Ion Wind (EAD) Thruster: Thrust, Corona and Collector Grid

Estimate ion-wind thrust, thrust density and thrust per watt from corona onset and Townsend current. Size emitter arrays, collector grids and repeated stages.

#collector grid #EAD propulsion #ion wind #multistage propulsion #Peek law #thrust density #Townsend relation

This ionic wind thrust calculator estimates the performance of a positive-corona electroaerodynamic thruster in air. It is intended for engineers comparing electrode layouts, students studying EHD propulsion, and prototype builders deciding which measurements to make next. Enter a round emitter wire, its distance from the collector, and the applied DC voltage to obtain current, thrust, thrust density and thrust per watt.

The emitter array consists of parallel wires facing a conducting collector grid. Wire span, wire count and pitch define the active frontal area, including half a pitch beyond each outer wire. The calculator solves the electrostatic interaction between the wires and their images in a grounded plane. Peek’s law then estimates the voltage at which each wire starts emitting. Edge wires can start before the inner wires because neighbouring emitters shield one another.

For an initial design, select the Cooperman estimate for the Townsend current coefficient. This is a semiempirical wire–plane estimate with a derived array correction, rather than a calibrated prediction for a particular mesh. When test data are available, select the calibrated coefficient and enter C divided by total active emitter length. A measured onset can also replace Peek’s estimate. Recalibrate after changing the gap, mesh or emitter arrangement. Plane-field estimates require a collector at least four gaps wide and an outer-wire side margin of at least one gap; smaller collectors require both measured onset and current.

Ideal ion force follows the current–distance relation I d/μ. The retained thrust uses a separate assembly retention factor to represent collector drag and other losses. The default retention of 0.7 is an illustrative assumption, not a measured property of the entered grid. Grid transparency alone cannot determine this factor. Electrode power and supply power are reported separately, so high-voltage conversion losses are included in the supply thrust-per-watt result.

Repeated emitter–collector stages share the same frontal area and each operates at the entered voltage. They are parallel electrical loads arranged along the airflow. The stage table compares cumulative thrust, power and both area and volume density. Use the successive-stage current ratio to represent measured electrical interaction. Overall thrust retention must represent the complete stack. Increasing stage count does not automatically improve thrust per watt. This unshielded layout requires two forward gaps of clearance between a collector's back face and the next wire surface. The field screen also checks that backward path.

The curves show the current rise after onset and the tradeoff between thrust density and thrust per supply watt. Thrust per watt has units of force divided by power; it is not a percentage efficiency. Below onset, thrust and power are zero, and the undefined ratio is omitted from the tradeoff curve.

This EHD thruster tool does not calculate sparkover, reverse corona, three-dimensional end fields, insulation distances, ozone production or aircraft flight performance. The electrode envelope excludes supports, power electronics and batteries. An ion propulsion drone needs a separate mass, aerodynamic and stability analysis. Electrical construction and installation belong to a qualified person, with appropriate high-voltage protection and ventilation.

How it is calculated

Corona onset. Use relative air density δ=(p/101.325 kPa)(293.15 K/T)\delta=(p/101.325\,\mathrm{kPa})(293.15\,\mathrm{K}/T) and Peek’s surface field Ec=3×106msδ[1+0.0301/δr]E_c=3\times10^6 m_s\delta[1+0.0301/\sqrt{\delta r}] in V/m with rr in metres. The curvature constant has units m\sqrt{\mathrm m}. Drew and Pister (2017), p. 4, Eq. (6), gives the wire–plane form at reference density. For a single wire this yields V0=Ecrln⁡(2d/r)V_0=E_c r\ln(2d/r).

Emitter interaction. The grounded-plane image-charge solution is derived here. Define Gii=ln⁡(2d/r)G_{ii}=\ln(2d/r) and Gij=12ln⁡[1+(2d/sij)2]G_{ij}=\tfrac12\ln[1+(2d/s_{ij})^2] for wire spacing sij=∣i−j∣ss_{ij}=|i-j|s. Solve Ga=1G a=\mathbf1. The line charge is 2πϵ0Vai2\pi\epsilon_0 V a_i and, neglecting the small variation of external field around a thin wire, the local surface field is Vai/rV a_i/r. Thus V0,i=Ecr/aiV_{0,i}=E_c r/a_i. A measured common onset can replace this calculation.

