/ Physics of the Earth and Planetary Interiors 173 (2009) 33–50 35 2. 1. On Earth, the elastic thickness is controlled by the depth of the 450°C isotherm (Watts, 1994). It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. 116 W. Landuyt, D. Bercovici / Physics of the Earth and Planetary Interiors 175 (2009) 115–126 ation of localization mechanisms across the lithosphere is evident in experimentally inferred transitions in deformation mechanisms with depth (Kohlstedt et al., 1995). 1). the Earth’s and other planetary interiors is critical for understand-ingthe thermalhistoryand dynamicsof the core andmantle. / Physics of the Earth and Planetary Interiors 182 (2010) 187–198 189 2. Ziegler et al. / Physics of the Earth and Planetary Interiors 168 (2008) 71–87 73 Fig. Sitemap. K. Lawrence et al. Read the latest articles of Physics of the Earth and Planetary Interiors at ScienceDirect.com, Elsevier’s leading platform of peer-reviewed scholarly literature Paleointensity versus age for lunar samples (a) reproduced from Cisowski et al. Both studies involved sections from the northwestern part of the forma-tion, and have indicated low virtual dipolar moments (2.2 ± 0.9 1022 Am2 and 2.9 ± 2.3 1022 Am2, respectively). Li, S. Zhong / Physics of the Earth and Planetary Interiors 176 (2009) 143–156 145 Fig. Physics of the Earth and Planetary Interiors 281 (2018) 68–78 69. earthquake sources, the modes 0S 0and 10S are particularly suited to this inversion, since the two excitation coefficients are comparable for 10S (10KN=− =−0.094; 0.11 Klemperer on 18 December 2007, but labels given here are original and used for reference in the text of this paper. 218 C. Beggan, K. Whaler / Physics of the Earth and Planetary Interiors 167 (2008) 217–222 one-norm minimisation inversion technique, initially imposing a minimumglobalroot-mean-square(RMS)flowvelocityconstraint. 3. M.W.L. About Physics of The Earth and Planetary Interiors Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary … B. Romanowicz, H.-R. Wenk/Physics of the Earth and Planetary Interiors 269 (2017) 58–90 59. Z and Z are the real and imaginary part of complex impedance respectively. Kennett / Physics of the Earth and Planetary Interiors 167 (2008) 84–97 85 Fig. (1983) where samples measured using Thellier–Thellier (closed circle), Shaw (open https://doi.org/10.1016/j.pepi.2021.106654, https://doi.org/10.1016/j.pepi.2021.106652, https://doi.org/10.1016/j.pepi.2021.106651, https://doi.org/10.1016/j.pepi.2020.106638, https://doi.org/10.1016/j.pepi.2019.106325, High-pressure vibrational spectra of humite-group minerals: Fluorine effect on thermodynamic properties and hydrogen bonds, Erratum to “The influence of spreading rate and permeability on melt focusing beneath mid-ocean ridges” [Physics of the Earth and Planetary Interiors 304 (2020) 106486], 3-D time-domain electromagnetic modeling based on multi-resolution grid with application to geomagnetically induced currents, MAGLAB: A computing platform connecting geophysical signatures to melting processes in Earth's mantle, Extremely young melt infiltration of the sub-continental lithospheric mantle, Geller-Fest Workshop on Big Data in Geosciences: From Earthquake Swarms to Consequences of Slab Dynamics, Physical properties and observations of the lithosphere-asthenosphere system, Variations of the Earth’s magnetic field as revealed by archaeological baked clays: contribution of archaeomagnetism to geomagnetism and archaeology. The work focuses on how the different modes of damage (i.e. Bower Physics of the Earth and Planetary Interiors 278 (2018) 59–74 60. / Physics of the Earth and Planetary Interiors 176 (2009) 109–123 113 Tilik Volcano is the main Fentale volcanic edifice and it is the major central volcano in this magmatic segment. It can be seen that this phase is vibrationally stable to pressures well beyond that of the inner core; however, it is Please click here for more information on our author services. 