Example of Geoscience Letters format
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Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format
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Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format Example of Geoscience Letters format
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open access Open Access

Geoscience Letters — Template for authors

Publisher: Springer
Categories Rank Trend in last 3 yrs
Earth and Planetary Sciences (all) #43 of 186 down down by 4 ranks
journal-quality-icon Journal quality:
High
calendar-icon Last 4 years overview: 56 Published Papers | 192 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 18/07/2020
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Related Journals

open access Open Access

Taylor and Francis

Quality:  
High
CiteRatio: 4.1
SJR: 0.694
SNIP: 0.72
open access Open Access
recommended Recommended

Taylor and Francis

Quality:  
High
CiteRatio: 6.6
SJR: 0.813
SNIP: 1.434
open access Open Access
recommended Recommended

Springer

Quality:  
High
CiteRatio: 7.2
SJR: 1.148
SNIP: 1.68
open access Open Access
recommended Recommended

IEEE

Quality:  
High
CiteRatio: 15.5
SJR: 3.038
SNIP: 7.166

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.

3.4

29% from 2019

CiteRatio for Geoscience Letters from 2016 - 2020
Year Value
2020 3.4
2019 4.8
2018 3.9
2017 3.2
graph view Graph view
table view Table view

1.031

7% from 2019

SJR for Geoscience Letters from 2017 - 2020
Year Value
2020 1.031
2019 1.114
2018 1.022
2017 0.696
graph view Graph view
table view Table view

1.394

3% from 2019

SNIP for Geoscience Letters from 2017 - 2020
Year Value
2020 1.394
2019 1.435
2018 1.146
2017 0.807
graph view Graph view
table view Table view

insights Insights

  • CiteRatio of this journal has decreased by 29% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

insights Insights

  • SJR of this journal has decreased by 7% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has decreased by 3% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Geoscience Letters

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Springer

Geoscience Letters

Approved by publishing and review experts on SciSpace, this template is built as per for Geoscience Letters formatting guidelines as mentioned in Springer author instructions. The current version was created on and has been used by 329 authors to write and format their manuscripts to this journal.

Biogeosciences

i
Last updated on
18 Jul 2020
i
ISSN
1606-8610
i
Open Access
Yes
i
Sherpa RoMEO Archiving Policy
White faq
i
Plagiarism Check
Available via Turnitin
i
Endnote Style
Download Available
i
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/S40562-016-0039-2
History and Development of Coronal Mass Ejections as a Key Player in Solar Terrestrial Relationship
Nat Gopalswamy1
03 Mar 2016 - Geoscience Letters

Abstract:

Coronal mass ejections (CMEs) are relatively a recently discovered phenomenon—in 1971, some 15 years into the Space Era. It took another two decades to realize that CMEs are the most important players in solar terrestrial relationship as the root cause of severe weather in Earth’s space environment. CMEs are now counted among... Coronal mass ejections (CMEs) are relatively a recently discovered phenomenon—in 1971, some 15 years into the Space Era. It took another two decades to realize that CMEs are the most important players in solar terrestrial relationship as the root cause of severe weather in Earth’s space environment. CMEs are now counted among the major natural hazards because they cause large solar energetic particle (SEP) events and major geomagnetic storms, both of which pose danger to humans and their technology in space and ground. Geomagnetic storms discovered in the 1700s, solar flares discovered in the 1800s, and SEP events discovered in the 1900s are all now found to be closely related to CMEs via various physical processes occurring at various locations in and around CMEs, when they interact with the ambient medium. This article identifies a number of key developments that preceded the discovery of white-light CMEs suggesting that CMEs were waiting to be discovered. The last two decades witnessed an explosion of CME research following the launch of the Solar and Heliospheric Observatory mission in 1995, resulting in the establishment of a full picture of CMEs. read more read less

Topics:

Coronal mass ejection (56%)56% related to the paper, Solar flare (51%)51% related to the paper, Geomagnetic storm (51%)51% related to the paper
View PDF
101 Citations
open accessOpen access Journal Article DOI: 10.1186/S40562-018-0113-Z
Hydrologic modeling: progress and future directions
Vijay P. Singh1
28 May 2018 - Geoscience Letters

Abstract:

