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pith:R3HOGO5V

pith:2026:R3HOGO5VN34IM5VPDBUI6XIWSR
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Global evolution of electric fields during planet encircling dust storms on Mars

Amanda S. Brecht, Ina Taxis, Leonardos Gkouvelis, Melinda A. Kahre, Richard A. Urata

Global dust storms on Mars generate near-surface electric fields of 100-1000 volts per meter concentrated in southern low-to-mid latitudes.

arxiv:2605.13781 v1 · 2026-05-13 · astro-ph.EP

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4 Citations open
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Claims

C1strongest claim

The simulations reveal broad storm-active belts of enhanced electrification, with the most frequent threshold exceedances occurring in southern low-to-mid latitudes and secondary activity in northern low-to-mid latitudes. Modeled near-surface electric fields reach 10^{2}--10^{3} V m^{-1} comparable to values inferred for smaller-scale dust phenomena.

C2weakest assumption

The triboelectric charging and electrostatic diagnostic scheme accurately links collisional charging to the local dynamical state of the atmosphere, and that unresolved small-scale turbulent structures do not invalidate the large-scale electrification patterns predicted.

C3one line summary

Simulations of global dust storms on Mars show near-surface electric fields reaching 100-1000 V/m, strongest in southern low-to-mid latitudes, mostly in weak discharge regimes due to conductivity changes.

References

41 extracted · 41 resolved · 0 Pith anchors

[1] Abdelaal, M. E., Dokuchaev, I. V ., Kuznetsov, I. A., et al. 2025, Solar System Research, 59, 71 2025
[2] Adzhieva, A. A., Shapovalov, V . A., Mashukov, I. K., & Tumgoeva, H. A. 2020, in Journal of Physics Conference Series, V ol. 1604, Journal of Physics Con- ference Series, 012016 2020
[3] 2022, Journal of Geophysical Re- search (Planets), 127, e07206 2022
[4] Barth, E. L., Farrell, W. M., & Rafkin, S. C. R. 2016, Icarus, 268, 253 2016
[5] Bertrand, T., Wilson, R. J., Kahre, M. A., Urata, R., & Kling, A. 2020, Journal of Geophysical Research (Planets), 125, e06122 2020
Receipt and verification
First computed 2026-05-18T02:44:15.732742Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

8ecee33bb56ef88676af18688f5d169449d837101b2aecd1026aa66d34f9d533

Aliases

arxiv: 2605.13781 · arxiv_version: 2605.13781v1 · doi: 10.48550/arxiv.2605.13781 · pith_short_12: R3HOGO5VN34I · pith_short_16: R3HOGO5VN34IM5VP · pith_short_8: R3HOGO5V
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/R3HOGO5VN34IM5VPDBUI6XIWSR \
  | 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: 8ecee33bb56ef88676af18688f5d169449d837101b2aecd1026aa66d34f9d533
Canonical record JSON
{
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    "abstract_canon_sha256": "442298b3c059ac5668c9b4a4c3d95f630ef1202f8accfd77e113878837939dd2",
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    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.EP",
    "submitted_at": "2026-05-13T17:02:35Z",
    "title_canon_sha256": "624153c622458a747c6ec71f4c8b74081e4d3e0329b4afdb50bb18075fdf4127"
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