... First, I don't quite understand the "10-28 W/m2", it seems, um, wrong. Perhaps the Tarter document was written rather too many years' ago? But I need to dig into it a bit more ...
Please do .. I'd appreciate it.

The Tarter document may well be out of date relative to technology improvements. (I'm always eager to be updated on the latest).
Regardless of the perhaps, (maybe), datedness of the numerical quantity, the search for SETI is fundamentally different from general radio astronomy and I think that was the general backdrop to her paper (at the time she authored it).
ETA: Her paper became available online 5 Nov 2004. See here. (So, yes, I accept its 12 years old ... please feel free to update the figure ..
JeanTate said:
Second, astrophysical sources of radio emission are now fairly well understood, certainly those 'close' to us are (i.e. within ~1 Mpc). None have spectra that look remotely like the integrated 'Earth radio emission', as viewed from afar, nor its variability.
Then that would count as evidence for a lack of radio-intelligent lifeforms and geophysical Earths within ~1 Mpc then, no?
JeanTate said:
If you'd like a quick tutorial on radio astronomy, I'd be happy to help ... but please, not in this thread (already far too many OT posts for my liking).
I'm always eager to learn more ... thank you for your offer.
Perhaps we could drill a little more into how SETI ('information signal') searches differ from astrophysical searches. Whilst there may be particular customisations for SETI, Tarter etal are clearly prepared to use any and all techniques to make sense and gather data of interest. (Thank goodness!)
As she points out in that paper, their searches are limited by the amount of time available for any given observation, and thence computer processing technologies (which clearly improves).
(I agree about the OT post count, too).
JeanTate said:
It's not so easy to give a visual analogy; the 'optical' is barely 1 dex wide, the 'radio' dozens of dex (I'm OOMing here). The Earth's integrated radio emission, if analogized to the optical, might be something like 'an intense, and variable, orange-yellow, with highly variable spikes in the violet'. No astrophysical source looks remotely like that, even at this qualitative level.
Again, perhaps evidence of the apparent scarcity of Earths .. (but perhaps not for long).
I think the distance factor needs to be layered on top of such qualitative comparisons. There are other parameters which come into play at larg(er) distances which in turn, call for models for interpretation.
JeanTate said:
Radio telescopes are generally located rather a long way from where lots of people live. And in their vicinity, there tend to be some rather strict local laws (or equivalent) re electronic equipment etc (though sometimes this has holes; e.g. the recent 'faulty microwave oven' that was identified as the cause of some interesting-looking RFI, at Parkes, IIRC).
Sure .. Eg: the latest RATAN 600 signal detection calls into question local military sources, too. Also, I notice they were using a receiver with a 1 GHz bandwidth (which produced a flux density of only 0.75 Jy). That's not the way Tarter's SETI organisation goes about 'its business'. (The signal only turned up once in 39 attempts, too).
JeanTate said:
The sky's background radio noise is ... not much (once you're well away from the CMB's main frequencies).
Sure .. which throws the emphasis back onto the detection method and technologies, because of the noise introduced by the receivers and processing. (Our observational eyes and ears, so to speak).
Eventually, we might get into discussing Optical SETI(?)
(Whose techniques are also becoming relevant for intra Solar System communications .. (just trying to link back to the OP topic here)).