36 L.B. A.L. Looking for an author or a specific volume/issue? Geodynamic models are necessary to suggest realistic deforma-tion paths. Each trace is aligned to manually picked PKIKP (t=0). / Physics of the Earth and Planetary Interiors 173 (2009) 33–50 35 2. Goncharov et al. Check the Author information pack on Elsevier.com 1. various types of finite frequency effects. / Physics of the Earth and Planetary Interiors 170 (2008) 34–45 Fig. Miller, F. Niu / Physics of the Earth and Planetary Interiors 170 (2008) 89–94 91 Fig. Thanks in advance for your time. Tectonic setting Hainan island is located near the southeastern margin of the Eurasian plate, and has been affected by the motions and interac-tion of the Indian and Philippine Sea plates and by the extension of the South China Sea basin (Fig. 142 C. Xuan, J.E.T. Okal Physics of the Earth and Planetary Interiors 274 (2018) 37–48 38. Karato / Physics of the Earth and Planetary Interiors 176 (2009) 83–88 85 Fig. / Physics of the Earth and Planetary Interiors 176 (2009) 198–212 199 Fig. K. Key, S. Constable / Physics of the Earth and Planetary Interiors 184 (2011) 194–207 195 was ubiquitous throughout the ocean basins. Physics of the Earth and Planetary Interiors 110 1999 83–93 . If you decide to participate, a new browser tab will open so you can complete the survey after you have completed your visit to this website. Sofia Akber. Please feel free to … PHYSICS OF THE EARTH AND PLANETARY INTERIORS A JOURNAL DEVOTED TO OBSERVATIONAL AND EXPERIMENTAL STUDIES OF THE CHEMISTRY AND PHYSICS OF PLANETARY INTERIORS AND THEIR THEORETICAL INTERPRETATION related ISSN: 1872-7395 Country: Netherlands. Phonon dispersion relations for the omega phase. Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. 35 Full PDFs related to this paper . Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. 3. Publisher country is Netherlands. / Physics of the Earth and Planetary Interiors 182 (2010) 129–138 131 finite-elementconvectioncodeCitcomS(Zhongetal.,2000)tosolve an instantaneous Stokes flow calculation for a whole-mantle con- Copyright © 2021 Elsevier B.V. or its licensors or contributors. Hochsimmer (SI) and Hochstein (HS) an additional, unoriented hand sample was taken due to drilling difficulties (SI) and the suspected likelihood of past lightning strikes at the only in situ outcrop (HS). Ziegler et al. Red (purple) values show areas with a high (low) K. Lawrence et al. / Physics of the Earth and Planetary Interiors 174 (2009) 159–164 161 Fig. Mineral Physics of Earth and Planetary Interiors . A.F. J.M. ⇑ Corresponding author at: Department of Earth and Planetary Science, University of California at Berkeley, United States. They derive this expression using the variational perturbation method for hard spheres (Mansoori and Canfield, 1969). T. Höink et al./Physics of the Earth and Planetary Interiors 221 (2013) 22–26 23. In a previous paper (Miyagi et al., 2006), we presented texture and stress analysis using the Rietveld method with data measured on a single image at 49.3GPa. Thus, when we look at the interior of the Earth from the surface, we are faced with a situation where clear indications of anisotropy could arise from intrinsic effects such as LPO, or be apparent, rep- Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. This paper. 2. Tectonic setting Hainan island is located near the southeastern margin of the Eurasian plate, and has been affected by the motions and interac-tion of the Indian and Philippine Sea plates and by the extension of the South China Sea basin (Fig. please, Physics of the Earth and Planetary Interiors. PDF. We also take into consider-ation the relative contribution of the modes to the total surface Physics of the Earth and Planetary Interiors 269 (2017) 58–90 Contents lists available at ScienceDirect Physics of the Earth and Planetary Interiors L. Dai, S.-i. A Z versus Z plot of complex impedance of hydrous garnet from 10−2 to 106 Hz (right to left), obtained under conditions of 8.0GPa, 873–1273K and 0.0046wt% water content. A similar isotherm exists beneath the lunar lithosphere (Crosby and McKenzie, 2005). / Physics of the Earth and Planetary Interiors 182 (2010) 113–118 115 Table 1a Unit-cell parameters and unit-cell volume for CaPtO3 at ambient pressure and temperature; the numbers in parentheses are estimated standard uncertainties and refer to the least-significant digits. This process releases First Previous Next Last (0/0) Start your review of [PHYSICS OF THE EARTH AND PLANETARY INTERIORS]: Your review informs others about the journal. Subject: PHYSICS AND SPACE SCIENCES; GEOLOGY AND EARTH SCIENCES. Physics of the Earth and Planetary Interiors 274 (2018) 148–157 149. Box 1028 Blindern, N-0315 Oslo, Norway d GFZ German Research Centre for Geosciences, Telegraphenberg, D-14473 Potsdam, Germany e Mineral Physics Institute, Department of Earth and Space Sciences, Stony Brook University, Stony Brook, New York, USA / Physics of the Earth and Planetary Interiors 173 (2009) 207–215 209 Table 1 Corralitos logbook entries verbatim from a spreadsheet supplied by D. Culp and S.L. (2011), doi:10.1016/ j.pepi.2011.04.011. Benefits to authors We also provide many author benefits, such as free PDFs, a liberal copyright policy, special discounts on Elsevier publications and much more. A. Wüstefeld et al. A.S. Wolf, D.J. 1. We use cookies to help provide and enhance our service and tailor content and ads. Physics of the Earth and Planetary Interiors. 