Briefly tracing the history of hydrologic modeling, this paper discusses the progress that has been achieved in hydrologic modeling since the advent of computer and what the future may have in store for hydrologic modeling. Hydrologic progress can be described through the developments in data collection and processing, concep... Briefly tracing the history of hydrologic modeling, this paper discusses the progress that has been achieved in hydrologic modeling since the advent of computer and what the future may have in store for hydrologic modeling. Hydrologic progress can be described through the developments in data collection and processing, concepts and theories, integration with allied sciences, computational and analysis tools, and models and model results. It is argued that with the aid of new information gathering and computational tools, hydrology will witness greater integration with both technical and non-technical areas and increasing applications of information technology tools. Furthermore, hydrology will play an increasingly important role in meeting grand challenges of the twenty-first century, such as food security, water security, energy security, health security, ecosystem security, and sustainable development. read more read less

Topics:

Hydrological modelling (57%)57% related to the paper
View PDF
97 Citations
open accessOpen access Journal Article DOI: 10.1186/S40562-016-0037-4
Geomagnetic storms: historical perspective to modern view
Gurbax S. Lakhina, Bruce T. Tsurutani1
20 Feb 2016 - Geoscience Letters

Abstract:

The history of geomagnetism is more than 400 years old. Geomagnetic storms as we know them were discovered about 210 years ago. There has been keen interest in understanding Sun–Earth connection events, such as solar flares, CMEs, and concomitant magnetic storms in recent times. Magnetic storms are the most important componen... The history of geomagnetism is more than 400 years old. Geomagnetic storms as we know them were discovered about 210 years ago. There has been keen interest in understanding Sun–Earth connection events, such as solar flares, CMEs, and concomitant magnetic storms in recent times. Magnetic storms are the most important component of space weather effects on Earth. We give an overview of the historical aspects of geomagnetic storms and the progress made during the past two centuries. Super magnetic storms can cause life-threatening power outages and satellite damage, communication failures and navigational problems. The data for such super magnetic storms that occurred in the last 50 years during the space era is sparce. Research on historical geomagnetic storms can help to create a database for intense and super magnetic storms. New knowledge of interplanetary and solar causes of magnetic storms gained from spaceage observations will be used to review the super magnetic storm of September 1–2, 1859. We discuss the occurrence probability of such super magnetic storms, and the maximum possible intensity for the effects of a perfect ICME: extreme super magnetic storm, extreme magnetospheric compression, and extreme magnetospheric electric fields. read more read less

Topics:

Space weather (59%)59% related to the paper, Geomagnetic storm (56%)56% related to the paper, Coronal mass ejection (52%)52% related to the paper
View PDF
95 Citations
open accessOpen access Journal Article DOI: 10.1186/S40562-016-0066-Z
A trio-interaction theory for Madden–Julian oscillation
Bin Wang1, Bin Wang2, Fei Liu2, Guosen Chen1, Guosen Chen2
01 Dec 2016 - Geoscience Letters

Abstract:

The Madden–Julian oscillation (MJO) is the dominant mode of tropical atmospheric intraseasonal variability and a primary source of predictability for global sub-seasonal prediction. Understanding the origin and perpetuation of the MJO has eluded scientists for decades. The present paper starts with a brief review of progresse... The Madden–Julian oscillation (MJO) is the dominant mode of tropical atmospheric intraseasonal variability and a primary source of predictability for global sub-seasonal prediction. Understanding the origin and perpetuation of the MJO has eluded scientists for decades. The present paper starts with a brief review of progresses in theoretical studies of the MJO and a discussion of the essential MJO characteristics that a theory should explain. A general theoretical model framework is then described in an attempt to integrate the major existing theoretical models: the frictionally coupled Kelvin–Rossby wave, the moisture mode, the frictionally coupled dynamic moisture mode, the MJO skeleton, and the gravity wave interference, which are shown to be special cases of the general MJO model. The last part of the present paper focuses on a special form of trio-interaction theory in terms of the general model with a simplified Betts–Miller (B-M) cumulus parameterization scheme. This trio-interaction theory extends the Matsuno–Gill theory by incorporating a trio-interaction among convection, moisture, and wave-boundary layer (BL) dynamics. The model is shown to produce robust large-scale characteristics of the observed MJO, including the coupled Kelvin–Rossby wave structure, slow eastward propagation (~5 m/s) over warm pool, the planetary (zonal) scale circulation, the BL low-pressure and moisture convergence preceding major convection, and amplification/decay over warm/cold sea surface temperature (SST) regions. The BL moisture convergence feedback plays a central role in coupling equatorial Kelvin and Rossby waves with convective heating, selecting a preferred eastward propagation, and generating instability. The moisture feedback can enhance Rossby wave component, thereby substantially slowing down eastward propagation. With the trio-interaction theory, a number of fundamental issues of MJO dynamics are addressed: why the MJO possesses a mixed Kelvin–Rossby wave structure and how the Kelvin and Rossby waves, which propagate in opposite directions, could couple together with convection and select eastward propagation; what makes the MJO move eastward slowly in the eastern hemisphere, resulting in the 30–60-day periodicity; why MJO amplifies over the warm pool ocean and decays rapidly across the dateline. Limitation and ramifications of the model results to general circulation modeling of MJO are discussed. read more read less

