Does anyone know what a typical number of acquired frames is for a space telescope?
It might be compressed for transmission, but raw data (warts and all) is king .. once it's "processed" and raw data is discarded .. there's no recovering the raw.
Years later raw data can be reprocessed with new algorithms, faster processes and combined with other sources to create "better" processed images.
Onboard hardware errors (eg: the historic Hubble Telescope erros) can be "corrected" later on the ground with an elaborate backpropagated trandfer function that optimally "fixes" the error, etc.
Data errors (spikes in cell values, glitches from cosmic rays, etc) can be combed out of the raw in post .. if smart people have access to the raw.
Baking processing into on board instrument processing prior to transmission isn't a good procedure.
The launch mass of a petabyte of SSD is under 10 kg. I don't know if it would survive 17 years of space radiation though.
Probably worse than sending up well-shielded flash, but I don't think the Seagate/WD warranty expressly forbids this usage.
I don't think I'd do that.
Ignoring the failure modes of a petabyte of SSD spending decades in deep space, what kinds of things are difficult and|or impossible if you were to
> store all the data on the satellite, upload new code to process it differently, and download the resulting image
?
My understanding is that some newer instruments do both compress and select data to be downloaded (i.e. prioritizing signal over noise), and that there is more and more consideration of on-board processing for future missions, as well as possibly introducing the capability within DSN itself to prioritize which instruments get bandwidth based on scientific value of their data.
Source: A presentation from people at NASA Heliophysics last week, where this very topic came up.
[1]: < https://www.nasa.gov/communicating-with-missions/dsn/> [2]: < https://science.nasa.gov/mission/soho/>
Instead, we would use lasers with a far superior gain to what radio communication is capable of. The divergence on even a decent pocket laser pointer diode is less than 0.1 degree. This is a gain of 10*log10(41,253/(0.1*0.1)) = 66 degrees. Launch telescopes of modest size can increase this further. Then receiver telescopes fitted with narrowband filters can hone in on that laser signal.
> "First, transmitted beams from optical telescopes are far more slender than their radio counterparts owing to the high gain of optical telescopes (150 dB for the Keck Telescope versus 70 dB for Arecibo)." - https://www.princeton.edu/~willman/observatory/oseti/bioast9...
With no way to send commands to the decices?