1. Cookie Settings, Terms and Conditions Free PDF. N. Saloor, E.A. Physics of the Earth and Planetary Interiors 285 (2018) 76–90 77. here it is solved using a particle method (e.g., Tackley and King, 2003), similarly to how the compositional field is modeled in mantle convec-tion studies (McNamara and Zhong, 2004). Earth’s time-variable gravity field and to measure mass redistribution, such as terrestrial water storage and Earth Rotation excitation (Jin and Feng, 2013; Jin et al., 2011; Jin and Zhang, 2012), ice sheet mass balance and sea level change (Jin et al., 2016; Jin and Zou, 2015). If you wish to place a tax exempt order J. Lei et al. The scope of Physics of the Earth and Planetary Interiors covers Physics and Astronomy (miscellaneous) (Q1), Astronomy and Astrophysics (Q2), Geophysics (Q2), Space and Planetary Science (Q2) . cCentre for Earth Evolution and Dynamics (CEED), University of Oslo, P.O. A short summary of this paper. PDF. Earth Planet. / Physics of the Earth and Planetary Interiors 174 (2009) 159–164 was made. 1A). It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. 180 K. Otsuka et al. Monster et al. Download PDF Package. / Physics of the Earth and Planetary Interiors 180 (2010) 179–188 (MgFe2O4), which is likely different from the more reduced con- ditions inferred for the lower mantle (e.g., Frost and McCammon, 2008). Z.-X. Squares indicate the first arrival of the PKIKP precursors estimated from a random scattering model. The time convolution arises from the fact that μ B in Eq. The scientific journal Physics of the Earth and Planetary Interiors is included in the Scopus database. Carcione et al. Gerd Steinle-neumann. The Murray Basin and other Cenozoic deposits obscure much of the underlying Palaeozoic basement. Premium PDF Package. Earth’s time-variable gravity field and to measure mass redistribution, such as terrestrial water storage and Earth Rotation excitation (Jin and Feng, 2013; Jin et al., 2011; Jin and Zhang, 2012), ice sheet mass balance and sea level change (Jin et al., 2016; Jin and Zou, 2015). a Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD 21218, USA bDepartment of Physics, University of Colorado, Boulder, CO 80309, USA article info Article history: Received 25 April 2012 Receivedin revised form20September 2012 Accepted 7 October 2012 Available online xxxx Edited by Chris Jones Keywords: Geodynamo Mantle convection Polarity reversals … Download Full PDF Package. Thus, previous studies on transport properties commonly coming from the collision in Eastern Anatolia (Reilinger et al., 2006; Bulut et al., 2012). 2. d-Spacings vs. angle between the diffracting plane normal and the maximum stress axis at 49.3GPa. (a) SMEAN shear wave velocity anomalies near the core–mantle boundary (Becker and Boschi, 2002), illustrating the location and lateral extent of the present African (A) An example of PKIKP precursors and PKIKP/PKiKP phases observed at northern South America and the southeastern Caribbean. E.A. Physics of the Earth and Planetary Interiors is a peer-reviewed scientific journal. Besides, GRACE observations have improved our understanding of the / Physics of the Earth and Planetary Interiors 174 (2009) 24–32 27 monochromator-spectrograph with CCD detector in UV–vis and by FT-IR spectrometer (Nicolet 750 Magna) equipped by a halo- gen lamp and a CaF2 beamsplitter for near IR spectral range. Physics of the Earth and Planetary Interiors - Editorial Board. (1983) where samples measured using Thellier–Thellier (closed circle), Shaw (open circle) and ARM (×) techniques are labeled with associated sample number. Sign in to view your account details and order history, Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. / Physics of the Earth and Planetary Interiors 180 (2010) 179–188 (MgFe2O4), which is likely different from the more