Example of Journal of Space Weather and Space Climate format
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Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format
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Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format Example of Journal of Space Weather and Space Climate format
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open access Open Access

Journal of Space Weather and Space Climate — Template for authors

Publisher: EDP Sciences
Categories Rank Trend in last 3 yrs
Space and Planetary Science #30 of 97 down down by 8 ranks
Atmospheric Science #40 of 124 down down by 19 ranks
journal-quality-icon Journal quality:
Good
calendar-icon Last 4 years overview: 184 Published Papers | 898 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 12/07/2020
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Top papers
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FAQ

Related Journals

open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.6
SJR: 0.682
SNIP: 1.274
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Elsevier

Quality:  
Good
CiteRatio: 3.2
SJR: 0.515
SNIP: 0.994
open access Open Access

IEEE

Quality:  
High
CiteRatio: 7.2
SJR: 1.246
SNIP: 1.579
open access Open Access

IEEE

Quality:  
High
CiteRatio: 3.7
SJR: 0.396
SNIP: 1.133

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.

3.095

10% from 2018

Impact factor for Journal of Space Weather and Space Climate from 2016 - 2019
Year Value
2019 3.095
2018 2.821
2017 2.333
2016 2.446
graph view Graph view
table view Table view

4.9

8% from 2019

CiteRatio for Journal of Space Weather and Space Climate from 2016 - 2020
Year Value
2020 4.9
2019 5.3
2018 3.8
2017 5.7
2016 4.8
graph view Graph view
table view Table view

insights Insights

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

insights Insights

  • CiteRatio of this journal has decreased by 8% 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.

1.027

22% from 2019

SJR for Journal of Space Weather and Space Climate from 2016 - 2020
Year Value
2020 1.027
2019 0.84
2018 0.74
2017 1.439
2016 1.264
graph view Graph view
table view Table view

1.359

12% from 2019

SNIP for Journal of Space Weather and Space Climate from 2016 - 2020
Year Value
2020 1.359
2019 1.21
2018 1.25
2017 2.302
2016 1.776
graph view Graph view
table view Table view

insights Insights

  • SJR of this journal has increased by 22% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has increased by 12% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Journal of Space Weather and Space Climate

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EDP Sciences

Journal of Space Weather and Space Climate

Approved by publishing and review experts on SciSpace, this template is built as per for Journal of Space Weather and Space Climate formatting guidelines as mentioned in EDP Sciences author instructions. The current version was created on 12 Jul 2020 and has been used by 911 authors to write and format their manuscripts to this journal.

Atmospheric Science

Space and Planetary Science

Earth and Planetary Sciences

i
Last updated on
12 Jul 2020
i
ISSN
2115-7251
i
Acceptance Rate
Not provided
i
Frequency
Not provided
i
Open Access
No
i
Sherpa RoMEO Archiving Policy
Green faq
i
Plagiarism Check
Available via Turnitin
i
Endnote Style
Download Available
i
Bibliography Name
Vancouver
i
Citation Type
Numbered
[25]
i
Bibliography Example
Blonder GE, Tinkham M, Klapwijk TM. Transition from metallic to tunneling regimes in superconducting microconstrictions: Excess current, charge imbalance, and supercurrent con-version. Phys Rev B. 1982;25(7):4515–4532. Available from: 10.1103/PhysRevB.25.4515.

Top papers written in this journal

open accessOpen access Journal Article DOI: 10.1051/SWSC/2014004
The International Reference Ionosphere 2012 – a model of international collaboration

Abstract:

The International Reference Ionosphere (IRI) project was established jointly by the Committee on Space Research (COSPAR) and the International Union of Radio Science (URSI) in the late sixties with the goal to develop an international standard for the specification of plasma parameters in the Earth’s ionosphere. COSPAR needed... The International Reference Ionosphere (IRI) project was established jointly by the Committee on Space Research (COSPAR) and the International Union of Radio Science (URSI) in the late sixties with the goal to develop an international standard for the specification of plasma parameters in the Earth’s ionosphere. COSPAR needed such a specification for the evaluation of environmental effects on spacecraft and experiments in space, and URSI for radiowave propagation studies and applications. At the request of COSPAR and URSI, IRI was developed as a data-based model to avoid the uncertainty of theory-based models which are only as good as the evolving theoretical understanding. Being based on most of the available and reliable observations of the ionospheric plasma from the ground and from space, IRI describes monthly averages of electron density, electron temperature, ion temperature, ion composition, and several additional parameters in the altitude range from 60 km to 2000 km. A working group of about 50 international ionospheric experts is in charge of developing and improving the IRI model. Over time as new data became available and new modeling techniques emerged, steadily improved editions of the IRI model have been published. This paper gives a brief history of the IRI project and describes the latest version of the model, IRI-2012. It also briefly discusses efforts to develop a real-time IRI model. The IRI homepage is at http://IRImodel.org. read more read less