Topics:

Rossby wave (55%)55% related to the paper, Madden–Julian oscillation (55%)55% related to the paper
View PDF
80 Citations
open accessOpen access Journal Article DOI: 10.1186/S40562-018-0102-2
The Indonesian throughflow, its variability and centennial change
Ming Feng1, Ming Feng2, Ningning Zhang3, Qinyan Liu4, Susan Wijffels2, Susan Wijffels1
01 Dec 2018 - Geoscience Letters

Abstract:

The Indonesian Throughflow (ITF) is an important component of the upper cell of the global overturning circulation that provides a low-latitude pathway for warm, fresh waters from the Pacific to enter the Indian Ocean. Variability and changes of the ITF have significant impacts on Indo-Pacific oceanography and global climate.... The Indonesian Throughflow (ITF) is an important component of the upper cell of the global overturning circulation that provides a low-latitude pathway for warm, fresh waters from the Pacific to enter the Indian Ocean. Variability and changes of the ITF have significant impacts on Indo-Pacific oceanography and global climate. In this paper, the observed features of the ITF and its interannual to decadal variability are reviewed, and processes that influence the centennial change of the ITF under the influence of the global warming are discussed. The ITF flows across a region that comprises the intersection of two ocean waveguides—those of the equatorial Pacific and equatorial Indian Ocean. The ITF geostrophic transport is stronger during La Ninas and weaker during El Ninos due to the influences through the Pacific waveguide. The Indian Ocean wind variability associated with the Indian Ocean Dipole (IOD) in many years offsets the Pacific ENSO influences on the ITF geostrophic transport during the developing and mature phases of El Nino and La Nina through the Indian Ocean waveguide, due to the co-varying IOD variability with ENSO. Decadal and multi-decadal changes of the geostrophic ITF transport have been revealed: there was a weakening change from the mid-1970s climate regime shift followed by a strengthening trend of about 1Sv every 10 year during 1984–2013. These decadal changes are mostly due to the ITF responses to decadal variations of the trade winds in the Pacific. Thus, Godfrey’s Island Rule, as well as other ITF proxies, appears to be able to quantify decadal variations of the ITF. Climate models project a weakening trend of the ITF under the global warming. Both climate models and downscaled ocean model show that this ITF weakening is not directly associated with the changes of the trade winds in the Pacific into the future, and the reduction of deep upwelling in the Pacific basin is mainly responsible for the ITF weakening. There is a need to amend the Island Rule to take into account the contributions from the overturning circulation which the current ITF proxies fail to capture. The implication of a weakened ITF on the Indo-Pacific Ocean circulation still needs to be assessed. read more read less

Topics:

Indian Ocean Dipole (58%)58% related to the paper, Ocean current (52%)52% related to the paper, La Niña (52%)52% related to the paper, Climate change (50%)50% related to the paper
View PDF
78 Citations
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Frequently asked questions

1. Can I write Geoscience Letters in LaTeX?

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

2. Do you follow the Geoscience Letters guidelines?

Yes, the template is compliant with the Geoscience Letters 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 Geoscience Letters?

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 Geoscience Letters citation style.

4. Can I use the Geoscience Letters 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 Geoscience Letters.

5. Can I use a manuscript in Geoscience Letters 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 Geoscience Letters that you can download at the end.

6. How long does it usually take you to format my papers in Geoscience Letters?

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

7. Where can I find the template for the Geoscience Letters?

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 Geoscience Letters'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 Geoscience Letters'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. Geoscience Letters an online tool or is there a desktop version?

SciSpace's Geoscience Letters 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 Geoscience Letters?

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 Geoscience Letters?”

11. What is the output that I would get after using Geoscience Letters?

After writing your paper autoformatting in Geoscience Letters, you can download it in multiple formats, viz., PDF, Docx, and LaTeX.

12. Is Geoscience Letters'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 Geoscience Letters?

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 Geoscience Letters. 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 Geoscience Letters?

The 5 most common citation types in order of usage for Geoscience Letters 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 Geoscience Letters?

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 Geoscience Letters's guidelines and download the same in Word, PDF and LaTeX formats? Give us a try!.

16. Can I download Geoscience Letters 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 Geoscience Letters Endnote style according to Elsevier guidelines.

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