Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

PROSERPINA: An Automated Pipeline for Martian Ionospheric Radio-occultation Retrievals with Probabilistic Uncertainty and Spherical-symmetry Bias Quantification

  • Authors: Marianna Felici, Yu-Ming (Oscar) Yang, Luke Moore, Jennifer Segale, Joshua Semeter, Prakash Ishwar, Paul Withers, Kamal Oudrhiri

Marianna Felici et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Frequency residual Δf as a function of data point number (acquisition order; 0 is the start of the record, in free space) for occultation MGS20081539X54, with tangent-point altitude on the upper axis. Grey: the full residual (945 points). Red: the samples used in the first-iteration (Iteration a) baseline fit (n = 270). Dark blue: the fitted baseline, with its 95% credible interval shaded.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse