Evidence map›Paper›PMID 36874191›Full record

ReviewSpace science reviews2023

Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe.

P C Brandt, E Provornikova, S D Bale, A Cocoros, R DeMajistre, K Dialynas, H A Elliott, S Eriksson, B Fields, A Galli and 33 more

Open access · hybridAbstract readReview
PubMed Full text at PMC Publisher
In one paragraph

Review in Space science reviews, 2023. 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
4.1field-weighted citation impact, top 6% 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, 24 citations in OpenAlex.

  1. 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

43 authors at 19 institutions in 6 countries.

P C BrandtThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.ORCID 0000-0002-4644-0306
E ProvornikovaThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
S D BaleUniversity of California Berkeley, Berkeley, CA USA.
A CocorosThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
R DeMajistreThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
K DialynasOffice of Space Research and Technology, Academy of Athens, Athens, 10679 Greece.
H A ElliottSouthwest Research Institute, San Antonio, TX USA.
S ErikssonLaboratory for Atmospheric and Space Physics, University of Colorado at Boulder, Boulder, CO USA.
B FieldsUniversity of Illinois Urbana-Champaign, Urbana, IL USA.
A GalliUniversity of Bern, Bern, Switzerland.
M E HillThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
M HoranyiLaboratory for Atmospheric and Space Physics, University of Colorado at Boulder, Boulder, CO USA.
T HorburyImperial College London, London, UK.
S HunzikerETH, Zurich, Switzerland.
P KollmannThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
J KinnisonThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
G FountainThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
S M KrimigisOffice of Space Research and Technology, Academy of Athens, Athens, 10679 Greece.
W S KurthUniversity of Iowa, Iowa City, IA USA.
J LinskyUniversity of Colorado Boulder, Boulder, CO USA.
C M LisseThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
K E MandtThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
W MagnesSpace Research Institute, Austrian Academy of Sciences, Graz, Austria.
R L McNuttThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
J MillerBoston University, Boston, MA USA.
E MoebiusUniversity of New Hampshire, Durham, NH USA.
P MostafaviThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
M OpherBoston University, Boston, MA USA.
L PaxtonThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
F PlaschkeTechnical University Braunschweig, Braunschweig, Germany.
A R PoppeUniversity of California Berkeley, Berkeley, CA USA.
E C RoelofThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
K RunyonPlanetary Science Institute, Tucson, AZ USA.
S RedfieldWeslayan University, Middeltown, CT USA.
N SchwadronUniversity of New Hampshire, Durham, NH USA.
V SterkenETH, Zurich, Switzerland.
P SwaczynaPrinceton University, Princeton, NJ USA.
J SzalayPrinceton University, Princeton, NJ USA.
D TurnerThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
H VannierWeslayan University, Middeltown, CT USA.
R Wimmer-SchweingruberUniversity of Kiel, Kiel, Germany.
P WurzUniversity of Bern, Bern, Switzerland.
E J ZirnsteinPrinceton University, Princeton, NJ USA.
Johns Hopkins University Applied Physics Laboratory · USPrinceton University · USAcademy of Athens · GRBoston University · USETH Zurich · CHLaboratory for Atmospheric and Space Physics · USUniversity of Bern · CHUniversity of California, Berkeley · USUniversity of New Hampshire · USWesleyan University · USAustrian Academy of Sciences · ATChristian-Albrechts-Universität zu Kiel · DEImperial College London · GBPlanetary Science Institute · USSouthwest Research Institute · USTechnische Universität Braunschweig · DEUniversity of Colorado Boulder · USUniversity of Illinois Urbana-Champaign · USUniversity of Iowa · US

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

A detailed overview of the knowledge gaps in our understanding of the heliospheric interaction with the largely unexplored Very Local Interstellar Medium (VLISM) are provided along with predictions of with the scientific discoveries that await. The new measurements required to make progress in this expanding frontier of space physics are discussed and include in-situ plasma and pick-up ion measurements throughout the heliosheath, direct sampling of the VLISM properties such as elemental and isotopic composition, densities, flows, and temperatures of neutral gas, dust and plasma, and remote energetic neutral atom (ENA) and Lyman-alpha (LYA) imaging from vantage points that can uniquely discern the heliospheric shape and bring new information on the interaction with interstellar hydrogen. The implementation of a pragmatic Interstellar Probe mission with a nominal design life to reach 375 Astronomical Units (au) with likely operation out to 550 au are reported as a result of a 4-year NASA funded mission study.

Indexed as

Interstellar mediumInterstellar probeOuter heliosphere

Identifiers

PMID36874191
PMCPMC9974711
OpenAlexW4322775599

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.