Evidence map›Paper›PMID 36245894›Full record

ArticleGeophysical research letters2022

Hexagonal Prisms Form in Water-Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover.

M T Lemmon, D Toledo, V Apestigue, I Arruego, M J Wolff, P Patel, S Guzewich, A Colaprete, Á Vicente-Retortillo, L Tamppari and 6 more

Abstract read
In one paragraph

Article in Geophysical research letters, 2022. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
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

2 citing papers in PubMed.

  1. Article
  2. 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

16 authors.

M T LemmonSpace Science Institute Boulder CO USA.ORCID https://orcid.org/0000-0002-4504-5136
D ToledoInstituto Nacional de Técnica Aerospacial Madrid Spain.ORCID https://orcid.org/0000-0002-0103-1891
V ApestigueInstituto Nacional de Técnica Aerospacial Madrid Spain.ORCID https://orcid.org/0000-0002-4349-8019
I ArruegoInstituto Nacional de Técnica Aerospacial Madrid Spain.ORCID https://orcid.org/0000-0001-9705-9743
M J WolffSpace Science Institute Boulder CO USA.ORCID https://orcid.org/0000-0002-1127-8329
P PatelJet Propulsion Laboratory California Institute of Technology Pasadena CA USA.ORCID https://orcid.org/0000-0001-7407-3251
S GuzewichNASA Goddard Space Flight Center Greenbelt MD USA.ORCID https://orcid.org/0000-0003-1149-7385
A ColapreteNASA Ames Research Center Moffett Field CA USA.
Á Vicente-RetortilloCentro de Astrobiología (INTA-CSIC) Madrid Spain.ORCID https://orcid.org/0000-0002-4553-7624
L TamppariJet Propulsion Laboratory California Institute of Technology Pasadena CA USA.ORCID https://orcid.org/0000-0001-5124-6375
F MontmessinLATMOS Paris France.ORCID https://orcid.org/0000-0002-4187-1457
M de la Torre JuarezJet Propulsion Laboratory California Institute of Technology Pasadena CA USA.ORCID https://orcid.org/0000-0003-1393-5297
J MakiJet Propulsion Laboratory California Institute of Technology Pasadena CA USA.ORCID https://orcid.org/0000-0002-7887-0343
T McConnochieSpace Science Institute Boulder CO USA.
A BrownPlancius Research Severna Park MD USA.ORCID https://orcid.org/0000-0002-9352-6989
J F BellArizona State University Tempe AZ USA.ORCID https://orcid.org/0000-0002-2006-4074

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Observations by several cameras on the Perseverance rover showed a 22° scattering halo around the Sun over several hours during northern midsummer (solar longitude 142°). Such a halo has not previously been seen beyond Earth. The halo occurred during the aphelion cloud belt season and the cloudiest time yet observed from the Perseverance site. The halo required crystalline water-ice cloud particles in the form of hexagonal columns large enough for refraction to be significant, at least 11 μm in diameter and length. From a possible 40-50 km altitude, and over the 3.3 hr duration of the halo, particles could have fallen 3-12 km, causing downward transport of water and dust. Halo-forming clouds are likely rare due to the high supersaturation of water that is required but may be more common in northern subtropical regions during northern midsummer.

Identifiers

PMID36245894
PMCPMC9539710

What OpenQuestion holds

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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.