Evidence map›Paper›PMID 38585189›Full record

ReviewSpace science reviews2024

Possible Effects of Volcanic Eruptions on the Modern Atmosphere of Venus.

Colin F Wilson, Emmanuel Marcq, Cédric Gillmann, Thomas Widemann, Oleg Korablev, Nils T Mueller, Maxence Lefèvre, Paul B Rimmer, Séverine Robert, Mikhail Y Zolotov

Open access · hybridAbstract readReview
In one paragraph

Review in Space science reviews, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing papers in PubMed
3.0field-weighted citation impact, top 10% of its field
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

1 citing paper in PubMed, 10 citations in OpenAlex.

  1. Venus reawakening.Nature communications · 2026
    Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

10 authors at 8 institutions in 8 countries.

Colin F WilsonEuropean Space Agency, Keplerlaan 1, 2201, AZ Noordwijk, The Netherlands.ORCID 0000-0001-5355-1533
Emmanuel MarcqLATMOS/IPSL, UVSQ Sorbonne Université Paris-Saclay, Sorbonne Université, CNRS, Guyancourt, France.
Cédric GillmannInstitut für Geophysik, Geophysical Fluid Dynamics, ETH Zurich, Sonneggstraße 5, 8092 Zürich, Switzerland.
Thomas WidemannLESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Cité, 5 place Jules Janssen, 92195 Meudon, France.
Oleg KorablevSpace Research Institute (IKI), Russian Academy of Sciences, Moscow, 117997 Russia.
Nils T MuellerInstitute for Planetary Research, DLR, Rutherfordstraße 2, 12489 Berlin, Germany.ORCID 0000-0001-9229-8921
Maxence LefèvreLATMOS/IPSL, UVSQ Sorbonne Université Paris-Saclay, Sorbonne Université, CNRS, Guyancourt, France.
Paul B RimmerCavendish Laboratory, University of Cambridge, JJ Thomson Avenue, Cambridge, CB3 0HE UK.
Séverine RobertRoyal Belgian Institute for Space Aeronomy, Brussels, Belgium.
Mikhail Y ZolotovSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287-1404 USA.
Centre National de la Recherche Scientifique · FRArizona State University · USNOAA Geophysical Fluid Dynamics Laboratory · USPlanetary Science Institute · USRoyal Belgian Institute for Space Aeronomy · BESpace Research Institute · RUUniversity of Cambridge · GBUniversity of Oxford · GB

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

This work reviews possible signatures and potential detectability of present-day volcanically emitted material in the atmosphere of Venus. We first discuss the expected composition of volcanic gases at present time, addressing how this is related to mantle composition and atmospheric pressure. Sulfur dioxide, often used as a marker of volcanic activity in Earth's atmosphere, has been observed since late 1970s to exhibit variability at the Venus' cloud tops at time scales from hours to decades; however, this variability may be associated with solely atmospheric processes. Water vapor is identified as a particularly valuable tracer for volcanic plumes because it can be mapped from orbit at three different tropospheric altitude ranges, and because of its apparent low background variability. We note that volcanic gas plumes could be either enhanced or depleted in water vapor compared to the background atmosphere, depending on magmatic volatile composition. Non-gaseous components of volcanic plumes, such as ash grains and/or cloud aerosol particles, are another investigation target of orbital and

Indexed as

Detecting volcanismPlanetary volcanismVenusVenus evolutionVenus explorationVolcanic plumes

Identifiers

PMID38585189
PMCPMC10997549
OpenAlexW4393981017

What OpenQuestion holds

Textmetadata
LicenceCC BY
Read underepoch 390

Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.