Energy Aperture

Value chain · CLM-0440

Low confidence

The evidence behind this statement is thin, indirect or second-hand. Read it as a lead to check, not as a settled finding.

In plain terms

A 2026 computer model of a gigawatt-class space solar power beam finds it would barely disturb the density of the upper atmosphere's electrically charged layer, but would locally heat one part of it (the F-region) by several thousand degrees.

The claim as recorded

Guo et al. (2026) model, for a 1 GW SPS beam, a maximum ponderomotive electron-density depletion of 0.00565% at 2.45 GHz and 0.01525% at 5.8 GHz, both stated as "far below self-focusing and cavitation thresholds," alongside a peak electron-temperature perturbation of 3815 K (2.45 GHz) and 3585 K (5.8 GHz) concentrated in the F-region.

Scope and limits

A MODELLED result from a 2026 arXiv preprint whose peer-review status is not established; applies only to the specific 1 GW, 2.45/5.8 GHz, mid-latitude, vertical-incidence, quiet-ionosphere case modelled. The paper flags oblique incidence, geomagnetic anisotropy, and disturbed/storm-time ionospheres as future work not yet done. A POSSIBLE SOURCE-SIDE DEFECT AGAINST THE 3585 K FIGURE, raised by VER-1094 and NOT resolved. SRC-105 states at printed p.9 that its neural surrogate is trained on |E| from 1e-2 to 500 V/m and at printed p.10 that inputs are "clipped to the training ranges", yet its Figure 13(a) at printed p.21 shows the 5.8 GHz peak field at roughly 532 to 614 V/m along the ENTIRE path - above the stated ceiling everywhere - while the 2.45 GHz case sits at about 234 to 248 V/m and is inside range. If the clipping was applied as described, the 5.8 GHz maximum dTe and maximum Qh are biased LOW, and the paper's limitations paragraph does not mention it. Not asserted as an error: Table 1 shows separate surrogates per frequency, so the range may have been widened without being restated. What is established is an unreconciled discrepancy between the stated method and the plotted result, and it bears on any figure this claim takes from that column.

What it assumes

The IRI/NRLMSISE-00 background ionosphere and neural-network collision-frequency closure used in the model are representative; the paper does not state its solar-activity input precisely.

Where it comes from

SRC-105 Full-Path Nonlinear Modeling of Microwave Power Transmission Through Ionospheric Plasma for...
SRC-105 Full-Path Nonlinear Modeling of Microwave Power Transmission Through Ionospheric Plasma for...
Guo et al. (2026), Table 3 and Conclusion, p.21-22: ponderomotive density depletion 0.00565% (2.45GHz) / 0.01525% (5.8GHz), "far below self-focusing and cavitation thresholds... consistent with the threshold analyses of Thome, Perkins, and Shinohara et al."; peak electron-temperature perturbation 3815 K / 3585 K, "set by the cooling bottleneck rather than the heating strength (paraphrase, not a quotation)."

Basis: percentage electron-density depletion; temperature in K; 1 GW beam, 2.45/5.8 GHz

Related records
Answers question
QST-001 not published in this release
Supersedes
CLM-0140 not published in this release

Cite this

energyaperture.com/c/clm-0440

CLM-0440, Energy Aperture, as of 2026.

Connected records

Other published records linked to this one. A list, not a judgement.

Also from SRC-105
CLM-0058 (low confidence)A 2026 modelling paper finds that a reference space solar power beam stays well below the instability thresholds at both candidate...
CLM-0109In normal conditions the ionosphere takes essentially none of the beam. In a severe solar storm it could take a little under a fifth of it.
CLM-0130The quiet-condition absorption figures from four sources do not disagree. One of them states an upper bound and the others sit inside it.
CLM-0461The ionosphere absorbs about one part in a hundred thousand of the beam. It is not a meaningful loss.