دورية أكاديمية

ScintPi 2.0 and 3.0: low-cost GNSS-based monitors of ionospheric scintillation and total electron content

التفاصيل البيبلوغرافية
العنوان: ScintPi 2.0 and 3.0: low-cost GNSS-based monitors of ionospheric scintillation and total electron content
المؤلفون: Josemaria Gomez Socola, Fabiano S. Rodrigues
المصدر: Earth, Planets and Space, Vol 74, Iss 1, Pp 1-18 (2022)
بيانات النشر: SpringerOpen, 2022.
سنة النشر: 2022
المجموعة: LCC:Geography. Anthropology. Recreation
LCC:Geodesy
LCC:Geology
مصطلحات موضوعية: Ionosphere, Scintillation, Total electron content, TEC, Monitor, Scintpi, Geography. Anthropology. Recreation, Geodesy, QB275-343, Geology, QE1-996.5
الوصف: Abstract We have devoted efforts to the development and performance evaluation of new low-cost ionospheric instruments for studies that require distributed observations and for educational and citizen science initiatives. Here, we report results of some of these efforts. More specifically, we describe the design of new ionospheric sensors based on Global Navigation Satellite System (GNSS) receivers and single-board computers. The first sensor (ScintPi 2.0) is a multi-constellation, single-frequency ionospheric scintillation monitor. The second sensor (ScintPi 3.0) is a multi-constellation, dual-frequency ionospheric scintillation and total electron content (TEC) monitor. Both sensors were created using Raspberry Pi computers and off-the-shelf GNSS receivers. While they are not intended to fully replace commercial ionospheric monitors, they cost a fraction of their price and can be used in various scientific applications. In addition to describing these new sensors, we present examples of observations made by ScintPi 3.0 deployed in Presidente Prudente, Brazil (22.12 S, 51.41 W, − 17.67° dip latitude). These examples show the ability of our system to detect scintillation events and TEC depletions such as those associated with equatorial plasma bubbles. Additionally, our observations were made in parallel with a commercial receiver (Septentrio PolaRx5S), which allowed an evaluation of the scintillation and TEC measurements provided by our system. The comparison shows that ScintPi 3.0 can provide estimates of the amplitude scintillation index (S4) and TEC that are in excellent agreement with those provided by PolaRx5S. We also show an example of the application of ScintPi 3.0 in distributed observations of ionospheric irregularities and scintillation over South America. Graphical Abstract
نوع الوثيقة: article
وصف الملف: electronic resource
اللغة: English
تدمد: 1880-5981
Relation: https://doaj.org/toc/1880-5981
DOI: 10.1186/s40623-022-01743-x
URL الوصول: https://doaj.org/article/9870412a123141118d657c0c389ea819
رقم الأكسشن: edsdoj.9870412a123141118d657c0c389ea819
قاعدة البيانات: Directory of Open Access Journals
الوصف
تدمد:18805981
DOI:10.1186/s40623-022-01743-x