Example of Earth, Planets and Space format
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Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format
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Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format Example of Earth, Planets and Space format
Sample paper formatted on SciSpace - SciSpace
This content is only for preview purposes. The original open access content can be found here.
open access Open Access

Earth, Planets and Space — Template for authors

Publisher: Springer
Categories Rank Trend in last 3 yrs
Geology #58 of 251 down down by 11 ranks
Space and Planetary Science #34 of 97 down down by 1 rank
journal-quality-icon Journal quality:
High
calendar-icon Last 4 years overview: 631 Published Papers | 2774 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 06/07/2020
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FAQ

Related Journals

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IEEE

Quality:  
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SJR: 0.935
SNIP: 1.026
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Journal Performance & Insights

Impact Factor

CiteRatio

Determines the importance of a journal by taking a measure of frequency with which the average article in a journal has been cited in a particular year.

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

2.075

24% from 2018

Impact factor for Earth, Planets and Space from 2016 - 2019
Year Value
2019 2.075
2018 2.736
2017 2.773
2016 2.243
graph view Graph view
table view Table view

4.4

15% from 2019

CiteRatio for Earth, Planets and Space from 2016 - 2020
Year Value
2020 4.4
2019 5.2
2018 5.0
2017 4.1
2016 3.3
graph view Graph view
table view Table view

insights Insights

  • Impact factor of this journal has decreased by 24% in last year.
  • This journal’s impact factor is in the top 10 percentile category.

insights Insights

  • CiteRatio of this journal has decreased by 15% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

SCImago Journal Rank (SJR)

Source Normalized Impact per Paper (SNIP)

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.

0.835

30% from 2019

SJR for Earth, Planets and Space from 2016 - 2020
Year Value
2020 0.835
2019 1.2
2018 1.209
2017 1.289
2016 0.981
graph view Graph view
table view Table view

1.116

2% from 2019

SNIP for Earth, Planets and Space from 2016 - 2020
Year Value
2020 1.116
2019 1.144
2018 1.43
2017 1.379
2016 0.937
graph view Graph view
table view Table view

insights Insights

  • SJR of this journal has decreased by 30% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has decreased by 2% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Earth, Planets and Space

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Springer

Earth, Planets and Space

Approved by publishing and review experts on SciSpace, this template is built as per for Earth, Planets and Space formatting guidelines as mentioned in Springer author instructions. The current version was created on and has been used by 745 authors to write and format their manuscripts to this journal.

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Last updated on
06 Jul 2020
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ISSN
1606-8610
i
Open Access
Yes
i
Sherpa RoMEO Archiving Policy
White faq
i
Plagiarism Check
Available via Turnitin
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Endnote Style
Download Available
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Citation Type
Author Year
(Blonder et al, 1982)
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Bibliography Example
Beenakker CWJ (2006) Specular andreev reflection in graphene. Phys Rev Lett 97(6):067,007, URL 10.1103/PhysRevLett.97.067007

Top papers written in this journal

open accessOpen access Journal Article DOI: 10.1186/S40623-015-0228-9
International Geomagnetic Reference Field: the 12th generation
27 May 2015 - Earth, Planets and Space

Abstract:

The 12th generation of the International Geomagnetic Reference Field (IGRF) was adopted in December 2014 by the Working Group V-MOD appointed by the International Association of Geomagnetism and Aeronomy (IAGA). It updates the previous IGRF generation with a definitive main field model for epoch 2010.0, a main field model for... The 12th generation of the International Geomagnetic Reference Field (IGRF) was adopted in December 2014 by the Working Group V-MOD appointed by the International Association of Geomagnetism and Aeronomy (IAGA). It updates the previous IGRF generation with a definitive main field model for epoch 2010.0, a main field model for epoch 2015.0, and a linear annual predictive secular variation model for 2015.0-2020.0. Here, we present the equations defining the IGRF model, provide the spherical harmonic coefficients, and provide maps of the magnetic declination, inclination, and total intensity for epoch 2015.0 and their predicted rates of change for 2015.0-2020.0. We also update the magnetic pole positions and discuss briefly the latest changes and possible future trends of the Earth’s magnetic field. read more read less

