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Insensitive Nuclei Enhanced by Polarization Transfer (INEPT) is an advanced Nuclear Magnetic Resonance (NMR) technique specifically designed to detect and enhance the signals of low-abundance nuclei, such as carbon-13 and nitrogen-15, in small molecules. The fundamental principle behind INEPT is the transfer of polarization from a more abundant and highly polarizable nucleus, typically hydrogen-1, to the low-abundance nucleus of interest. This process effectively boosts the NMR signal of the...
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Related Experiment Video

Updated: Mar 11, 2026

Direct Imaging of Laser-driven Ultrafast Molecular Rotation
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The Low-Energy Neutral Imager (LENI).

J H Westlake1, D G Mitchell1, P C-Son Brandt1

  • 1Applied Physics Laboratory The Johns Hopkins University Laurel Maryland USA.

Journal of Geophysical Research. Space Physics
|November 22, 2016
PubMed
Summary
This summary is machine-generated.

A new energetic neutral atom (ENA) imager concept offers high angular resolution for studying the heliospheric boundary and magnetospheric ENA emissions. This advanced instrument utilizes novel technology for improved spatial and temporal understanding of space plasma.

Keywords:
ENAenergetic particlesheliospheric imaginginstrumentmagnetospheric imagingmeasurement techniques

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Area of Science:

  • Space physics
  • Plasma physics
  • Instrument development

Background:

  • Breakthroughs in heliospheric and magnetospheric energetic neutral atom (ENA) imaging necessitate novel instrument designs.
  • Existing instruments have provided initial insights into the heliospheric boundary and magnetospheric ENA emissions.
  • Understanding suprathermal plasma populations is crucial for characterizing these regions.

Purpose of the Study:

  • To present a concept for a high angular resolution ENA imager.
  • To enable detailed study of the heliospheric boundary's spatial and temporal structure.
  • To characterize magnetospheric ENA emissions from various regions, including the ring current and magnetosheath.

Main Methods:

  • The proposed instrument targets suprathermal plasma populations with energies from 0.5 to 20 keV.
  • It employs ultrathin carbon foils for ENA detection.
  • Utilizes 2-D collimation and a novel electron optical design for enhanced imaging capabilities.

Main Results:

  • The concept achieves high angular resolution (≤2°).
  • It offers high sensitivity (≥10⁻³ cm² sr/pixel).
  • The design is suitable for imaging ENA emissions in the 0.5-20 keV energy range.

Conclusions:

  • This new ENA imager concept represents a significant advancement for heliospheric and magnetospheric research.
  • It will enhance our understanding of dynamic space plasma environments.
  • The instrument is well-suited for future space missions requiring detailed ENA imaging.