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Id : 335
Type : BUG
Reporter : Fredrik Johansson
Assignee :
Benoit Thiebault
Priority : BLOCKER
Creation Date : 20 Jan 16 03:26
Last Update Date : 20 Jan 16 04:56
Resolution : Fixed
Secondary Yield unrealistically high at low energies
Hello!

I'm getting a SEE yield of 1 at 10eV electrons for ITO (no modifications) for a negatively charged spacecraft doing Langmuir probe sweeps in a cold plasma.

More info below:

I'm doing some Langmuir probe sweeps with secondary electrons from electron impact (SEE). It's not very straight forward as you know, as the SEE sweep current will only give me the collected current, and not the emitted current. This is sort-of okay when dealing with photoemission, since we can assume it to be static during the sweep, but since the electron current increases as the probe steps upwards in bias, so does the secondary emission.

(This is an issue I really wish somebody would fix, but that's a different topic. Also, I found a complex way) around this by using the emitted_currents.txt file, and very carefully modelling the emission)

however: look at the end result for the electron + SEE sweep http://imgur.com/PV6X2hj

Disregarding everything but the electron current (purple crosses) and the SEE collection current(blue dots), as they are outputted when doing the sweep

Already at Vb = 20 V, the collected SEE current is much higher than the collected electrons. This is about the point where most emitted SEEs are recollected by the probe, as seen in my model current(orange circles, the SEE sweep + modelled emission) approaches zero.

This represent (if I'm not going crazy) a SEE Yield of one, as the emission and collection is of the same size, and the current collection of SEEs from the spacecraft should be negligble since the spacecraft is highly negative an repel everything to infinity, so what's left are the secondaries emitted by the probe. That's the logic part, but It's also supported by the calculations I did of the emission.

a Yield of 1 at 20 Vb -> electrons accelerated by about 5 V, so 10eV tops. The SEEYield files in the simulation, SEEYield_materialId_ITOC material properties_isotropic.txt, (and others). state that the ITO should have a SEEYield of 0.24 at that point.

What is going on? Can somebody else confirm this? I've rerun the simulations and sweeps with different Emin/Emax, resolutions, steps, delay between steps. Can't make this huge secondary current go away.

Best regards, Fredrik


1 comment(s)
comment by Jean-Charles Mateo-Velez - 20 Jan 16 04:55 PM Hi, The current voltage I-V sweep for secondary electrons SEE takes into account SEE from all spacecraft surfaces. At Vb = +20 V, all SEE emitted by the probe may be recollected you're right. But I don't agree with your analysis of SEE from SC being repelled directly to infinity. 2 eV SEE from SC can be collected by the +20 V biased probe, even if the spacecraft is negative. A large spacecaft emits a large current and even a small fraction of it recollected by the probe may by significant for the probe, whose measurement is totally polluted. So to me, this is not a probem of SEEE yield computation. Hope this will help you.


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