Topics:

International Reference Ionosphere (63%)63% related to the paper, Committee on Space Research (60%)60% related to the paper
View PDF
572 Citations
open accessOpen access Journal Article DOI: 10.1051/SWSC/2018020
EUHFORIA: European heliospheric forecasting information asset
Jens Pomoell1, Stefaan Poedts2

Abstract:

The implementation and first results of the new space weather forecasting-targeted inner heliosphere model “European heliospheric forecasting information asset” (EUHFORIA) are presented. EUHFORIA consists of two major components: a coronal model and a heliosphere model including coronal mass ejections. The coronal model provi... The implementation and first results of the new space weather forecasting-targeted inner heliosphere model “European heliospheric forecasting information asset” (EUHFORIA) are presented. EUHFORIA consists of two major components: a coronal model and a heliosphere model including coronal mass ejections. The coronal model provides data-driven solar wind plasma parameters at 0.1 AU by constructing a magnetic field model of the coronal large-scale magnetic field and employing empirical relations to determine the plasma state such as the solar wind speed and mass density. These are then used as boundary conditions to drive a three-dimensional time-dependent magnetohydrodynamics model of the inner heliosphere up to 2 AU. CMEs are injected into the ambient solar wind modeled using the cone model, with their parameters obtained from fits to imaging observations. In addition to detailing the modeling methodology, an initial validation run is presented. The results feature a highly dynamic heliosphere that the model is able to capture in good agreement with in situ observations. Finally, future horizons for the model are outlined. read more read less

Topics:

Solar wind (59%)59% related to the paper, Coronal mass ejection (59%)59% related to the paper, Heliosphere (58%)58% related to the paper, Space weather (57%)57% related to the paper, Interplanetary medium (52%)52% related to the paper
View PDF
266 Citations
open accessOpen access Journal Article DOI: 10.1051/SWSC/2013053
The 1859 space weather event revisited: limits of extreme activity
Edward W. Cliver1, W. F. Dietrich2

Abstract:

The solar flare on 1 September 1859 and its associated geomagnetic storm remain the standard for an extreme solar-terrestrial event. The most recent estimates of the flare soft X-ray (SXR) peak intensity and D st magnetic storm index for this event are: SXR class = X45 (±5) (vs. X35 (±5) for the 4 November 2003 flare) and min... The solar flare on 1 September 1859 and its associated geomagnetic storm remain the standard for an extreme solar-terrestrial event. The most recent estimates of the flare soft X-ray (SXR) peak intensity and D st magnetic storm index for this event are: SXR class = X45 (±5) (vs. X35 (±5) for the 4 November 2003 flare) and minimum D st = −900 (+50, −150) nT (vs. −825 to −900 nT for the great storm of May 1921). We have no direct evidence of an associated solar energetic proton (SEP) event but a correlation between >30 MeV SEP fluence (F30 ) and flare size based on modern data yields a best guess F30 value of ~1.1 × 1010 pr cm−2 (with the ±1σ uncertainty spanning a range from ~109 –1011  pr cm−2 ) for a composite (multi-flare plus shock) 1859 event. This value is approximately twice that of estimates/measurements – ranging from ~5–7 × 109  pr cm−2 – for the largest SEP episodes (July 1959, November 1960, August 1972) in the modern era. read more read less

Topics:

Solar flare (56%)56% related to the paper, Geomagnetic storm (53%)53% related to the paper, Flare (52%)52% related to the paper
View PDF
238 Citations
open accessOpen access Journal Article DOI: 10.1051/SWSC/2015001
The DTM-2013 thermosphere model

Abstract:

Aims – The Drag Temperature Model (DTM) is a semi-empirical model describing the temperature, density, and composition of the Earth’s thermosphere. DTM2013 was developed in the framework of the Advanced Thermosphere Modelling and Orbit Prediction project (ATMOP). It is evaluated and compared with DTM2009, the pre-ATMOP benchm... Aims – The Drag Temperature Model (DTM) is a semi-empirical model describing the temperature, density, and composition of the Earth’s thermosphere. DTM2013 was developed in the framework of the Advanced Thermosphere Modelling and Orbit Prediction project (ATMOP). It is evaluated and compared with DTM2009, the pre-ATMOP benchmark, and the Committe on Space Research (COSPAR) reference model for atmospheric drag JB2008.Methods – The total density data used in this study, including the high-resolution CHAMP, GRACE and GOCE data, cover the 200–900 km altitude range and all solar activities. DTM2013 was constructed with the data assimilated in DTM2009, but with more GRACE data, and low-altitude GOCE data in particular. The solar activity proxy, F10.7 in DTM2009, has been replaced with F30. The bias and precision of the models is evaluated by comparing to the observations according to a metric, which consists of computing mean, RMS, and correlation. Secondly, the residuals are binned, which procedure aids in revealing specific model errors.Results – This evaluation shows that DTM2013 is the least biased and most precise model for the data that were assimilated. Comparison to independent density data shows that it is also the most accurate model overall. It is a significant improvement over DTM2009 under all conditions and at all altitudes, but the largest improvements are obtained at low altitude thanks to GOCE data. The precision of JB2008 decreases with altitude, which is due to its modeling of variations in local solar time and seasons in particular of the exospheric temperature rather than modeling these variations for the individual constituents. read more read less

Topics:

Thermosphere (54%)54% related to the paper, Solar time (50%)50% related to the paper
View PDF
151 Citations
open accessOpen access Journal Article DOI: 10.1051/SWSC/2013025
Space weather challenges of the polar cap ionosphere
Joran Moen1, Kjellmar Oksavik2, Lucilla Alfonsi3, Yvonne Daabakk1, V. Romano3, Luca Spogli3

Abstract:

This paper presents research on polar cap ionosphere space weather phenomena conducted during the European Cooperation in Science and Technology (COST) action ES0803 from 2008 to 2012. The main part of the work has been directed toward the study of plasma instabilities and scintillations in association with cusp flow channels... This paper presents research on polar cap ionosphere space weather phenomena conducted during the European Cooperation in Science and Technology (COST) action ES0803 from 2008 to 2012. The main part of the work has been directed toward the study of plasma instabilities and scintillations in association with cusp flow channels and polar cap electron density structures/patches, which is considered as critical knowledge in order to develop forecast models for scintillations in the polar cap. We have approached this problem by multi-instrument techniques that comprise the EISCAT Svalbard Radar, SuperDARN radars, in-situ rocket, and GPS scintillation measurements. The Discussion section aims to unify the bits and pieces of highly specialized information from several papers into a generalized picture. The cusp ionosphere appears as a hot region in GPS scintillation climatology maps. Our results are consistent with the existing view that scintillations in the cusp and the polar cap ionosphere are mainly due to multi-scale structures generated by instability processes associated with the cross-polar transport of polar cap patches. We have demonstrated that the SuperDARN convection model can be used to track these patches backward and forward in time. Hence, once a patch has been detected in the cusp inflow region, SuperDARN can be used to forecast its destination in the future. However, the high-density gradient of polar cap patches is not the only prerequisite for high-latitude scintillations. Unprecedented high-resolution rocket measurements reveal that the cusp ionosphere is associated with filamentary precipitation giving rise to kilometer scale gradients onto which the gradient drift instability can operate very efficiently. Cusp ionosphere scintillations also occur during IMF B Z north conditions, which further substantiates that particle precipitation can play a key role to initialize plasma structuring. Furthermore, the cusp is associated with flow channels and strong flow shears, and we have demonstrated that the Kelvin-Helmholtz instability process may be efficiently driven by reversed flow events. read more read less

Topics:

Space weather (52%)52% related to the paper, Ionosphere (51%)51% related to the paper
View PDF
120 Citations
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Journal of Space Weather and Space Climate format uses Vancouver citation style.

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Frequently asked questions

1. Can I write Journal of Space Weather and Space Climate in LaTeX?

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

2. Do you follow the Journal of Space Weather and Space Climate guidelines?

Yes, the template is compliant with the Journal of Space Weather and Space Climate 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 Journal of Space Weather and Space Climate?

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 Journal of Space Weather and Space Climate citation style.

4. Can I use the Journal of Space Weather and Space Climate 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 Journal of Space Weather and Space Climate.

5. Can I use a manuscript in Journal of Space Weather and Space Climate 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 Journal of Space Weather and Space Climate that you can download at the end.

6. How long does it usually take you to format my papers in Journal of Space Weather and Space Climate?

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12. Is Journal of Space Weather and Space Climate'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 Journal of Space Weather and Space Climate?

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 Journal of Space Weather and Space Climate. 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 Journal of Space Weather and Space Climate?

The 5 most common citation types in order of usage for Journal of Space Weather and Space Climate 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 Journal of Space Weather and Space Climate?

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16. Can I download Journal of Space Weather and Space Climate 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 Journal of Space Weather and Space Climate Endnote style according to Elsevier guidelines.

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