TY - JOUR
T1 - Lower-Thermosphere-ionosphere (LTI) quantities
T2 - Current status of measuring techniques and models
AU - Palmroth, Minna
AU - Grandin, Maxime
AU - Sarris, Theodoros
AU - Doornbos, Eelco
AU - Tourgaidis, Stelios
AU - Aikio, Anita
AU - Buchert, Stephan
AU - Clilverd, Mark A.
AU - Dandouras, Iannis
AU - Heelis, Roderick
AU - Hoffmann, Alex
AU - Ivchenko, Nickolay
AU - Kervalishvili, Guram
AU - Knudsen, David J.
AU - Kotova, Anna
AU - Liu, Han Li
AU - Malaspina, David M.
AU - March, Gönther
AU - Marchaudon, Aurélie
AU - Marghitu, Octav
AU - Matsuo, Tomoko
AU - Miloch, Wojciech J.
AU - Moretto-Jørgensen, Therese
AU - Mpaloukidis, Dimitris
AU - Olsen, Nils
AU - Papadakis, Konstantinos
AU - Pfaff, Robert
AU - Pirnaris, Panagiotis
AU - Siemes, Christian
AU - Stolle, Claudia
AU - Suni, Jonas
AU - Van Den Ijssel, Jose
AU - Verronen, Pekka T.
AU - Visser, Pieter
AU - Yamauchi, Masatoshi
N1 - Funding Information:
Financial support. This research has been supported by the
Publisher Copyright:
© 2021 American Society of Mechanical Engineers (ASME). All rights reserved.
PY - 2021
Y1 - 2021
N2 - The lower-Thermosphere-ionosphere (LTI) system consists of the upper atmosphere and the lower part of the ionosphere and as such comprises a complex system coupled to both the atmosphere below and space above. The atmospheric part of the LTI is dominated by laws of continuum fluid dynamics and chemistry, while the ionosphere is a plasma system controlled by electromagnetic forces driven by the magnetosphere, the solar wind, as well as the wind dynamo. The LTI is hence a domain controlled by many different physical processes. However, systematic in situ measurements within this region are severely lacking, although the LTI is located only 80 to 200 km above the surface of our planet. This paper reviews the current state of the art in measuring the LTI, either in situ or by several different remote-sensing methods. We begin by outlining the open questions within the LTI requiring high-quality in situ measurements, before reviewing directly observable parameters and their most important derivatives. The motivation for this review has arisen from the recent retention of the Daedalus mission as one among three competing mission candidates within the European Space Agency (ESA) Earth Explorer 10 Programme. However, this paper intends to cover the LTI parameters such that it can be used as a background scientific reference for any mission targeting in situ observations of the LTI..
AB - The lower-Thermosphere-ionosphere (LTI) system consists of the upper atmosphere and the lower part of the ionosphere and as such comprises a complex system coupled to both the atmosphere below and space above. The atmospheric part of the LTI is dominated by laws of continuum fluid dynamics and chemistry, while the ionosphere is a plasma system controlled by electromagnetic forces driven by the magnetosphere, the solar wind, as well as the wind dynamo. The LTI is hence a domain controlled by many different physical processes. However, systematic in situ measurements within this region are severely lacking, although the LTI is located only 80 to 200 km above the surface of our planet. This paper reviews the current state of the art in measuring the LTI, either in situ or by several different remote-sensing methods. We begin by outlining the open questions within the LTI requiring high-quality in situ measurements, before reviewing directly observable parameters and their most important derivatives. The motivation for this review has arisen from the recent retention of the Daedalus mission as one among three competing mission candidates within the European Space Agency (ESA) Earth Explorer 10 Programme. However, this paper intends to cover the LTI parameters such that it can be used as a background scientific reference for any mission targeting in situ observations of the LTI..
U2 - 10.5194/angeo-39-189-2021
DO - 10.5194/angeo-39-189-2021
M3 - Journal article
AN - SCOPUS:85101604463
SN - 0992-7689
VL - 39
SP - 189
EP - 237
JO - Annales Geophysicae
JF - Annales Geophysicae
IS - 1
ER -