reduced con-ditions inferred for the lower mantle (e.g., Frost and McCammon, 2008). Editors Professor Vernon Cormier. The Standard Abbreviation (ISO4) of Physics of the Earth and Planetary Interiors is “Phys. Gerd Steinle-neumann. No sample adjustment is necessary when changing the spectral range. Early models assumed flow in an isotropic medium dri-ven by temperature and density gradients (e.g. The stress-strain relations are written in the particle-velocity/stress formulation, which is suitable to perform numerical simulations. Inter.” . In. 1. Copyright © 2021 Elsevier B.V. All rights reserved. A.F. ScienceDirect ® is a registered trademark of Elsevier B.V. ScienceDirect ® is a registered trademark of Elsevier B.V. Hager and O’Connell, 1981; Tackley, 1993; Bunge et al., 1996). i.e. 3. Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader. We cannot process tax exempt orders online. In our particle-based method, the fineness field Ais represented by a distribution of particles. PDF. E-mail address: barbara@seismo.berkeley.edu (B. Romanowicz). M.S. The co-editors are G. Helffrich (University of Bristol), K. Hirose (Tokyo Institute of Technology), M. Jellinek (University of British Columbia), and K. Zhang (University of Exeter). We assume that each of Earth’s plates operates in either the sluggish-lid or the mobile-lid mode. Poloidal-only flows were also examined, for completeness, throw- Physics of the Earth and Planetary Interiors ... As the Earth cools, material from the liquid outer core crystallises onto the surface of the inner core at a rate of about 0.3mm/year (Jacobs, 1953; Labrosse et al., 2001; Aubert et al., 2008). University College London, London, United Kingdom Email Dr. ana Ferreira, PhD. The main subject areas of published articles are Space and Planetary Science, Geophysics, Astronomy and Astrophysics, Physics and Astronomy (miscellaneous). Besides, GRACE observations have improved our understanding of the Bull et al. / Physics of the Earth and Planetary Interiors 168 (2008) 71–87 73 Fig. J.N. A. Lindsay-Scott et al. N. Rawlinson, B.L.N. Academic field: PHYSICS … (a) Global distribution of 0–1Ma absolute paleointensity plotted as a probability distribution function on a log scale. 54 L. Vocadlo et al. Box 1028 Blindern, N-0315 Oslo, Norway d GFZ German Research Centre for Geosciences, Telegraphenberg, D-14473 Potsdam, Germany e Mineral Physics Institute, Department of Earth and Space Sciences, Stony Brook University, Stony Brook, New York, USA Download PDF. E. Font et al. PDF. Kanani Lee. Geological settings and sampling Relics of the Tsunami generated by the 1755 Lisbon earthquake, magnitude 8.5–8.75 (e.g., Abe, 1979; Johnston, 1996), were found in the Algarve region, southern Portugal (Hindson and Andrade, 1999), in the estuary of the Boca do Rio (Fig. Based on 2018, SJR is 2.173. / Physics of the Earth and Planetary Interiors 170 (2008) 34–45 37 et al., 2000). Cookie Notice L. Miyagi et al. The same setup can be used for the … 1). 160 L. Miyagi et al. 2 P. Olson/Physics of the Earth and Planetary Interiors xxx (2011) xxx–xxx Please cite this article in press as: Olson, P. Laboratory experiments on the dynamics of the core. Substantial efforts were made by the planetary science community to adapt these techniques to multi-anvil apparatus, and pressures up to 20 GPa were reached (see for instance Osako et al., 2004;Katsura, 1993Katsura, , 1995Katsura, ,1997Xu et al., 2004).Static experiments at substantially higher pressure require use of DACs. 1. Thick solid lines is recalculated from the Rietveld refinement with C12 or C44 refined. Our new study presents the … Based on 2018, SJR is 2.173. Channell / Physics of the Earth and Planetary Interiors 169 (2008) 140–151 Table 1 Location, water depth, length, sedimentation rate, normalizer, and estimated age for relative paleointensity records used in this study Records Location Water depth (m) Record length (m) Sedimentation rate (cm/kyr) Normalizer used Oldest age (Ma) References ODP 983 60.40N, 23.64W … / Physics of the Earth and Planetary Interiors 170 (2008) 52–59ˇ Fig. Schematic map of the southern Tasman Orogen in eastern Australia. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. Kanani Lee. We are always looking for ways to improve customer experience on Elsevier.com. Open circles were extracted from the diffraction spectra using single peak fitting. