@InProceedings{ArrasReseWick:2021:HoGPRa,
author = "Arras, C. and Resende, Laysa Cristina Ara{\'u}jo and Wickert,
J.",
affiliation = "{German Research Center for Geosciences (GFZ)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {German Research
Center for Geosciences (GFZ)}",
title = "Investigating the Earth’s lower ionosphere from space: How GPS
radio occultation profiles provide a global overview on sporadic E
layer occurrence",
year = "2021",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 8. (SBGEA)",
abstract = "The GPS radio occultation (RO) technique established successfully
during the last two decades and evolved into a valuable
application for precise atmospheric and ionospheric profiling. GPS
RO signals are very sensitive to vertical changes in the electron
density in the Earths ionosphere. This issue becomes visible as
strong fluctuations in e.g. signal-to-noise ratio recordings,
which allow detecting sporadic E layers in the lower ionosphere.
Due to the geometry of the GPS RO technique, it enables for the
first time receiving a global and comprehensive picture of
sporadic E layer occurrence and properties in a high spatial
resolution. Sporadic E (Es) layers are thin sheets of enhanced
electron density occurring in the lower ionospheric E region,
preferably between 95 and 120 km. It is widely accepted that Es
formation at low- and midlatitudes is due to the wind shear
mechanism when the ionized metallic particles of meteoric origin
interact with the lower thermospheric neutral wind field. In polar
and equatorial electric fields play and additional important role
in the Es layer formation process. In this presentation, we like
to give an overview on global sporadic E characteristics. We will
demonstrate the varying behavior of this phenomenon at different
latitudinal regions and we will illustrate that the Es formation
results from complex coupling processes in the
thermosphere-ionosphere-magnetosphere system. We will discuss
several geophysical parameters such as tidal winds in the upper
atmosphere, the presence of metallic ions and the Earths magnetic
field influencing the Es formation.",
conference-location = "Online",
conference-year = "22-26 mar.",
language = "en",
targetfile = "arras_2021.pdf",
urlaccessdate = "05 jun. 2024"
}