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Effect of Solar Activities to the Earth's Atmosphere
This special issue belongs to the section “Upper Atmosphere“.
Special Issue Information
Dear Colleagues,
Solar activity has a strong influence on Earth's atmosphere. The Sun can affect the atmosphere in many ways, including solar flares, variations in solar X-ray and ultraviolet irradiance, release of intense fluxes of solar energetic particles, and coronal mass ejections resulting in auroral phenomena and geomagnetic storms. The contribution of these factors to the overall response of the atmosphere to solar activity requires further comprehensive studies. The occurrence of all these phenomena increases with solar activity. A solar maximum phase of the 25th solar cycle has begun in 2023 with several strong solar events, which have caused major geomagnetic storms. During some of them, anomalous phenomena occurred such as rare mid-latitude aurora.
Studying the response of Earth’s atmosphere to solar activity is of great practical importance. Increased solar radiation and occurrence of geomagnetic storms may cause disturbances in the density of atmospheric gases that result in a greater drag effect, which reduces the lifetime of satellites. Hard electromagnetic radiation produced by solar flares may disturb the ionosphere and, thus, interfere with radio signals, resulting in the degradation of communication quality. More and more accurate knowledge is needed for the stable operation of satellites, telecommunications, etc.
The Special Issue is open to research on the influence of solar activity on the Earth’s atmosphere and the elucidation of various aspects of the mechanism and consequences of its influence.
Additionally, studies of atmospheric and ionospheric phenomena associated with geomagnetic storms at the beginning of the solar maximum of the current 25th solar cycle are welcome.
Dr. Alla Suvorova
Dr. Alexei Dmitriev
Guest Editors
Manuscript Submission Information
Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 250 words) can be sent to the Editorial Office for assessment.
Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Atmosphere is an international peer-reviewed open access monthly journal published by MDPI.
Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 2400 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.
Keywords
- solar activity
- solar flares
- solar energetic particles
- solar irradiance
- solar‒terrestrial coupling
- geomagnetic activity
- ionospheric disturbances
- atmospheric perturbations
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