GNSS High Rate Data for Research of the Ionosphere

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Space Science".

Deadline for manuscript submissions: closed (31 December 2021) | Viewed by 656

Special Issue Editors


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Guest Editor
Institute of Solar and Terrestrial Physics, Siberian Branch of Russian Academy of Sciences, Irkutsk 664033, Russia
Interests: remote sensing; science education; global navigation satellite systems; ionosphere; space weather
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Special Issue Information

Dear Colleagues,

GNSS data of high-rate sampling is becoming increasingly available worldwide. It provides new opportunities to achieve better results in researching the ionosphere. Accuracy, efficiency, and reliability of standard ionospheric indices and parameters (S4, σφ, ROTI, TEC et al) depend on the integration time, sampling rate, de-trending and filtering procedures as well as on the receiver hardware and software architecture. The first important question is this: Is the data sampling rate high enough to ensure that all the ionospheric events are derived from the data? The second crucial question is: Are you certain in your results if your primary data was derived from the GNSS receiver like from a “black box”? The aim of this Special Issue is to present the latest state-of-the-art findings which seek to answer these questions.

You may choose our Joint Special Issue in Remote Sensing.

Prof. Vladislav Demyanov
Prof. Dr. Shuanggen Jin
Guest Editors

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Keywords

  • Ionosphere TEC
  • GNSS Ionosphere
  • Remote Sensing
  • Traveling Ionospheric Disturbances
  • Magnetic Storms
  • Ionospheric Scintillation
  • Scintillation Modelling
  • Ionospheric Scintillation Indices
  • High-rate GNSS Data

Related Special Issue

Published Papers

There is no accepted submissions to this special issue at this moment.
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