Preprints
https://doi.org/10.5194/angeo-2019-136
https://doi.org/10.5194/angeo-2019-136
18 Sep 2019
 | 18 Sep 2019
Status: this discussion paper is a preprint. It has been under review for the journal Annales Geophysicae (ANGEO). The manuscript was not accepted for further review after discussion.

Ionospheric Plasma Density Measurements by Swarm Langmuir Probes: Limitations and possible Corrections

Piero Diego, Igino Coco, Igor Bertello, Maurizio Candidi, and Pietro Ubertini

Abstract. The ESA Swarm constellation includes three satellites, which have been observing the Earth's ionosphere since November 2013, following polar orbits. The main ionospheric plasma parameters, such as electron density and temperature, are measured by means of Langmuir probes (Lps); electron density measurements, in particular, are nowadays largely considered as qualitatively reliable, and have been used in several published papers to date. In this work, we aim to discuss how some technical characteristics of Swarm Lps, such as their size and location on board the satellites, as well as the operational setup of the instruments, could lead to limitations in their accuracy if one underestimates the influence of satellite proximity, and the larger extension of the plasma sheath surrounding the probes due to the operational point of the voltage ripple. Two specific corrections are proposed for the assessment and possible mitigation of such effects. Finally, a comparison is made with electron density measurements from CSES-01 mission, which relies on Langmuir probes as well, whose geometry and operating mode are standard.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this preprint. The responsibility to include appropriate place names lies with the authors.
Piero Diego, Igino Coco, Igor Bertello, Maurizio Candidi, and Pietro Ubertini
 
Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement
 
Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement
Piero Diego, Igino Coco, Igor Bertello, Maurizio Candidi, and Pietro Ubertini
Piero Diego, Igino Coco, Igor Bertello, Maurizio Candidi, and Pietro Ubertini

Viewed

Total article views: 1,477 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
837 560 80 1,477 91 90
  • HTML: 837
  • PDF: 560
  • XML: 80
  • Total: 1,477
  • BibTeX: 91
  • EndNote: 90
Views and downloads (calculated since 18 Sep 2019)
Cumulative views and downloads (calculated since 18 Sep 2019)

Viewed (geographical distribution)

Total article views: 1,324 (including HTML, PDF, and XML) Thereof 1,319 with geography defined and 5 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 20 Nov 2024
Download
Short summary
In-situ measurements validation is always a delicate matter of study until data are collected by a single mission. In case of different missions operating almost in the same environment (i.e. latitude, altitude, local time) it is of fundamental importance the detection of instrumental setting and algorithms to provide the best accordance among measurements. The present work aims to validate both Swarm and CSES plasma density measures for the improvements of the ionospheric models development.