Topics:

International Geomagnetic Reference Field (76%)76% related to the paper, Secular variation (52%)52% related to the paper, Epoch (reference date) (50%)50% related to the paper
View PDF
1,268 Citations
open accessOpen access Journal Article DOI: 10.1186/BF03353076
Recent progress of seismic observation networks in Japan —Hi-net, F-net, K-NET and KiK-net—
01 Aug 2004 - Earth, Planets and Space

Abstract:

After the disastrous 1995 Kobe earthquake, a new national project has started to drastically improve seismic observation system in Japan. A large number of strong-motion, high-sensitivity, and broadband seismographs were installed to construct dense and uniform networks covering the whole of Japan. The new high-sensitivity se... After the disastrous 1995 Kobe earthquake, a new national project has started to drastically improve seismic observation system in Japan. A large number of strong-motion, high-sensitivity, and broadband seismographs were installed to construct dense and uniform networks covering the whole of Japan. The new high-sensitivity seismo-graph network consisting of 696 stations is called Hi-net, while the broadband seismograph network consisting of 71 stations is called F-net. At most of Hi-net stations strong-motion seismographs are also equipped both at depth and the ground surface. The network of these 659 stations with an uphole/downhole pair of strong-motion seismographs is called KiK-net, while another network consisting of 1034 strong-motion seismographs installed at the ground surface is called K-NET. Here, all the station numbers are as of April 2003. High-sensitivity data from Hi-net and pre-existing seismic networks operated by various institutions have been transmitted to and processed by the Japan Meteorological Agency since October 1997 to monitor the seismic activity in and around Japan. The same data are shared to university group in real time using satellite communication for their research work. The data are also archived at the National Research Institute for Earth Science and Disaster Prevention and stored in their database system for public use under a fully open policy. read more read less

Topics:

Seismometer (51%)51% related to the paper
View PDF
729 Citations
open accessOpen access Journal Article DOI: 10.5047/EPS.2011.06.010
Tsunami source of the 2011 off the Pacific coast of Tohoku Earthquake
Yushiro Fujii1, Kenji Satake2, Shin'ichi Sakai2, Masanao Shinohara2, Toshihiko Kanazawa2
27 Sep 2011 - Earth, Planets and Space

Abstract:

Tsunami waveform inversion for the 11 March, 2011, off the Pacific coast of Tohoku Earthquake (M 9.0) indicates that the source of the largest tsunami was located near the axis of the Japan trench. Ocean-bottom pressure, and GPS wave, gauges recorded two-step tsunami waveforms: a gradual increase of sea level (~2 m) followed ... Tsunami waveform inversion for the 11 March, 2011, off the Pacific coast of Tohoku Earthquake (M 9.0) indicates that the source of the largest tsunami was located near the axis of the Japan trench. Ocean-bottom pressure, and GPS wave, gauges recorded two-step tsunami waveforms: a gradual increase of sea level (~2 m) followed by an impulsive tsunami wave (3 to 5 m). The slip distribution estimated from 33 coastal tide gauges, offshore GPS wave gauges and bottom-pressure gauges show that the large slip, more than 40 m, was located along the trench axis. This offshore slip, similar but much larger than the 1896 Sanriku “tsunami earthquake,” is responsible for the recorded large impulsive peak. Large slip on the plate interface at southern Sanriku-oki (~30 m) and Miyagi-oki (~17 m) around the epicenter, a similar location with larger slip than the previously proposed fault model of the 869 Jogan earthquake, is responsible for the initial water-level rise and, presumably, the large tsunami inundation in Sendai plain. The interplate slip is ~10 m in Fukushima-oki, and less than 3 m in the Ibaraki-oki region. The total seismic moment is estimated as 3.8 × 1022 N m (Mw = 9.0). read more read less

Topics:

Tsunami earthquake (69%)69% related to the paper, Seismic moment (56%)56% related to the paper, Slip (materials science) (56%)56% related to the paper, Epicenter (52%)52% related to the paper
View PDF
496 Citations
open accessOpen access Journal Article DOI: 10.1186/BF03353258
Plasmoid-induced-reconnection and fractal reconnection
Kazunari Shibata1, S. Tanuma2
01 Jun 2001 - Earth, Planets and Space

Abstract:

As a key to understanding the basic mechanism for fast reconnection in solar flares, plasmoid-induced-reconnection and fractal reconnection are proposed and examined. We first briefly summarize recent solar observations that give us hints on the role of plasmoid (flux rope) ejections in flare energy release. We then discuss t... As a key to understanding the basic mechanism for fast reconnection in solar flares, plasmoid-induced-reconnection and fractal reconnection are proposed and examined. We first briefly summarize recent solar observations that give us hints on the role of plasmoid (flux rope) ejections in flare energy release. We then discuss the plasmoid-induced-reconnection model, which is an extention of the classical two-ribbon-flare model which we refer to as the CSHKP model. An essential ingredient of the new model is the formation and ejection of a plasmoid which play an essential role in the storage of magnetic energy (by inhibiting reconnection) and the induction of a strong inflow into reconnection region. Using a simple analytical model, we show that the plasmoid ejection and acceleration are closely coupled with the reconnection process, leading to a nonlinear instability for the whole dynamics that determines the macroscopic reconnection rate uniquely. Next we show that the current sheet tends to have a fractal structure via the following process path: tearing ⇒ sheet thinning ⇒ Sweet-Parker sheet ⇒ secondary tearing ⇒ further sheet thinning ⇒ ⋯. These processes occur repeatedly at smaller scales until a microscopic plasma scale (either the ion Larmor radius or the ion inertial length) is reached where anomalous resistivity or collisionless reconnection can occur. The current sheet eventually has a fractal structure with many plasmoids (magnetic islands) of different sizes. When these plasmoids are ejected out of the current sheets, fast reconnection occurs at various different scales in a highly time dependent manner. Finally, a scenario is presented for fast reconnection in the solar corona on the basis of above plasmoid-induced-reconnection in a fractal current sheet. read more read less

Topics:

Magnetic reconnection (61%)61% related to the paper, Plasmoid (61%)61% related to the paper, Current sheet (61%)61% related to the paper
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460 Citations
open accessOpen access Journal Article DOI: 10.1186/BF03351933
Swarm: A constellation to study the Earth’s magnetic field
Eigil Friis-Christensen, Hermann Lühr, Gauthier Hulot1
14 Apr 2006 - Earth, Planets and Space

Abstract:

The Swarm mission was selected as the 5th mission in ESA’s Earth Explorer Programme in 2004. The mission will provide the best ever survey of the geomagnetic field and its temporal evolution that will lead to new insights into the Earth system by improving our understanding of the Earth’s interior and its effect on Geospace, ... The Swarm mission was selected as the 5th mission in ESA’s Earth Explorer Programme in 2004. The mission will provide the best ever survey of the geomagnetic field and its temporal evolution that will lead to new insights into the Earth system by improving our understanding of the Earth’s interior and its effect on Geospace, the vast region around the Earth where electrodynamic processes are influenced by the Earth’s magnetic field. Scheduled for launch in 2010, the mission will comprise a constellation of three satellites, with two spacecraft flying sideby- side at lower altitude (450 km initial altitude), thereby measuring the East-West gradient of the magnetic field, and the third one flying at higher altitude (530 km). High-precision and high-resolution measurements of the strength, direction and variation of the magnetic field, complemented by precise navigation, accelerometer and electric field measurements, will provide the necessary observations that are required to separate and model the various sources of the geomagnetic field. This results in a unique “view” inside the Earth from space to study the composition and processes of its interior. It also allows analysing the Sun’s influence within the Earth system. In addition practical applications in many different areas, such as space weather, radiation hazards, navigation and resource management, will benefit from the Swarm concept. read more read less

Topics:

Earth's magnetic field (60%)60% related to the paper, Space weather (56%)56% related to the paper, Earth system science (55%)55% related to the paper, Spacecraft (52%)52% related to the paper, Satellite (52%)52% related to the paper
View PDF
446 Citations
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Frequently asked questions

1. Can I write Earth, Planets and Space in LaTeX?

Absolutely not! Our tool has been designed to help you focus on writing. You can write your entire paper as per the Earth, Planets and Space guidelines and auto format it.

