Example of Physics of The Earth and Planetary Interiors format
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Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format Example of Physics of The Earth and Planetary Interiors format
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open access Open Access

Physics of The Earth and Planetary Interiors — Template for authors

Publisher: Elsevier
Categories Rank Trend in last 3 yrs
Physics and Astronomy (miscellaneous) #13 of 58 down down by 3 ranks
Geophysics #40 of 131 down down by 14 ranks
Astronomy and Astrophysics #30 of 88 down down by 2 ranks
Space and Planetary Science #38 of 97 down down by 6 ranks
journal-quality-icon Journal quality:
High
calendar-icon Last 4 years overview: 445 Published Papers | 1829 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 27/06/2020
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Related Journals

open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.6
SJR: 0.682
SNIP: 1.274
open access Open Access

Oxford University Press

Quality:  
High
CiteRatio: 9.2
SJR: 2.067
SNIP: 0.962
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 6.8
SJR: 1.485
SNIP: 1.164
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 7.7
SJR: 1.785
SNIP: 1.24

Journal Performance & Insights

CiteRatio

SCImago Journal Rank (SJR)

Source Normalized Impact per Paper (SNIP)

A measure of average citations received per peer-reviewed paper published in the journal.

Measures weighted citations received by the journal. Citation weighting depends on the categories and prestige of the citing journal.

Measures actual citations received relative to citations expected for the journal's category.

4.1

CiteRatio for Physics of The Earth and Planetary Interiors from 2016 - 2020
Year Value
2020 4.1
2019 4.1
2018 3.8
2017 4.2
2016 4.5
graph view Graph view
table view Table view

1.099

13% from 2019

SJR for Physics of The Earth and Planetary Interiors from 2016 - 2020
Year Value
2020 1.099
2019 1.269
2018 1.16
2017 1.285
2016 1.585
graph view Graph view
table view Table view

1.093

8% from 2019

SNIP for Physics of The Earth and Planetary Interiors from 2016 - 2020
Year Value
2020 1.093
2019 1.013
2018 1.106
2017 0.981
2016 1.078
graph view Graph view
table view Table view

insights Insights

  • This journal’s CiteRatio is in the top 10 percentile category.

insights Insights

  • SJR of this journal has decreased by 13% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has increased by 8% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Physics of The Earth and Planetary Interiors

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Elsevier

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 Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely ...... Read More

Physics and Astronomy

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Last updated on
27 Jun 2020
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ISSN
0031-9201
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Impact Factor
High - 1.285
i
Open Access
No
i
Sherpa RoMEO Archiving Policy
Green faq
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Plagiarism Check
Available via Turnitin
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Endnote Style
Download Available
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Bibliography Name
elsarticle-num
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Citation Type
Numbered
[25]
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Bibliography Example
G. E. Blonder, M. Tinkham, T. M. Klapwijk, Transition from metallic to tunneling regimes in superconducting microconstrictions: Excess current, charge imbalance, and supercurrent conversion, Phys. Rev. B 25 (7) (1982) 4515–4532. URL 10.1103/PhysRevB.25.4515

Top papers written in this journal

Journal Article DOI: 10.1016/0031-9201(81)90046-7
Preliminary reference earth model
Adam M. Dziewonski1, Don L. Anderson2

Abstract:

A large data set consisting of about 1000 normal mode periods, 500 summary travel time observations, 100 normal mode Q values, mass and moment of inertia have been inverted to obtain the radial distribution of elastic properties, Q values and density in the Earth's interior. The data set was supplemented with a special study ... A large data set consisting of about 1000 normal mode periods, 500 summary travel time observations, 100 normal mode Q values, mass and moment of inertia have been inverted to obtain the radial distribution of elastic properties, Q values and density in the Earth's interior. The data set was supplemented with a special study of 12 years of ISC phase data which yielded an additional 1.75 × 10^6 travel time observations for P and S waves. In order to obtain satisfactory agreement with the entire data set we were required to take into account anelastic dispersion. The introduction of transverse isotropy into the outer 220 km of the mantle was required in order to satisfy the shorter period fundamental toroidal and spheroidal modes. This anisotropy also improved the fit of the larger data set. The horizontal and vertical velocities in the upper mantle differ by 2–4%, both for P and S waves. The mantle below 220 km is not required to be anisotropic. Mantle Rayleigh waves are surprisingly sensitive to compressional velocity in the upper mantle. High S_n velocities, low P_n velocities and a pronounced low-velocity zone are features of most global inversion models that are suppressed when anisotropy is allowed for in the inversion. The Preliminary Reference Earth Model, PREM, and auxiliary tables showing fits to the data are presented. read more read less

Topics:

Preliminary reference Earth model (61%)61% related to the paper, Core–mantle boundary (58%)58% related to the paper, Mantle convection (57%)57% related to the paper, Seismic anisotropy (57%)57% related to the paper, Outer core (56%)56% related to the paper
8,477 Citations
Journal Article DOI: 10.1016/0031-9201(77)90108-X
Hysteresis properties of titanomagnetites: Grain-size and compositional dependence
R. Day1, Michael D Fuller1, Victor A. Schmidt2

Abstract:

Sized fractions of x = 0.6, 0.4, 0.2 and 0.0 titanomagnetites were studied with a vibration magnetometer. In the course particles (d > 150 μm), no compositional dependence of hysteresis parameters was found. HC was less than 50 Oe, HR/HC > 4 and JR/JS < 10−2, reflecting multi-domain behaviour. In contrast, fine particles (d ⋍... Sized fractions of x = 0.6, 0.4, 0.2 and 0.0 titanomagnetites were studied with a vibration magnetometer. In the course particles (d > 150 μm), no compositional dependence of hysteresis parameters was found. HC was less than 50 Oe, HR/HC > 4 and JR/JS < 10−2, reflecting multi-domain behaviour. In contrast, fine particles (d ⋍ 0.1 μm) revealed systematic grain-size dependence of parameters with coercive force as high as 2,000 Oe in x = 0.6 titanomagnetite. Grain-size dependence studies revealed broad transition sizes for the onset of true multi-domain behaviour depending upon which factor is chosen. In magnetite it varies from 10 to 20 μm. The experimental critical size for single-domain behaviour for magnetite is about 0.1 μm and for x = 0.6 titanomagnetite 1–2 μm. read more read less
2,496 Citations
Journal Article DOI: 10.1016/J.PEPI.2012.04.002
The global CMT project 2004–2010: Centroid-moment tensors for 13,017 earthquakes
Göran Ekström1, Meredith Nettles1, Adam M. Dziewonski2

Abstract:

Earthquake moment tensors reflecting seven years of global seismic activity (2004–2010) are presented. The results are the product of the global centroid-moment-tensor (GCMT) project, which maintains and extends a catalog of global seismic moment tensors beginning with earthquakes in 1976. Starting with earthquakes in 2004, t... Earthquake moment tensors reflecting seven years of global seismic activity (2004–2010) are presented. The results are the product of the global centroid-moment-tensor (GCMT) project, which maintains and extends a catalog of global seismic moment tensors beginning with earthquakes in 1976. Starting with earthquakes in 2004, the GCMT analysis takes advantage of advances in the mapping of propagation characteristics of intermediate-period surface waves, and includes these waves in the moment-tensor inversions. This modification of the CMT algorithm makes possible the globally uniform determination of moment tensors for earthquakes as small as MW = 5.0. For the period 2004–2010, 13,017 new centroid-moment tensors are reported. read more read less

Topics:

Seismic moment (55%)55% related to the paper, Moment (mathematics) (50%)50% related to the paper
View PDF
1,576 Citations
Journal Article DOI: 10.1016/0031-9201(90)90002-F
Evidence for and implications of self-healing pulses of slip in earthquake rupture
Thomas H. Heaton1

Abstract:

Dislocation time histories of models derived from waveforms of seven earthquakes are discussed. In each model, dislocation rise times (the duration of slip for a given point on the fault) are found to be short compared to the overall duration of the earthquake (∼ 10%). However, in many crack-like numerical models of dynamic r... Dislocation time histories of models derived from waveforms of seven earthquakes are discussed. In each model, dislocation rise times (the duration of slip for a given point on the fault) are found to be short compared to the overall duration of the earthquake (∼ 10%). However, in many crack-like numerical models of dynamic rupture, the slip duration at a given point is comparable to the overall duration of the rupture; i.e. slip at a given point continues until information is received that the rupture has stopped propagating. Alternative explanations for the discrepancy between the short slip durations used to model waveforms and the long slip durations inferred from dynamic crack models are: (1) the dislocation models are unable to resolve the relatively slow parts of earthquake slip and have seriously underestimated the dislocations for these earthquakes; (2) earthquakes are composed of a sequence of small-dimension (short duration) events that are separated by locked regions (barriers); (3) rupture occurs in a narrow self-healing pulse of slip that travels along the fault surface. Evidence is discussed that suggests that slip durations are indeed short and that the self-healing slip-pulse model is the most appropriate explanation. A qualitative model is presented that produces self-healing slip pulses. The key feature of the model is the assumption that friction on the fault surface is inversely related to the local slip velocity. The model has the following features: high static strength of materials (kilobar range), low static stress drops (in the range of tens of bars), and relatively low frictional stress during slip (less than several hundreds of bars). It is suggested that the reason that the average dislocation scales with fault length is because large-amplitude slip pulses are difficult to stop and hence tend to propagate large distances. This model may explain why seismicity and ambient stress are low along fault segments that have experienced large earthquakes. It also qualitatively explains why the recurrence time for large earthquakes may be irregular. read more read less

Topics:

Slip (materials science) (72%)72% related to the paper, Earthquake rupture (68%)68% related to the paper, Supershear earthquake (54%)54% related to the paper
843 Citations
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13. What is Sherpa RoMEO Archiving Policy for Physics of The Earth and Planetary Interiors?

SHERPA/RoMEO Database

We extracted this data from Sherpa Romeo to help researchers understand the access level of this journal in accordance with the Sherpa Romeo Archiving Policy for Physics of The Earth and Planetary Interiors. The table below indicates the level of access a journal has as per Sherpa Romeo's archiving policy.

RoMEO Colour Archiving policy
Green Can archive pre-print and post-print or publisher's version/PDF
Blue Can archive post-print (ie final draft post-refereeing) or publisher's version/PDF
Yellow Can archive pre-print (ie pre-refereeing)
White Archiving not formally supported
FYI:
  1. Pre-prints as being the version of the paper before peer review and
  2. Post-prints as being the version of the paper after peer-review, with revisions having been made.

14. What are the most common citation types In Physics of The Earth and Planetary Interiors?

The 5 most common citation types in order of usage for Physics of The Earth and Planetary Interiors are:.

S. No. Citation Style Type
1. Author Year
2. Numbered
3. Numbered (Superscripted)
4. Author Year (Cited Pages)
5. Footnote

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