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pith:E4X5Q2HZ

pith:2026:E4X5Q2HZW4CBXDRRHALJRGJ5RC
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Role of Magnetic Field in the Redistribution of Turbulence from Large-Scale Structures to Small-Scale Fluctuations

Abhijit Sen, Bhoomi Khodiyar, Lavkesh Lachhvani, Prabal K. Chattopadhyay, Raju Daniel, Rosh Roy, Sayak Bose, Tanmay Karmakar

Increasing the magnetic field from 600 to 1000 G suppresses zonal flows while shifting turbulence power from low to high frequencies through reduced Reynolds stress.

arxiv:2605.17321 v1 · 2026-05-17 · physics.plasm-ph

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Claims

C1strongest claim

As the magnetic field is increased from 600 to 1000 G, zonal flow is suppressed while the mean flow increases, with spectral analysis showing redistribution of power from low-frequency (0.1-1 kHz) to high-frequency (1-300 kHz) components linked to reduction in Reynolds stress due to loss of correlation between radial and poloidal velocity fluctuations.

C2weakest assumption

The inference that the observed loss of correlation between radial and poloidal velocity fluctuations directly causes the reduction in Reynolds stress and thereby suppresses zonal flow generation; this causal link is stated as 'possibly' in the abstract and rests on the assumption that no other unmeasured factors dominate the change when B is increased.

C3one line summary

Increasing magnetic field strength suppresses zonal flows and redistributes turbulence power from low to high frequencies through reduced Reynolds stress in a linear plasma device.

References

36 extracted · 36 resolved · 0 Pith anchors

[1] Drift waves and transport, 1999
[2] Drift waves in a high-density cylindrical helicon discharge, 2005
[3] Collisional drift instability in a variable radial electric field, 1986
[4] On the transition to drift turbulence in a magnetized plasma column, 2005
[5] Observation of turbulent- driven shear flow in a cylindrical laboratory plasma de- vice, 2006

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-20T00:03:52.033680Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

272fd868f9b7041b8e31381698993d88ac1af0f6e5499bcb602a17adf88be457

Aliases

arxiv: 2605.17321 · arxiv_version: 2605.17321v1 · doi: 10.48550/arxiv.2605.17321 · pith_short_12: E4X5Q2HZW4CB · pith_short_16: E4X5Q2HZW4CBXDRR · pith_short_8: E4X5Q2HZ
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/E4X5Q2HZW4CBXDRRHALJRGJ5RC \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 272fd868f9b7041b8e31381698993d88ac1af0f6e5499bcb602a17adf88be457
Canonical record JSON
{
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    "abstract_canon_sha256": "425d4a8dfc7a1578dd7cba6eeb482ecf84eca301b5d5994f6d30fff1705b65fa",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by-nc-sa/4.0/",
    "primary_cat": "physics.plasm-ph",
    "submitted_at": "2026-05-17T08:29:10Z",
    "title_canon_sha256": "405ff1a732abfe75090f804170bec01b94da56ebd7156b863438f8c1c3048c73"
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  "source": {
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    "kind": "arxiv",
    "version": 1
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}