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. University of Connecticut, Storrs, Connecticut, United States Email Professor Vernon Cormier. A number of experimental high-pressure techniques, including ultrasonic interferometry, nuclear resonant inelastic X-ray scatter-ing (NRIXS), high-energy resolution inelastic X-ray scattering Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. The main subject areas of published articles are Space and Planetary Science, Geophysics, Astronomy and Astrophysics, Physics and Astronomy (miscellaneous). You may choose to submit your manuscript as a single Word or PDF file to be used in the refereeing process. By continuing you agree to the use of cookies. physics and geochemistry of the Earth’s core as well as the interi-ors of other planetary bodies (Sohl and Schubert, 2007). Get more information about 'Physics of the Earth and Planetary Interiors'. cCentre for Earth Evolution and Dynamics (CEED), University of Oslo, P.O. Goncharov et al. 2 E. Türkog˘lu et al./Physics of the Earth and Planetary Interiors 241 (2015) 1–14. Replacing (8) with (10) and adding the contribution of S-wave ra-diation at the source, the estimated energy EE is then defined as: = E +〈 〉q ∗ π F F ε 1 4 () E . Please see our Guide for Authors for information on article submission. Privacy Policy experiment by adding a small amount of hydrochloric acid. Paleointensity versus age for lunar samples (a) reproduced from Cisowski et al. Earth Planet. period of the Earth’s magnetic field based on previous work. / Physics of the Earth and Planetary Interiors 182 (2010) 113–118 115 Table 1a Unit-cell parameters and unit-cell volume for CaPtO3 at ambient pressure and temperature; the numbers in parentheses are estimated standard uncertainties and refer to the least-significant digits. T. Kidane et al. Physics of the Earth and Planetary Interiors. These are all of direct relevance for planetary accretion and differen-tiation processes (Stevenson, 1990), the time evolution of mantle and core temperatures (Stacey and Loper, 1984), and the gen- Personal information is secured with SSL technology. Download Free PDF. Okal et al. We would like to ask you for a moment of your time to fill in a short questionnaire, at the end of your visit. Gravitational energy of core evolution: implications for thermal history and geodynamo power Frank D. Stacey a,), Conrad H.B. The scientific journal Physics of the Earth and Planetary Interiors is included in the Scopus database. If you require any further information or help, please visit our Support Center, Copyright © 2021 Elsevier, except certain content provided by third parties, Cookies are used by this site. emplaced. Read the latest articles of Physics of the Earth and Planetary Interiors at ScienceDirect.com, Elsevier’s leading platform of peer-reviewed scholarly literature Before mixing these material types into a larger com-pilation, results obtained from the different material types should be quantitatively compared. The method involves frequency-dependent filtering and weighting, and the phase veloc-ity curve is interactively selected in the frequency domain. Physics of the Earth and Planetary Interiors, established in October 1967, is a biweekly peer-reviewed scientific journal published by Elsevier. With the rapid advances of the past decade in ultrahigh-pressure x-ray synchrotron technology, researchers are now able to tackle some of the most fundamental, long-standing questions regarding Earth and planetary interiors. Sofia Akber. Physics of the Earth and Planetary Interiors: Phase Transformations and the Earth's Interior v. 3: Symposium Proceedings: Ringwood, A.E., Green, D. H.: Amazon.nl ) 159–164 161 Fig Corresponding author at: Department of Earth ’ s plates operates in either the or! Labels given here are original and used for reference in the frequency domain physical! May choose to submit your manuscript as a probability distribution function on a log scale 174. 14–22 15. the symbol “ ∗ ” denotes time convolution arises from the refinement! Be used for the … ccentre for Earth Evolution and Dynamics ( CEED ), University Connecticut. Interiors ' 167 ( 2008 ) 71–87 73 Fig Physics … A.S.,. Is interactively selected in the Scopus database this expression using the variational perturbation method for spheres. That μ B in Eq your manuscript as a single Word or PDF file to be entirely to!, University of Oslo, P.O this Paper and tailor content and ads we use cookies to help and... Information about 'Physics of the Earth and Planetary Interiors 274 ( 2018 ) 37–48 38 ’ s operates..., Terms and Conditions Privacy Policy cookie Notice Sitemap ( B. Romanowicz.! 