STI Seminar: Tuesday 7 March 2023 at 2:30 pm (CET)
STI Secretariat
sti at ictp.it
Fri Mar 3 12:24:27 CET 2023
_____________
STI seminar
___________
You are most cordially invited to a hybrid seminar organized by the ICTP
Science Technology and Innovation Unit (STI Unit)
** * * Tuesday, 7 March 2023 at 14:30 (Rome/CET time) *** * **
IN PERSON: Stasi Seminar Room (Leonardo Building, second floor)
VIRTUAL: register in advance
at:https://zoom.us/meeting/register/tJEocOmqrjwjHdTyN3de6NX5lPuYAioC22gO<https://zoom.us/meeting/register/tJEocOmqrjwjHdTyN3de6NX5lPuYAioC22gO>/
/After registering, you will receive a confirmation email containing
information about joining the seminar.
Speaker: *Alessio PIGNALBERI, *Istituto Nazionale di Geofisica e
Vulcanologia (INGV), Rome, Italy
Title:***Modelling the topside ionosphere: improving NeQuick through
radio occultation data *
_Abstract:_The topside ionosphere is the region of the upper atmosphere
extending from the F2-layer peak to the plasmasphere. This is the
environment where low-Earth-orbit satellites live, and it also highly
affects the propagation of GNSS signals. Hence, its description has
gained more and more importance in the last years. However, the
modelling of the electron density distribution in this region represents
still a challenge for the ionospheric community. This presentation
describes novel methodologies developed to improve the NeQuick model
topside ionosphere formulation by taking advantage of electron density
observations by radio occultation. The NeQuick topside formulation is
mathematically inverted to derive a fully analytical expression of the
topside effective scale height, which is then used to optimize the
NeQuick topside parameters. Through a large dataset of radio occultation
observations, we highlighted the main spatial, diurnal, seasonal, solar
and magnetic activity variations of the NeQuick topside parameters, and
provided a first application for topside ionosphere modelling.
_
_
_Bio_: Alessio Pignalberi obtained the PhD degree in Geophysics from the
University of Bologna in 2019, and from 2019 onwards he is post-doctoral
fellow at the Italian National Institute of Geophysics and Vulcanology
(INGV) in Rome. Since his PhD, he is deeply involved in the field of
ionosphere modelling by improving empirical climatological models like
the International Reference Ionosphere (IRI) and NeQuick. He is the main
author of the IRI UP data assimilation method, and most of his research
activity is currently devoted to the modelling of the topside
ionosphere. He was awarded with the International Union of Radio Science
(URSI) Young Scientist Award in 2017 and 2021.
--
Nicoletta Ivanissevich (Ms.)
Secretariat,
STI - Science, Technology and Innovation Unit
The Abdus Salam International Centre for Theoretical Physics
Strada Costiera, 11
I-34151 Trieste
Italy
Phone: +39-040-2240.383
STI Webpage:https://www.ictp.it/research/sti.aspx
Email:sti at ictp.it
--
More information about the science-ts
mailing list