaling laws from a set of numerical simulations that span the accessible parameter space (Christensen and Tilgner 2004; Christensen and Aubert 2006).
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Astrophysics
9 (RLIN) 875801
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Extraterrestrial physics
9 (RLIN) 875802
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Planetology physics
9 (RLIN) 875803
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Space sciences
9 (RLIN) 875804
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Physics
9 (RLIN) 875805
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name Balogh, A
9 (RLIN) 875806
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name Culhane, J L
9 (RLIN) 875807
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name Nordlund, A
9 (RLIN) 875808
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name Solanki, S K
9 (RLIN) 875809
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Classification part B93 P9 TC
Koha item type Textbook
Source of classification or shelving scheme Colon Classification (CC)
Suppress in OPAC No
Holdings
Withdrawn status Lost status Source of classification or shelving scheme Damaged status Not for loan Home library Current library Date acquired Source of acquisition Total Checkouts Full call number Barcode Date last seen Price effective from Koha item type
    Colon Classification (CC)     Central Science Library Central Science Library 2022-09-12 319, 26/02/2010, N R Book Distributors   B93 P9 TC SL1446762 2022-09-12 2022-09-12 Textbook
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