On the nightglow polarisation for space weather exploration

We present here observations of the polarisation of four auroral lines in the auroral oval and in the polar cusp using a new ground polarimeter called Petit Cru. Our results confirm the already known polarisation of the red line, and show for the first time that the three other lines observed here (...

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Bibliographic Details
Published in:Journal of Space Weather and Space Climate
Main Authors: Bosse Léo, Lilensten Jean, Gillet Nicolas, Rochat Sylvain, Delboulbé Alain, Curaba Stephane, Roux Alain, Magnard Yves, Johnsen Magnar G., Løvhaug Unni-Pia, Amblard Pierre-Olivier, Le Bihan Nicolas, Nabon Maxime, Marif Hanane, Auriol Frédérique, Noûs Camille
Format: Article in Journal/Newspaper
Language:English
Published: EDP Sciences 2020
Subjects:
polarisation
aurora
Meteorology. Climatology
QC851-999
New Ground
EISCAT
Online Access:https://doi.org/10.1051/swsc/2020036
https://doaj.org/article/633c5e6b3a4b450db9d5684a3c50fb71
Description
Summary:We present here observations of the polarisation of four auroral lines in the auroral oval and in the polar cusp using a new ground polarimeter called Petit Cru. Our results confirm the already known polarisation of the red line, and show for the first time that the three other lines observed here (namely 557.7 nm, 391.4 nm and 427.8 nm) are polarised as well up to a few percent. We show that in several circumstances, this polarisation is linked to the local magnetic activity and to the state of the ionosphere through the electron density measured with EISCAT. However, we also show that the contribution of light pollution from nearby cities via scattering can not be ignored and can play an important role in polarisation measurements. This series of observations questions the geophysical origin of the polarisation. It also leaves open its relation to the magnetic field orientation and to the state of both the upper atmosphere and the troposphere.

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