2. Do you follow the Earth, Planets and Space guidelines?

Yes, the template is compliant with the Earth, Planets and Space guidelines. Our experts at SciSpace ensure that. If there are any changes to the journal's guidelines, we'll change our algorithm accordingly.

3. Can I cite my article in multiple styles in Earth, Planets and Space?

Of course! We support all the top citation styles, such as APA style, MLA style, Vancouver style, Harvard style, and Chicago style. For example, when you write your paper and hit autoformat, our system will automatically update your article as per the Earth, Planets and Space citation style.

4. Can I use the Earth, Planets and Space templates for free?

Sign up for our free trial, and you'll be able to use all our features for seven days. You'll see how helpful they are and how inexpensive they are compared to other options, Especially for Earth, Planets and Space.

5. Can I use a manuscript in Earth, Planets and Space that I have written in MS Word?

Yes. You can choose the right template, copy-paste the contents from the word document, and click on auto-format. Once you're done, you'll have a publish-ready paper Earth, Planets and Space that you can download at the end.

6. How long does it usually take you to format my papers in Earth, Planets and Space?

It only takes a matter of seconds to edit your manuscript. Besides that, our intuitive editor saves you from writing and formatting it in Earth, Planets and Space.

7. Where can I find the template for the Earth, Planets and Space?

It is possible to find the Word template for any journal on Google. However, why use a template when you can write your entire manuscript on SciSpace , auto format it as per Earth, Planets and Space's guidelines and download the same in Word, PDF and LaTeX formats? Give us a try!.

8. Can I reformat my paper to fit the Earth, Planets and Space's guidelines?

Of course! You can do this using our intuitive editor. It's very easy. If you need help, our support team is always ready to assist you.

9. Earth, Planets and Space an online tool or is there a desktop version?

SciSpace's Earth, Planets and Space is currently available as an online tool. We're developing a desktop version, too. You can request (or upvote) any features that you think would be helpful for you and other researchers in the "feature request" section of your account once you've signed up with us.

10. I cannot find my template in your gallery. Can you create it for me like Earth, Planets and Space?

Sure. You can request any template and we'll have it setup within a few days. You can find the request box in Journal Gallery on the right side bar under the heading, "Couldn't find the format you were looking for like Earth, Planets and Space?”

11. What is the output that I would get after using Earth, Planets and Space?

After writing your paper autoformatting in Earth, Planets and Space, you can download it in multiple formats, viz., PDF, Docx, and LaTeX.

12. Is Earth, Planets and Space's impact factor high enough that I should try publishing my article there?

To be honest, the answer is no. The impact factor is one of the many elements that determine the quality of a journal. Few of these factors include review board, rejection rates, frequency of inclusion in indexes, and Eigenfactor. You need to assess all these factors before you make your final call.

13. What is Sherpa RoMEO Archiving Policy for Earth, Planets and Space?

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 Earth, Planets and Space. 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 Earth, Planets and Space?

The 5 most common citation types in order of usage for Earth, Planets and Space are:.

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

15. How do I submit my article to the Earth, Planets and Space?

It is possible to find the Word template for any journal on Google. However, why use a template when you can write your entire manuscript on SciSpace , auto format it as per Earth, Planets and Space's guidelines and download the same in Word, PDF and LaTeX formats? Give us a try!.

16. Can I download Earth, Planets and Space in Endnote format?

Yes, SciSpace provides this functionality. After signing up, you would need to import your existing references from Word or Bib file to SciSpace. Then SciSpace would allow you to download your references in Earth, Planets and Space Endnote style according to Elsevier guidelines.

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I spent hours with MS word for reformatting. It was frustrating - plain and simple. With SciSpace, I can draft my manuscripts and once it is finished I can just submit. In case, I have to submit to another journal it is really just a button click instead of an afternoon of reformatting.

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