Energy Aperture

Value chain · CLM-0960

In plain terms

The 1975 study found the satellite's harmonics - the multiples of its transmit frequency - would trouble radio astronomy at the second and third harmonic, would trouble ordinary radio only at the klystron's second harmonic unless a filter was added, and would be clear at the fourth. A later reading of a redrawn chart says all three harmonics exceed everything. The original does not say that.

The claim as recorded

The same study's harmonic analysis concludes that the klystron converters' second harmonic would interfere with commercial services without a further -22 dB filter, that the second and third harmonics of all converters would interfere with radio astronomy but not with commercial services, and - verbatim - that "The fourth harmonic of all three tubes is below the level of radio astronomy (Class A)." It recommends that "Radio astronomy and similar sensitive receiving systems will need notch filters to protect against MPTS harmonics." SRC-439 reads SRC-111's redraw of this as "the 2nd, 3rd, and 4th harmonics will all exceed various CCIR recommendations, and ITU regulations for both Klystron and Amplitron systems". The primary says the fourth clears radio astronomy and only the klystrons' second touches commercial.

Evidence behind this: T3-primary-report, the primary behind SRC-111's Figure C.

Scope and limits

COMPUTED, NOT MEASURED - a power budget of total power plus effective harmonic gain minus path loss minus three filter terms, with harmonic gains of 18.7 to 34.4 dB from an effective-area argument using a K factor of 0.15, 0.04 and 0.01 that the report itself calls an estimate. Where the broadening to "all three exceed" happened is settled in two steps and only the second is an overstatement: SRC-111's Figure C keeps the data faithful to the dB but substitutes its own, stricter and later limit lines, cited on the figure - CCIR 1974 Report 387-2 for line-of-sight links at about -140 to -150, against the -116 this study used - so on SRC-111's own figure the klystron third harmonic exceeds too, and its text says exactly that: "in some cases (e.g., 3rd harmonic) violate ITU radio regulations". SRC-111 does not say the fourth exceeds; on its own figure the amplitron fourth sits 20 dB below the radio-astronomy line. The broadening to the fourth is SRC-439's reading of the redraw, not the redraw.

What it assumes

No assumptions are recorded against this claim.

Where it comes from

SRC-451 Microwave Power Transmission System Studies, Volumes I to IV, December 1975, NASA-CR-134886,...
SRC-111 PNL-2482: Initial Assessment of Electromagnetic Compatibility of the SPS Microwave Power...
SRC-439 Preliminary Study: Electromagnetic Compatibility, Tropospheric and Ionospheric Aspects of SPS...
Computed on PDF p.60: amplitron with filter at 2f0, 3f0, 4f0 of -144, -147, -185 dBW/m2; 5 kW klystron -104, -141, -174; 48 kW klystron -95, -132, -165. Limits: worst-case commercial IRR about -116; radio astronomy isotropic IRR rising from about -177 at 3 GHz to -163 at 10 GHz, taken from "REP 224-2, page 437" - SRC-111 cites 224-3 Annex 1, the next edition, which is not an error. The fourth-harmonic sentence matches at the normalised level on PDF p.61; the notch-filter sentence on p.63. The -22 dB filter and the per-service conclusions are transcribed from letterspaced pages. The two secondaries read directly: SRC-111 PDF p.20, "Figure C shows estimated levels of harmonic power (from Reference R-31) with recommended interference limits. Because of uncertainties in antenna gains and appropriate bandwidths comparison of the two is not entirely straightforward" (normalised; "1 eve1 s" for "levels"), and PDF p.22, "SPS harmonic radiation would exceed established recommendations and in some cases (3.g., 3rd harmonic) violate ITU radio regulations" ("3.g." for "e.g." in the text layer). SRC-439 PDF p.11, normalised: "the report shows that the znd, 3rd, and 4th harmonics will all exceed various CCIR recommendations, and ITU regulations for both Klystron and Amplitron systems" ("znd" for "2nd", "a l l" letterspaced), followed by "It is assumed that the levels given are mainbeam levels."

Basis: dBW/m2 power flux at the earth's surface, by harmonic

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

Cite this

energyaperture.com/c/clm-0960

CLM-0960, Energy Aperture, as of 1975.

Connected records

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

Also from SRC-111
CLM-0918The 1978 study of what a solar power satellite would do to the radio spectrum found two things. Its transmitter NOISE would exceed what...
CLM-0919In 1978 there was no rule allowing a solar power satellite to transmit power, and the industrial band everyone assumed it would use permits...
CLM-0920The 1978 study says a solar power satellite cannot keep its beam entirely on the receiving station - the physics of beams forbids it - so...
CLM-0921The 1978 report says the power density a solar power satellite apparently needs to make economic sense was thought to be about the same as...
CLM-0959The original 1975 calculation found the satellite's radio noise would be fine for ordinary and troposcatter radio links and a problem only...
CLM-0961Everything in the 1975 interference analysis is for one satellite. The study itself says that a hundred of them would raise the noise and...
CLM-1315The 1975 estimate of the satellite's radio noise, taken at its own frequency, is about a hundred million times above today's threshold for...
Also from SRC-439
CLM-0927The 1978 review found an interference route the report it was reviewing never considered: the power beam bouncing off rain, hail or blown...
Also from SRC-451
CLM-0954The 1975 designers worked out how much their kilometre-wide antenna would bend, precisely so they could decide how good the beam-steering...
CLM-0959The original 1975 calculation found the satellite's radio noise would be fine for ordinary and troposcatter radio links and a problem only...
CLM-0961Everything in the 1975 interference analysis is for one satellite. The study itself says that a hundred of them would raise the noise and...
CLM-0965In 1973 an astronaut on Skylab put together two long poles from short sections in just over two hours, about six minutes per join. A 1975...
CLM-0966In 1975 the antenna alone was expected to take one to two years to assemble in orbit with about fifty people, and robot arms were judged...
CLM-0968The 1975 antenna study worked out how hot the middle of the transmitter gets depending on how efficient the tubes are and how tightly they...
CLM-0969If the tubes are only 70 per cent efficient, the transmitter's own face is not big enough to get rid of the heat they make, even spread...
CLM-0972If you take a 1975 estimate of how fast people could build structure in space, checked against one Skylab task, and apply it to the 1978...
More on the source page.