Radiation Hard Electronic Design for LVO Long Mission

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TL;DR Summary
For std LEO electronic design, the modern radiation-hard components with a Single Event Latchup (SEL) Immune to LET = 85 MeV-cm2/mg are in a safe condition. What about for a Venus mission?
Venus does not have a magnetosphere, so the Galactic Cosmic Rays (GCRs) environment shall be much worse than in a LEO environment. Looking to the std radiation models for Venus, the standard radiation-hard space level electronic component with tested immunity LET = 85 MeV-cm2/mg seems not enough, so, for example, a 1cm2 Si die will suffer considerable flux above this level during a long mission (10 years for example). So, the question is, usually we are not paying attention to latch-up condition for LEO designs, as using tested immunity LET = 85 MeV-cm2/mg, but for a venus mission (LVO), shall be design be different, including additional protection against Latchup? Thank you!!!
 
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Arend said:
TL;DR Summary: For std LEO electronic design, the modern radiation-hard components with a Single Event Latchup (SEL) Immune to LET = 85 MeV-cm2/mg are in a safe condition. What about for a Venus mission?

venus mission (LVO),
LVO = Low Venus Orbit?

What references has one found regarding the radiation environment around Venus, or at

For example:

Venus Radiation environment monitor (VeRad) for the Venus Orbiter Mission
https://ui.adsabs.harvard.edu/abs/2022cosp...44..331S/abstract

Revisiting the cosmic-ray induced Venusian radiation dose in the context of habitability
https://www.aanda.org/articles/aa/full_html/2020/01/aa36968-19/aa36968-19.html

Ionization of the venusian atmosphere from solar and galactic cosmic rays
https://www.sciencedirect.com/science/article/pii/S0019103514004941

Venus has an orbit with a semi-major axis of 0.723 au (108,200,000 km; 67,200,000 mi), and an eccentricity of 0.007. Ref: https://en.wikipedia.org/wiki/Orbit_of_Venus

https://angeo.copernicus.org/articles/34/595/2016/angeo-34-595-2016.pdf

Galactic Cosmic Rays at Mars and Venus: Temporal Variations from Hours to Decades
Measured as the Background Signal of Onboard Microchannel Plates
https://iopscience.iop.org/article/10.3847/1538-4357/ac9a49/pdf

For those not familiar with SEU or SEL. (single event upset or latchup)
https://en.wikipedia.org/wiki/Latch-up

https://www.ti.com/lit/rr/slvk043a/slvk043a.pdf?ts=1760173958547

https://www.doeeet.com/content/eee-...ion/single-event-latchup-protection-circuits/
 
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A Venus mission doesn't have anything you don't see in LEO. The radiation is just more intense:
* You accumulate an integrated dose quicker - but longer missions in Earth orbit can end up with the same.
* You get a higher rate of single event upsets. Plan the electronics accordingly.
 
Venus does not have a magnetosphere, so the Galactic Cosmic Rays (GCRs) environment shall be much worse than in a LEO environment. Looking to the std radiation models for Venus, the standard radiation-hard space level electronic component with tested immunity LET = 85 MeV-cm2/mg seems not enough, so, for example, a 1cm2 Si die will suffer considerable flux above this level during a long mission (10 years for example). So, the question is, usually we are not paying attention to latch-up...
Due to the constant never ending supply of "cool stuff" happening in Aerospace these days I'm creating this thread to consolidate posts every time something new comes along. Please feel free to add random information if its relevant. So to start things off here is the SpaceX Dragon launch coming up shortly, I'll be following up afterwards to see how it all goes. :smile: https://blogs.nasa.gov/spacex/

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