Closed schuhmaj closed 1 year ago
@gomezzz The results seem to be okay. I got a half-heart attack when I saw the results for Nimbus-6. However, comparing two different outcomes of the original implementation with each other yields similar results (probably related to the smaller sample number):
Kolmogorov–Smirnov tests for fork and original implementations results
======fengyun======
L_c Result:
KstestResult(statistic=0.015267175572519083, pvalue=0.7678690653423059)
A/M Result:
KstestResult(statistic=0.02132140036851803, pvalue=0.353660015971757)
DV Result:
KstestResult(statistic=0.020531718873387735, pvalue=0.3999385532889875)
======iridium_cosmos======
L_c Result:
KstestResult(statistic=0.01618614061709661, pvalue=0.6783201007984564)
A/M Result:
KstestResult(statistic=0.012139605462822459, pvalue=0.9327670546409319)
DV Result:
KstestResult(statistic=0.014162873039959535, pvalue=0.8227115174375315)
======nimbus6======
L_c Result:
KstestResult(statistic=0.05662983425414365, pvalue=0.19607762570973)
A/M Result:
KstestResult(statistic=0.052486187845303865, pvalue=0.27161625352963614)
DV Result:
KstestResult(statistic=0.03867403314917127, pvalue=0.6514207246693081)
divide by 1000 --> 1e6
). I fixed this.And I decided to use a slightly modified formula so that the remnant cannot be heavier than the initial target satellite. It would be kind of weird if the collision of a 560kg and 950kg satellite yields a new 1500 kg satellite. Or is such a thing possible? That the satellites connect somehow?
Otherwise, if you give a green light, this can be merged, but not by me, since I don't have any rights to this repository ;)
@gomezzz Hmm, on the other hand, the authors would not have proposed that formula if it would not make sense. If one satellite is more massive, I guess it’s Reasonable to assume that parts will get stuck in it. Nevertheless, in the concrete example above: A 560 kg satellite crashing into a 950 kg satellite with 100 m/s leading to a 1500 kg fragment?
What Do you think? Limit the size of the remnant to the greater satellite’s size or not?
Hmm, on the other hand, the authors would not have proposed that formula if it would not make sense. If one satellite is more massive, I guess it’s Reasonable to assume that parts will get stuck in it. Nevertheless, in the concrete example above: A 560 kg satellite crashing into a 950 kg satellite with 100 m/s leading to a 1500 kg fragment?
What Do you think? Limit the size of the remnant to the greater satellite’s size or not?
I am a bit out of my depth here. Maybe you can ask our contact what they think?
@gomezzz Yeah, that might be a good idea. However, at first, I would argue that we merge this first. Since this fixes a bug + the behavior is only slightly changed for non-catastrophic collisions with enabled mass Conservation. A configuration that previously was not recommended. So either way, it is an improvement, even if a follow-up patch would be necessary.
Changelog
Overview
addFurtherFragments()
). This method adds fragments until the collision mass (not total involved mass) has been reached (ergo: no change for catastrophic collisions, but a reasonable change for non-catastrophic collisions)4 needs to be merged first!
4 actually introduced a bug. Due to the squared impact velocity, we need to divide by
1e6
not1e3
--> FIXEDComment
Generally, there is a wide variety of approaches available. Whereas the original publication does not mention mass conservation at all [1], other procedures fulfill mass conservation in a basic way of just regenerating fragments [2].
Both approaches have the advantage that the L_c distributions are not artificially changed. However, all models are empirical, so changes are always reasonable as the concrete strategy is based on the considered/ observed breakups.
[3] [4] [5] both propose some modifications. In the following, I stick to [3] with implementation comments:
Sources
[1] Johnson, N. L., Krisko, P. H., Liou, J. C., & Anz-Meador, P. D. (2001). NASA's new breakup model of EVOLVE 4.0. Advances in Space Research, 28(9), 1377-1384.
[2] Bade, A., Jackson, A. A., Reynolds, R. C., Eichler, P., Krisko, P., Matney, M., ... & Johnson, N. L. (1998). Breakup model update at nasa/jsc. In 49th International Astronautical Congress.
[3] Krisko, P. H. (2011). Proper implementation of the 1998 NASA breakup model. Orbital Debris Quarterly News, 15(4), 1-10.
[4] Andrișan, R. L., Ioniță, A. G., González, R. D., Ortiz, N. S., Caballero, F. P., & Krag, H. (2017). Fragmentation event model and assessment tool (FREMAT) supporting on-orbit fragmentation analysis. In 7th European Conference on Space Debris.
[5] Radtke, J., Mueller, S., Schaus, V., & Stoll, E. (2017, April). LUCA2-an enhanced long-term utility for collision analysis. In Proceedings of the 7th European Conference on Space Debris. Darmstadt, Germany: ESA Space Debris Office.
[6] Horstman, A. (2020). Enhancement of s/c Fragmentation and Environment Evolution Models. Final Report, Contract N. 4000115973/15/D/SR, Institute of Space System, Technische Universität Braunschweig, 26(08).