Townsend current. Each wire carries Ii=CiVmax⁡(V−V0,i,0)I_i=C_i V\max(V-V_{0,i},0). Masuyama’s MIT thesis (2012), printed p. 24, Eq. (1.20), gives Cooperman’s wire–plane estimate C=2πϵ0μL/[d2ln⁡(fgeo/r)]C=2\pi\epsilon_0\mu L/[d^2\ln(f_{geo}/r)]. Here the isolated-plane choice is fgeo=2df_{geo}=2d; the derived array extension replaces the reciprocal logarithm by aia_i, giving Ci=2πϵ0μLai/d2C_i=2\pi\epsilon_0\mu L a_i/d^2. This extension is an estimate, not Gilmore and Barrett’s experimental correlation. Alternatively set Ci=cmeasuredLC_i=c_{measured}L using a coefficient fitted for the actual layout and air conditions. Drew and Pister, p. 4, Eq. (5), supports the Townsend relation and need for calibration.

Force and power. With stage ratio qq, stage kk carries Ik=I1qk−1I_k=I_1q^{k-1}. Sum these stage currents; do not multiply the voltage by the stage count. Ideal axial ion force is F=∑Ikd/μF=\sum I_k d/\mu; retained assembly thrust is T=βFT=\beta F. Electrode power is PHV=V∑IkP_{HV}=V\sum I_k and supply power is Pin=PHV/ηHVP_{in}=P_{HV}/\eta_{HV}. This is the drift-current force relation used by Masuyama and Barrett (2013); T/PT/P is a dimensional performance ratio.

Packing and grid sizing. Frontal area is A=LnsA=Lns. Stack depth is D=(N−1)h+d+t+rD=(N-1)h+d+t+r. Densities are T/AT/A and T/(AD)T/(AD). The square-aperture unit-cell open fraction is [a/(a+w)]2[a/(a+w)]^2. Complete cell counts along panel dimensions are ⌊(L−w)/(a+w)⌋\lfloor(L-w)/(a+w)\rfloor and ⌊(ns−w)/(a+w)⌋\lfloor(ns-w)/(a+w)\rfloor. Their openings define finite panel transparency; leftover margins are solid metal. Collector metal volume is Nt(A−Aopen)N t(A-A_{open}). The planar space-charge benchmark is 9ϵ0(V/d)2/89\epsilon_0(V/d)^2/8 per stage (Drew and Pister, p. 3); it does not cap the model.

Collector-width screen. Across the array, W=nsW=ns and the outer-wire centre-to-side-edge margin is m=s/2m=s/2. If either onset or current uses a plane-field estimate, require W≥4dW\ge4d and m≥dm\ge d; otherwise both onset and current must be measured for the complete layout. The geometric screen is derived here from the normal self-image field of an isolated line charge. Truncating the infinite-plane induced charge to a strip gives the retained fraction f=[H(m/d)+H((W−m)/d)]/πf=[H(m/d)+H((W-m)/d)]/\pi, with H(z)=arctan⁡z+z/(1+z2)H(z)=\arctan z+z/(1+z^2). At the worst permitted corner m=dm=d, W=4dW=4d, this fraction is 0.9022. This diagnostic supports the chosen dimensions; it is not an error bound on a finite-conductor solution, nor a validation of the current estimate. The span direction retains the long-wire approximation.

Interstage domain. The nearest surface clearance from a previous grounded collector to the next emitter is gb=h−d−t−rg_b=h-d-t-r. Require gb≥2dg_b\ge2d for this unshielded repeated-wire estimate. Nelson and Drew, §III.B and §IV.C (PDF pp. 3, 5), discuss the earlier wire-geometry two-gap heuristic and failures from unwanted interstage discharge. The nominal bulk-field screen checks both V/(d−r)V/(d-r) and V/gbV/g_b; a single stage has no backward path. These checks do not calculate sparkover.

Assumptions

Positive, steady DC corona in near-ambient air; straight round emitters; thin-wire electrostatics and a plane-equivalent collector. Ion drift dominates air convection, with constant supplied ion mobility and negligible recombination. The active span is long compared with the gap.

Every stage has its own emitter and collector, with all stages at the same applied potential difference. The current ratio represents stage interaction; overall retention represents the complete assembly’s force losses. This repeated-stage layout is distinct from the three-electrode, decoupled ionization/acceleration arrangement studied by Masuyama and Barrett.

The default mobility of 2 cm²/(V·s) follows Drew and Pister’s force convention (p. 9). Default retention 0.7, stage ratio 1 and converter efficiency 0.85 are design assumptions. They are not experimental fits. The calibrated Townsend coefficient is per total emitter length at the entered operating conditions, including array interaction. Transparency sizes the grid; it is not multiplied into thrust a second time.

Successive stages are aligned, unshielded wire arrays at the same positive emitter voltage, each followed by a grounded planar grid. Stage spacing is measured between wire-centre planes; collector thickness and emitter radius are subtracted when evaluating the preceding-collector clearance.

Where it applies

Use the geometry current mode for preliminary sizing and calibrate current, onset and complete-stack retention before relying on absolute thrust. The image-charge onset calculation is a Laplace-field thin-wire approximation; its array-current extension does not solve space-charge transport. After the first wire emits, space charge may also shift the remaining onset thresholds. Long-span, sparse-wire assumptions become less accurate near ends, closely packed arrays and a collector whose grid pitch exceeds its distance from the emitters.

Peek’s isolated round-wire onset is typically an approximate prediction. The reference checks compare it with Masuyama’s wire–cylinder measurements to 10% without fitting the constants. Density correction uses a 20 °C, 101.325 kPa reference. Supply mobility for the actual humidity, temperature, pressure and field; this tool does not infer mobility from those conditions. If the ionization sheath is a significant part of the gap, Id/μId/\mu overestimates the useful drift contribution.

Collector drag, ion interception, reverse corona, leakage, finite-span fields and downstream aerodynamic interaction are represented only by calibrated coefficients and retention, or remain outside the model. A stage current ratio of 1 assumes independent electrical operation and does not establish independent airflow. The planar space-charge result is a comparison scale, not a universal bound for a nonuniform finite array. Neither it nor the nominal bulk-air-field warning predicts sparkover.

Voltage sweeps contain 301 directly calculated points and may extend beyond the stable corona range of real hardware. They are not operating-voltage limits. At zero current, displayed thrust-per-watt results use the off-state convention zero; the curve omits this undefined ratio. The drawing is schematic, with enlarged wire sections and grid ribs. The stack envelope excludes frames, insulation, wiring, converter and battery.

High voltage and corona byproducts require electrical protection and ventilation. Insulation coordination, ozone exposure and discharge stability must be assessed separately; the calculator does not perform those assessments.

The finite-collector limits apply whenever either Peek onset or the Cooperman current estimate is selected. Measurements must cover the same complete array, grid, air conditions and operating-voltage range. Changing only one coefficient does not replace the other plane-field approximation. The truncated-plane image-field diagnostic describes an isolated wire's self-image contribution; it does not solve charge redistribution on a finite plate, and a 90% diagnostic does not imply 10% thrust accuracy.

The two-gap interstage threshold is a preliminary spacing screen inherited from wire-to-cylinder guidance, not experimental validation of this wire-to-grid stack. Bent, shielded, offset or independently biased stages are outside the entered geometry. Retention must still include any backward-current force and aerodynamic losses; spacing alone does not establish independent discharge. At rejected overlaps the backward-field denominator is bounded by the emitter radius to keep evaluation finite.

References

  • Masuyama, K. and Barrett, S. R. H. (2013). On the performance of electrohydrodynamic propulsion. Proceedings of the Royal Society A 469, 20120623. https://doi.org/10.1098/rspa.2012.0623
  • Gilmore, C. K. and Barrett, S. R. H. (2015). Electrohydrodynamic thrust density using positive corona-induced ionic winds for in-atmosphere propulsion. Proceedings of the Royal Society A 471, 20140912. https://doi.org/10.1098/rspa.2014.0912
  • Xu, H. et al. (2018). Flight of an aeroplane with solid-state propulsion. Nature 563, 532–535. https://doi.org/10.1038/s41586-018-0707-9
  • Drew, D. S. and Pister, K. S. J. (2017). Geometric Optimization of Microfabricated Silicon Electrodes for Corona Discharge-Based Electrohydrodynamic Thrusters. Micromachines 8, 141, pp. 3–5, 8–10. https://doi.org/10.3390/mi8050141
  • Masuyama, K. (2012). Performance characterization of electrohydrodynamic propulsion devices. MIT SM thesis, September 2012; Eqs. (1.17)–(1.20), Table A.1. https://hdl.handle.net/1721.1/77114 ; open copy: https://riseflyorbit.org/downloads/LAE-2012-008-T.pdf
  • Nelson, C. L. and Drew, D. S. High Aspect Ratio Multi-stage Ducted Electroaerodynamic Thrusters for Micro Air Vehicle Propulsion. Author manuscript, §III.B and §IV.C, PDF pp. 3, 5. https://drl.ece.utah.edu/wp-content/uploads/sites/155/2023/08/RALHighARDucted.pdf

Inputs

InputSymbolUnitDefault
Applied stage voltageV_appkV20
Emitter wire diameterd_wiremm0.2
Wire centre to collectorgapmm50
Active wire spanspanmm400
Emitter wires per stagen_wire4
Emitter wire pitch
The panel has half a pitch of margin beyond each outer wire.
pitchmm100
Corona onsetonset_modelPeek law with array shielding
Emitter surface factor
Use 1 for a smooth round wire; lower values require an onset measurement.
surface1
Measured onset voltage
A common onset for all wires, measured in this electrode arrangement.
V_measkV8.3
Townsend coefficientcurrent_modelCooperman array estimate
Calibrated Townsend coefficient
Fit I = C V(V − V₀), then divide C by total emitter length at these conditions.
c_measuA/(kV^2*m)0.6
Ion mobility at operating conditions
Positive air ions typically span about 1.37–2.8 cm²/(V·s); humidity changes this value.
mu_ioncm^2/(V*s)2
Absolute air pressurep_airkPa101.325
Air temperatureT_airdegC20
Collector clear square apertureaperturemm5
Collector rib widthribmm0.5
Collector sheet thicknessthickmm0.25
Stages along the airflown_stage3
Stage centre spacing
Emitter-plane spacing must leave two forward gaps from the previous collector's back face to the next wire surface.
stage_pitchmm160
Successive stage current ratio
I₂/I₁ = I₃/I₂ = …; use measured data, or 1 for independent stages.
q_stage1
Overall thrust retention
Measured assembly thrust divided by total I d/μ; 0.7 is an illustrative assumption.
retention0.7
High-voltage supply efficiencyeta_hv0.85

Results

With the default inputs above, the calc gives:

ResultValue
Retained thrust107.8 mN
Frontal thrust density0.6737 N/m²
Volumetric thrust density1.8192 N/m³
Thrust per electrode watt8.75 mN/W
Thrust per supply watt7.438 mN/W
Total electrode current0.616 mA
Electrode power12.3196 W
Supply power14.4936 W
First corona onset8.9007 kV
All-wire onset9.303 kV
Ideal ion force154 mN
Corona stateAll wires emitting
Active frontal area0.16 m²
Electrode stack depth370.3 mm
Electrode envelope0.0593 m³
Total active emitter wire4.8 m
Finite grid open area (%)81
Apertures per collector5,184
Total collector metal volume22.8 cm³

Checked against sources

Each case below was calculated by this calc and agrees with the value from its source (within the tolerance where one is shown).

Measured onset, 10 mm wire–cylinder gap

Source: Masuyama, MIT SM thesis (2012), Table A.1, printed p. 79 (PDF p. 80): positive-corona onset 6.92 kV for a 0.202 mm wire and 10 mm gap. https://riseflyorbit.org/downloads/LAE-2012-008-T.pdf. This is a cylinder collector, so the plane approximation is checked to 10%; no fit of Peek constants is made.

Inputs: Emitter wire diameter = 0.202 mm; Wire centre to collector = 10 mm; Emitter wires per stage = 1; Stages along the airflow = 1; the others as above.

ResultSourceThis calc
First corona onset6.92 ± 0.692 kV6.402 kV

Measured onset, 30 mm wire–cylinder gap

Source: Masuyama, MIT SM thesis (2012), Table A.1, printed p. 79 (PDF p. 80): positive-corona onset 8.28 kV for a 0.202 mm wire and 30 mm gap. https://riseflyorbit.org/downloads/LAE-2012-008-T.pdf. Wire–plane Peek prediction is compared to this wire–cylinder measurement with 10% tolerance. The virtual plane comparison uses a 120 mm-wide panel to meet its own width screen; the measured collector was cylindrical.

Inputs: Emitter wire diameter = 0.202 mm; Wire centre to collector = 30 mm; Emitter wires per stage = 1; Stages along the airflow = 1; Emitter wire pitch = 120 mm; the others as above.

ResultSourceThis calc
First corona onset8.28 ± 0.828 kV7.731 kV

Published grid open fraction, 25 μm ribs

Source: Drew and Pister (2017), Micromachines 8, 141, p. 9: approximately 91% open area for 500 μm clear spacing and 25 μm ribs. Independent published geometry value, rounded to whole percent. DOI 10.3390/mi8050141.

Inputs: Collector clear square aperture = 0.5 mm; Collector rib width = 0.025 mm; the others as above.

ResultSourceThis calc
Periodic grid open fraction0.91 ± 0.010.907

Published grid open fraction, 50 μm ribs

Source: Drew and Pister (2017), Micromachines 8, 141, p. 9: approximately 83% open area for 500 μm clear spacing and 50 μm ribs. Independent published geometry value, rounded to whole percent. DOI 10.3390/mi8050141.

Inputs: Collector clear square aperture = 0.5 mm; Collector rib width = 0.05 mm; the others as above.

ResultSourceThis calc
Periodic grid open fraction0.83 ± 0.010.8264

Published Townsend current, optimized emitter

Source: Drew and Pister (2017), Fig. 7b, p. 8: approximately 53 μA at 2000 V, read from the optimized-emitter data points; ±3 μA allows graph reading and fit residual. Published V₀ = 1542 V and total C = 5.63e−11 A/V² are supplied. A 1 m normalization length converts this total C into the per-length input; this does not assert a 1 m experimental span. Only the calibrated Townsend relation is checked, not the round-wire geometry estimate for this spined electrode. DOI 10.3390/mi8050141.

Inputs: Applied stage voltage = 2 kV; Corona onset = Measured onset; Measured onset voltage = 1.542 kV; Townsend coefficient = Calibrated C per length; Calibrated Townsend coefficient = 56.3 uA/(kV²·m); Active wire span = 1,000 mm; Emitter wires per stage = 1; Stages along the airflow = 1; Wire centre to collector = 0.5 mm; Emitter wire diameter = 0.04 mm; Collector clear square aperture = 0.5 mm; Collector rib width = 0.025 mm; the others as above.

ResultSourceThis calc
First-stage corona current5.3 × 10⁻⁵ ± 3 × 10⁻⁶ A5.157 × 10⁻⁵ A

Measured current-to-thrust slope, 10 mm gap

Source: Masuyama, MIT SM thesis (2012), Table A.1, printed p. 79: a₁ = 53.88 mN/mA at d = 1 cm. Compare d/μ using the independent 2 cm²/(V·s) mobility convention from Drew and Pister (2017), allowing 10% for unknown humidity and geometry. a₁ is defined as a thrust-current slope by Eq. (1.40) and §4.1.1, p. 62; the appendix prose incorrectly calls it a voltage-current slope. No mobility is fitted to the measured slope. https://riseflyorbit.org/downloads/LAE-2012-008-T.pdf

Inputs: Wire centre to collector = 10 mm; Emitter wires per stage = 1; Stages along the airflow = 1; the others as above.

ResultSourceThis calc
Ideal current-to-force conversion53.88 ± 5.388 N/A50 N/A

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