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verified SJR 0,76 · Q2 • database Scopus / SJR & Web of Science indexed
Solar Physics
Netherlands · Springer Netherlands
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Solar Physics

Solar Physics is a journal indexed in SJR in Astronomy and Astrophysics and Space and Planetary Science with an H index of 134. It has a price of 2690 €. It has an SJR impact factor of 0,76 and it has a best quartile of Q2. It is published in English. It has an SJR impact factor of 0,76.

Solar Physics focuses its scope in these topics and keywords: solar, cme, coronal, type, shock, energetic, waves, response, regions, radio, ...

ISSN: 0038-0938
Publisher: Springer Netherlands
Category: Astronomy and Astrophysics
Indexation: verifiedScopus / SJR verifiedWeb of Science
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schedule CountryOfPapers database fields
SJR Impact Factor trending_up
0,76 Q2
H-index 134
Acceptance rate pie_chart
23% Selective
Source Acceptance_Rate
Time to publication hourglass_top
NPD
Field NPD
Publication cost (APC) payments
2.690 € Subscription
Non-OA path 0 €

Metrics

Scimago and CountryOfPapers database fields

Scopus / SJR Web of Science

SJR Impact

0,76

H-index

134

Docs (year)

166

Docs 3y

476

Total refs

8110

Cites 3y

1147

Citable 3y

468

Cites/Doc 2y

2.26

Ref/Doc

48.86

Immediate OA

2690 €

Embargoed OA

NPD

Non OA / Submission

0 €

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Best articles by citations

Multi-Scale Analysis of the Geomagnetic Symmetric Index (sym)

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The White-Light Limb Flare of 16 August 1989 and its Chromospheric Counterpart

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Statistical Characteristics of CMEs and Flares Associated with Solar Type II Radio Bursts

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Sky Brightness Measurements at Haleakala, 1955-2002

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Prominence atlas in the SUMER range 800-1250 u: -I. Observations, data reduction and preliminary results

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Predicting the Arrival Time of Shock Passages at Earth

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On the validity of application of the radial approximation for the photospheric field

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On the Dynamic Disconnection of Rising Omega Loops

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New Evidence for Long-Term Persistence in the Sun's Activity

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A Transfer Function Model for the Sunspot Cycle

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Linear and non-linear MHD wave propagation in steady-state magnetic cylinders

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HALL-MHD turbulence in the Solar atmosphere

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SHOW MORE ARTICLES

Flare-related changes in the profiles of six photospheric spectral lines

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Fip Enhancement by Alfven Ionization

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Extreme Ultraviolet Emission Lines of ca xv in Solar and Laboratory Spectra

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Extinction and Sky Brightness at Two Solar Observatories

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Correlation between Expansion Rate of the Coronal Magnetic Field and Solar Wind Speed in a Solar Activity Cycle

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Alignment of Fabry-Perot Interferometer Plates in a Solar Vector Magnetograph

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