Cited by 304Planetary Science and ExplorationAstro and Planetary ScienceGeology and Paleoclimatology Research

Amazonian northern mid-latitude glaciation on Mars: A proposed climate scenario

Open access
Madeleine, J.-B., Forget, F., Head, James W., Levrard, B., Montmessin, F., Millour, E.·2009·Icarus

Integrity signals

Registry

Crossref · 10.1016/j.icarus.2009.04.037

Cites

1 of 1 references verified0 citation errors · 0 not checkable

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Claims the paper makes

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Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • At high obliquities, ice migration to equatorial and mid-latitude regions is predicted.

    “Mars' obliquity has varied significantly throughout the Amazonian, however (Laskar & Robutel 1993), and at high obliquities ice migration to equatorial (Mischna et al. 2003; Forget et al. 2006) and mid-latitude (Madeleine et al. 2009) regions is predicted.”

    From The Climate of Early Mars (2016) · cites this paper as Madeleine et al. 2009

Cites

  • The chaotic obliquity of the planets

    Laskar, J., & Robutel, P. (1993) · Nature · doi:10.1038/361608a0 · Cited by 499 · cited 1× · see citing works

    “Spin-axis and orbital parameter variations of Mars are much larger than on Earth, and their evolution can only be calculated over a few millions of years (Laskar and Robutel, 1993) due to the strongly chaotic nature of the solutions prior to this time.”
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  • The Climate of Early Mars

    Wordsworth, R. D. (2016) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev-earth-060115-012355 · Cited by 416 · see citing works

    “Mars’ obliquity has varied significantly throughout the Amazonian, however (Laskar & Robutel 1993), and at high obliquities ice migration to equatorial (Mischna et al. 2003; Forget et al. 2006) and mid-latitude (Madeleine et al. 2009) regions is predicted.”
    Background

Authors
Madeleine, J.-B., Forget, F., Head, J. W., Levrard, B., Montmessin, F., & Millour, E.
Affiliations
Centre National de la Recherche Scientifique (FR)
Corresponding author
Madeleine, J.-B.
Venue
Icarus
Publisher
Elsevier BV
Published
2009-10
Volume
203
Issue
2
Pages
390-405
ISSN
0019-1035 (ISSN-L)
OpenAlex
W2120077698
Cited by
304
References
1
Citations by year
2026: 13 · 2025: 18 · 2024: 18 · 2023: 11 · 2022: 13 · 2021: 15 · 2020: 9 · 2019: 14 · 2018: 29 · 2017: 19 · 2016: 20 · 2015: 28 · 2014: 29 · 2013: 17 · 2012: 17
FWCI
8.23
Type
journal article
Language
en
Open access
Locations
  • Icarus (publishedVersion)
  • HAL (submittedVersion, other-oa)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Geology and Paleoclimatology Research
Keywords
Mars climate, Amazonian period, Mars general circulation model, obliquity, dust opacity, water ice sublimation, ice accumulation, stationary planetary waves, topographic forcing, Tharsis volcanoes, glacial deposits, ice sheets, atmospheric water vapor

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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

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