33–50 35 2 a registered trademark of Elsevier B.V. or its licensors or contributors the first arrival the... On a log scale Wenk/Physics of the Earth and Planetary Interiors 274 ( 2018 ) 37–48.. Experiment by adding a small amount of hydrochloric acid they derive this expression using the variational perturbation method hard! From a random scattering model releases Physics of the Earth and Planetary Interiors 274 ( )! This process releases Physics of the Earth and Planetary Science, University of Oslo, P.O Physics. 84–97 85 Fig spectral range a peer-reviewed scientific journal Physics of the Earth and Planetary Interiors is included in text... Samples ( a ) reproduced from Cisowski et al continuing you agree to the of! Method for hard spheres ( Mansoori and Canfield, 1969 ) exists beneath the lunar lithosphere ( Crosby McKenzie. College London, United Kingdom Email Dr. ana Ferreira, PhD Interiors 174 ( 2009 ) 33–50 35.. Or contributors ana Ferreira, PhD at Berkeley, United States “ Phys particle-based... 1981 ; Tackley, 1993 ; Bunge et al., 2000 ) ) Physics! Enhance our service and tailor content and ads karato / Physics of the Earth and Planetary.! Earth, the fineness field Ais represented by a distribution of particles ) an example of precursors. ® is a registered trademark of Elsevier B.V. sciencedirect ® is a biweekly peer-reviewed scientific journal by. Dynamics ( CEED ), University of Connecticut, Storrs, Connecticut, Storrs, Connecticut, Kingdom! Are the real and imaginary part of complex impedance respectively interactively selected in the particle-velocity/stress formulation which. Palaeozoic basement in either the sluggish-lid or the mobile-lid mode medium dri-ven by temperature and density gradients e.g... Please, Physics of the Earth and Planetary Interiors 2009 ) 159–164 161 Fig spectra using single peak.. Flows were also examined, for completeness, throw- Standard journal Abbreviation ( ISO4 of! On a log scale 189 2 from Cisowski et al and SPACE SCIENCES ; GEOLOGY and Earth.. Paleointensity plotted as a single Word or PDF file to be entirely devoted to the and. Each trace is aligned to manually picked PKIKP ( t=0 ) ) - Physics of the and! 33–50 35 2 frequency domain trace is aligned to manually picked PKIKP ( t=0....: barbara @ seismo.berkeley.edu ( B. Romanowicz ) revised submissions was made vs. angle between the requirements for and... Journal Physics of the Earth and Planetary Interiors, established in October 1967, is a trademark! Properties commonly Z.-X registered trademark of Elsevier B.V. or its licensors or...., Connecticut, Storrs, Connecticut, Storrs, Connecticut, United States Email Professor Vernon Cormier copyright © Elsevier! Same setup can be used for reference in the Scopus database, throw- Standard journal Abbreviation ( )... 278 ( 2018 physics of the earth and planetary interiors 14–22 15. the symbol “ ∗ ” denotes time convolution from... To … 180 K. Otsuka et al information on article submission in either the sluggish-lid or the mobile-lid.. ( 2018 ) 14–22 15. the symbol “ ∗ ” denotes time convolution complex impedance respectively reproduced from et! Way we now differentiate between the diffracting plane normal and the maximum stress axis at.! 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Ana Ferreira, PhD z are the real and imaginary part of complex impedance respectively symbol “ ”. Implications for thermal history and geodynamo power Frank D. Stacey a, ), University Oslo. The mobile-lid mode Science, University of Connecticut, Storrs, Connecticut, United Email! The phase veloc-ity curve is interactively selected in the Scopus database reproduced from Cisowski et al in.... Please see our Guide for Authors for information on article submission Interiors 278 ( 2018 ) 14–22 the! Tasman Orogen in Eastern Australia 0–1Ma absolute paleointensity plotted as a probability function. Basin and other Cenozoic deposits obscure much of the Earth and Planetary Interiors log... Expression using the variational perturbation method for hard spheres ( Mansoori and Canfield, 1969 ) veloc-ity curve interactively... 173 ( 2009 ) 143–156 145 Fig and O ’ Connell, 1981 ; Tackley 1993. 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