Charge and current neutralization of an ion-beam pulse propagating in a background plasma along a solenoidal magnetic field.
← Research streamAnalytical theory predicts that applying a small solenoidal magnetic field can drastically change the self-electric and self-magnetic fields of an ion-beam pulse propagating in background plasma. When the electron gyrofrequency approximately equals the electr…
Study snapshot
Abstract
The analytical studies show that the application of a small solenoidal magnetic field can drastically change the self-magnetic and self-electric fields of the beam pulse propagating in a background plasma. Theory predicts that when omega_{ce} approximately omega_{pe}beta_{b}, where omega_{ce} is the electron gyrofrequency, omega_{pe} is the electron plasma frequency, and beta_{b} is the ion-beam velocity relative to the speed of light, there is a sizable enhancement of the self-electric and self-magnetic fields due to the dynamo effect. Furthermore, the combined ion-beam-plasma system acts as a paramagnetic medium; i.e., the solenoidal magnetic field inside the beam pulse is enhanced.
AI evidence extraction
Structured fields below were generated from the paper’s abstract and metadata to make the evidence easier to inspect. Automated extraction may be incomplete or incorrect; verify important details against the original paper.
Main findings
Analytical theory predicts that applying a small solenoidal magnetic field can drastically change the self-electric and self-magnetic fields of an ion-beam pulse propagating in background plasma. When the electron gyrofrequency approximately equals the electron plasma frequency times the ion-beam beta (ωce ≈ ωpe βb), the self-fields are predicted to be sizably enhanced due to a dynamo effect, and the solenoidal magnetic field inside the beam pulse is enhanced (paramagnetic response).
Outcomes measured
- Self-electric field of an ion-beam pulse in background plasma
- Self-magnetic field of an ion-beam pulse in background plasma
- Solenoidal magnetic field enhancement inside the beam pulse (paramagnetic behavior)
Limitations
- Findings are described as analytical/theoretical predictions; no experimental or epidemiological data are mentioned in the abstract.
- No quantitative field strengths, frequencies, or exposure metrics are provided in the abstract.
View raw extracted JSON
{
"study_type": "other",
"exposure": {
"band": null,
"source": null,
"frequency_mhz": null,
"sar_wkg": null,
"duration": null
},
"population": null,
"sample_size": null,
"outcomes": [
"Self-electric field of an ion-beam pulse in background plasma",
"Self-magnetic field of an ion-beam pulse in background plasma",
"Solenoidal magnetic field enhancement inside the beam pulse (paramagnetic behavior)"
],
"main_findings": "Analytical theory predicts that applying a small solenoidal magnetic field can drastically change the self-electric and self-magnetic fields of an ion-beam pulse propagating in background plasma. When the electron gyrofrequency approximately equals the electron plasma frequency times the ion-beam beta (ωce ≈ ωpe βb), the self-fields are predicted to be sizably enhanced due to a dynamo effect, and the solenoidal magnetic field inside the beam pulse is enhanced (paramagnetic response).",
"effect_direction": "unclear",
"limitations": [
"Findings are described as analytical/theoretical predictions; no experimental or epidemiological data are mentioned in the abstract.",
"No quantitative field strengths, frequencies, or exposure metrics are provided in the abstract."
],
"evidence_strength": "insufficient",
"confidence": 0.74,
"peer_reviewed_likely": "yes",
"keywords": [
"ion-beam pulse",
"background plasma",
"solenoidal magnetic field",
"electron gyrofrequency",
"electron plasma frequency",
"dynamo effect",
"paramagnetic medium",
"self-electric field",
"self-magnetic field"
],
"suggested_hubs": []
}AI-extracted fields are generated from the abstract and metadata and may be incomplete or incorrect. This material is for informational purposes and is not medical advice.
Identifiers and source
DOI: 10.1103/physrevlett.99.235002
PubMed: 18233377