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A measure of ionospheric irregularities:zonal velocity and its implications for L-band scintillation at low-latitudes

Claudio Cesaroni Massimo Cafaro Luca Spogli Giorgiana De Franceschi Juliana Garrido Damaceno Marcin Grzesiak Bruno Vani Joao Francisco Galera Monico Vincenzo Romano Lucilla Alfonsi

地球与行星物理(英文)2021,Vol.5Issue(5):450-461,12.
地球与行星物理(英文)2021,Vol.5Issue(5):450-461,12.DOI:10.26464/epp2021042

A measure of ionospheric irregularities:zonal velocity and its implications for L-band scintillation at low-latitudes

A measure of ionospheric irregularities:zonal velocity and its implications for L-band scintillation at low-latitudes

Claudio Cesaroni 1Massimo Cafaro 2Luca Spogli 1Giorgiana De Franceschi 1Juliana Garrido Damaceno 3Marcin Grzesiak 1Bruno Vani 1Joao Francisco Galera Monico 4Vincenzo Romano 5Lucilla Alfonsi6

作者信息

  • 1. Istituto Nazionale di Geofisica e Vulcanologia,Italy
  • 2. University of Salento,Italy
  • 3. SpacEarth Technology,Italy
  • 4. Space Research Centre of the Polish Academy of Sciences,Poland
  • 5. Instituto Federal de Educa??o,Ciência e Tecnologia de S?o Paulo,Brazil
  • 6. Universidade Estadual Paulista"Julio de Mesquita Filho",Brazil
  • 折叠

摘要

关键词

ionospheric irregularities/GNSS/scintillation/plasma drift velocity/low-latitude ionosphere/spaced receivers/Equatorial Plasma Bubbles

Key words

ionospheric irregularities/GNSS/scintillation/plasma drift velocity/low-latitude ionosphere/spaced receivers/Equatorial Plasma Bubbles

引用本文复制引用

Claudio Cesaroni,Massimo Cafaro,Luca Spogli,Giorgiana De Franceschi,Juliana Garrido Damaceno,Marcin Grzesiak,Bruno Vani,Joao Francisco Galera Monico,Vincenzo Romano,Lucilla Alfonsi..A measure of ionospheric irregularities:zonal velocity and its implications for L-band scintillation at low-latitudes[J].地球与行星物理(英文),2021,5(5):450-461,12.

基金项目

This Micro Test Area experiment and the development of the Grzesiak et al.(2018)model have been conducted in the frame of the CALIBRA(Countering GNSS high Accuracy applications Limita-tions due to Ionospheric disturbances in BRAzil)project,which was submitted within the call FP7-GALILEO-2011-GSA-1a and GNSS-SP,funded by FAPESP(Process 06/04008-2).Improvement of the the Grzesiak et al.(2018)model has been realized in the frame of the TREASURE(Training REsearch and Ap-plications Network to Support the Ultimate Real-Time High Accur-acy EGNSS Solution)project,which received funding from the European Union's Horizon 2020 research and innovation pro-gramme under the Marie Sk?odowska-Curie Actions grant agree-ment No 722023. (2018)

地球与行星物理(英文)

OACSCDEI

2096-3955

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