Articles | Volume 37, issue 6
https://doi.org/10.5194/angeo-37-1121-2019
https://doi.org/10.5194/angeo-37-1121-2019
Review paper
 | 
10 Dec 2019
Review paper |  | 10 Dec 2019

Dust observations with antenna measurements and its prospects for observations with Parker Solar Probe and Solar Orbiter

Ingrid Mann, Libor Nouzák, Jakub Vaverka, Tarjei Antonsen, Åshild Fredriksen, Karine Issautier, David Malaspina, Nicole Meyer-Vernet, Jiří Pavlů, Zoltan Sternovsky, Joan Stude, Shengyi Ye, and Arnaud Zaslavsky

Viewed

Total article views: 4,486 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
3,511 936 39 4,486 64 44
  • HTML: 3,511
  • PDF: 936
  • XML: 39
  • Total: 4,486
  • BibTeX: 64
  • EndNote: 44
Views and downloads (calculated since 15 Jul 2019)
Cumulative views and downloads (calculated since 15 Jul 2019)

Viewed (geographical distribution)

Total article views: 4,486 (including HTML, PDF, and XML) Thereof 4,215 with geography defined and 271 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 28 Mar 2024
Download
Short summary
This work presents a review of dust measurements from spacecraft Cassini, STEREO, MMS, Cluster, Maven and WIND. We also consider the details of dust impacts and charge generation, and how different antenna signals can be generated. We compare observational data to laboratory experiments and simulations and discuss the consequences for dust observation with the new NASA Parker Solar Probe and ESA Solar Orbiter spacecraft.