The Atmospheric Imaging Assembly (AIA) provides multiple simultaneous high-resolution full-disk images of the corona and transition region up to 0.5 R ⊙ above the solar limb with 1.5-arcsec spatial resolution and 12-second temporal resolution. The AIA consists of four telescopes that employ normal-incidence, multilayer-coated optics to provide narrow-band imaging of seven extreme ultraviolet (EUV) band…
Solar Physics Template
Write in a clean editor, then format for Solar Physics in one click — DocuGuru applies the official Springer Nature template with superscript references and exports a submission-ready PDF plus the editable LaTeX source. Free to start.
About the Solar Physics format
Solar Physics is a peer-reviewed journal published by Springer Nature, covering Solar and Space Plasma Dynamics, Ionosphere and magnetosphere dynamics, Astro and Planetary Science.
| Publisher | Springer Nature |
|---|---|
| Reference style | Superscript numbered (Nature) Superscript — small raised numerals in the text 1. Smith, A., Jones, B. & Lee, C. A representative article title. Solar Physics 12, 45–58 (2023).
Formats any DOI in Solar Physics style. No sign-up. |
| Publishes research in | Solar and Space Plasma Dynamics Ionosphere and magnetosphere dynamics Astro and Planetary Science Stellar, planetary, and galactic studies Geomagnetism and Paleomagnetism Studies |
| ISSN | 0038-0938 |
| Citation impact (2-yr) | 2.44 |
| h-index | 201 |
| i10-index | 6,963 |
| Total citations | 368,525 |
| Article processing charge | $3,690 |
| Top institutions publishing here | Goddard Space Flight Center |
| Journal website | www.springer.com |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Papers published in Solar Physics per year
Citation impact of Solar Physics by publication year
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Most-cited papers in Solar Physics
The Solar Dynamics Observatory (SDO) was launched on 11 February 2010 at 15:23 UT from Kennedy Space Center aboard an Atlas V 401 (AV-021) launch vehicle. A series of apogee-motor firings lifted SDO from an initial geosynchronous transfer orbit into a circular geosynchronous orbit inclined by 28° about the longitude of the SDO-dedicated ground station…
The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal…