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AAWSAP DIRD, Pulsed High-Power Microwave Source Technology, January 2010

U.S. Department of War · 2010-01-28 · 37 pages · text from the file's own layer

This Defense Intelligence Reference Document (DIA-08-0912-005) is dated 28 January 2010. The Defense Intelligence Agency's Defense Warning Office prepared it under the Advanced Aerospace Weapon System Applications Program. It gives an overview of pulsed high-power microwave sources and the technologies needed to build them, including insulation, cathode materials, high-voltage switching, pulse generators and antennas. The paper concludes that progress requires better cathodes, switching and insulation, and that compact ultrawideband antennas will remain difficult to build.

From the source:Release of 2026-09-18 Incident: 1/28/10, Las Vegas, Nevada. Released with redactions. This document is a Defense Intelligence Reference Document (DIRD), a technical reference format used by the Defense Intelligence Agency (DIA) to capture baseline knowledge on a specific topic for later analytic use. DIRDs are best understood as reference and synthesis products rather than as original research. It is one of 38 DIRDs produced under the Advanced Aerospace Weapon System Applications Program (AAWSAP) between 2009 and 2011. Because AAWSAP’s scope permitted a broad range of supporting topics, not every DIRD in the series directly concerns aerospace systems or future threat assessment. The following summary reflects the DIRD’s scope and framing at the time of writing and should not be read as implying current validation of the concepts discussed. This DIRD surveys pulsed high-power microwave (HPM) source technology and argues that such systems remain of military interest because they can disrupt or damage electronic systems with short, intense electromagnetic pulses. The report reviews the main source types and the supporting technologies they depend on, including high-voltage insulation, switching, cathode materials, antennas, and pulse-power generation. It emphasizes the difficulty of building systems that are compact, efficient, and practical to field, since short pulse durations, antenna size, heating, detectability, and beam or signal quality all impose hard engineering limits. Its overall conclusion is that the technology has significant potential military value, but that further progress depends on advances in cathodes, predictive modeling, high-speed high-voltage switching, and low-loss insulation, while compact ultrawideband systems will remain difficult because of basic physical constraints on antenna design.

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An oft-forgotten aspect of the spectral content is that the spectrum also contains only
the odd harmonics of the lowest frequency by the definition of a Fourier transform .
Thus, the faster the rise time and the wider the pulse, the broader the spectral content.
Therefore, switching speed is the most important parameter of a UWB HPM source. The
types of switches used for HPM are essentially the same as the types of insulation
discussed earlier: gaseous, liquid, and solid state at lower voltages. The single most
important attribute of gases and liquids in switching is their self-healing ability, wh ich
implies some measure of PRR capability.
GASEOUS SWITCHING
Gas switches are commonly used for HPM sources as both a prime power and a high
speed or peaking switch. As mentioned in the discussion of insulation earlier, when
used in a high-speed switch, gas pressure can pose substantial safety concerns. In fact,
all of the discussion regarding gaseous insulation also applies to gas switch ing, since a
gas switch is simply a gas-insulated region that we wish to fail in a timely fashion. The
higher the voltage impressed across a gas switch, the greater the pressure required to
prevent the switch from conducting until the peak voltage is reached. This is why when
a gas switch is used as a final-stage peaking switch, very high pressures are often
required. A fast-rising pulse is crucial to source design since the rise time determines
the upper frequency content. This is why UWB HPM sources usually contain a peaking
switch at the output to decrease the rise time and increase the spectral content. If the
peaking switch is charged past the DC breakdown level faster than streamers can form
conduction channels, then the final breakdown occurs in an overvolted (compared with
the DC breakdown voltage) switching state. The higher electric field strength between
the switch electrodes results in shortened breakdown t imes since breakdown develops
in an elevated electric field. All switches exhibit some capacitance to an applied pulse
because of their electrode spacing, resulting in a displacement current as this switch
capacitance charges. This is seen on the other side of the switch as a pre-pulse. The
magnitude of the pre-pulse depends on the rate of change of the charging voltage as
well as the electrode cross-sectional area and spacing. Sometimes efforts to reduce this
pre-pulse are required if it causes problems at the load or undesired spectral content
from the antenna. The pre-pulse phase of breakdown occurs at the speed of light in the
media since it is essentially a field phenomenon. Because of the added inductance and
design of the switch components, pre-pulse has a distinct charging profile . The next
phase of breakdown is a resistive phase as t he weakly conducting streamer channel
heats to the final arc or inductive phase and the switch is fully conductive. Since the
final phase is inductive, very low switch inductance and very short gaps are required for
fast rise times. Both t he resistive and inductive phase periods contribute to the rise
time as:
2 1 3 4 3
where: -rr = (88ns x p1
f (Z 1 x E 1) / )
with p being the gas density as a multiple of that for sea level air, Z is the circuit
impedance in ohms, and E is the electric field between the electrodes in kV/cm. Also, ,r
and TL are known as the resistive and inductive rise times, respectively. The resistive
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Official release, from the pursue collection. The PDF is mirrored here; the original link is above. 37 pages are in the text index: search them above, or from the library's search.