Evidence map›Paper›PMID 41416174›Full record

ReviewSpace science reviews2026

The Compact Dual Ion Composition Experiment (CoDICE) for the IMAP Mission.

S A Livi, M I Desai, K Ogasawara, L Kistler, E Möbius, M J Starkey, M A Dayeh, D Kataria, H A Elliott, S Hart and 39 more

Abstract readReview
PubMed Full text at PMC Publisher
In one paragraph

Review in Space science reviews, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing 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

5 citing papers in PubMed.

  1. Review
  2. The IMAP Observatory Overview.Space science reviews · 2026
    Review
  3. Review
  4. Review
  5. Review
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

49 authors.

S A LiviSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M I DesaiSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.ORCID 0000-0002-7318-6008
K OgasawaraSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
L KistlerPhysics & Astronomy, University of New Hampshire, Durham, USA.
E MöbiusPhysics & Astronomy, University of New Hampshire, Durham, USA.
M J StarkeySpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M A DayehSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
D KatariaSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
H A ElliottSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
S HartSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
B AltermanHeliophysics Division, NASA Goddard Space Flight Center, Greenbelt, USA.
D J McComasDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
C J PollockHeliophysics Division, NASA Goddard Space Flight Center, Greenbelt, USA.
J MukherjeeSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
J TrevinoSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
S FerrellSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
T BrennerSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
S E PopeSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M TapleySpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
K PavlasSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
J S RankinDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
M M ShenDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
L KhooDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
M AlimaganbetovDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
J TeifertDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
E M RoemerDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
M Shaw-LecerfDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
J EscobarDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
E R ChristianHeliophysics Division, NASA Goddard Space Flight Center, Greenbelt, USA.
N A SchwadronPhysics & Astronomy, University of New Hampshire, Durham, USA.
M GkioulidouSpace Exploration Sector, Johns Hopkins University Applied Physics Laboratory, Laurel, USA.
G GrubbsSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M BryschSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M EpperlySpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
D GeorgeSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
G DunnSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
J FordSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
C L SchwendemanSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M CommonsL-3 Communications, Vertex Aerospace, Universal City, USA.
S PersynSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
S JaskulekSpace Exploration Sector, Johns Hopkins University Applied Physics Laboratory, Laurel, USA.
S WeidnerDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ USA.
C BertSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
M FerrisSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
B RodriguezSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
C NunezSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
C UrdialesSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
S CortinasSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.
H RodriguezSpace Science & Engineering, Southwest Research Institute, San Antonio, USA.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Stationed in an orbit about the first Sun-Earth Lagrange point, L1, NASA's Interstellar Mapping and Acceleration Probe (IMAP) mission is designed to provide well-coordinated measurements of the in-situ solar wind (SW) plasma and interplanetary magnetic field, interstellar pickup ions (PUIs), suprathermal and energetic ions, interstellar and energetic neutral atoms (ENAs), interstellar dust, and 3-dimensional (3D) maps of the global solar wind structure. Together these measurements from ten instruments address two key Heliophysics objectives, namely, 1) the acceleration of charged particles and 2) the interaction of the solar wind with the local interstellar medium. This paper describes one of the five in-situ instruments - the Compact Dual Ion Composition Experiment (CoDICE) that provides comprehensive measurements of the source populations and the charged particles that are accelerated near the Sun and throughout the heliosphere and beyond. CoDICE also provides the 3D velocity distribution functions (3D VDFs) of interstellar PU He

Indexed as

Energetic particlesHeliosphereIMAPParticle accelerationPickup ionsSolar wind plasmaSpace weatherSunSuprathermal ions

Identifiers

PMID41416174
PMCPMC12708712

What OpenQuestion holds

Textmetadata
LicenceCC BY-NC-ND
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.