Comprehensive in-orbit performance evaluation of the BepiColombo Laser Altimeter (BELA)

Hosseiniarani, Alireza; Bertone, Stefano; Arnold, Daniel; Stark, Alexander; Hussmann, Hauke; Beck, Thomas; Herny, Clémence; Pommerol, Antoine; Jäggi, Adrian; Thomas, Nicolas (2021). Comprehensive in-orbit performance evaluation of the BepiColombo Laser Altimeter (BELA). Planetary and space science, 195, p. 105088. Elsevier 10.1016/j.pss.2020.105088

[img] Text
1-s2.0-S0032063320303019-main.pdf - Published Version
Restricted to registered users only
Available under License Publisher holds Copyright.

Download (8MB) | Request a copy

The BepiColombo Laser Altimeter (BELA) is on its way to Mercury on board the Mercury Planetary Orbiter (MPO), one of the two spacecraft of the BepiColombo mission. It will arrive at Mercury in December 2025 and start measurements of Mercury’s surface and environment. The goal of this study is to analyze the performance of BELA by using a comprehensive in-orbit performance model of the instrument.

To determine the in-flight performance, we model the laser altimeter instrument noise based on laboratory tests performed on BELA. In order to obtain the most realistic in-flight performance, we add a realistic instrument degradation model on top of it. We thus obtain the probability of false detection for each simulated observation and based on that, we produce a coverage map over different surface terrains.

We show that the pointing uncertainty dominates the range measurement error. Moreover, we compare the predicted working limit using different gain settings and we show that instrument degradation can lower the working limit of the instrument by around 200 ​km in the worst case scenario.

Finally, we produce BELA measurement performance maps over the surface of Mercury, study the attainable quality of topography recovery and determine the expected accuracy of the measurements of surface properties, e.g., local slopes, surface roughness and albedo in different conditions and over different terrains.

We also suggest potential improvements to instrument operations by choosing an optimum gain setting and by combining different measurements together when constructing a digital terrain model of Mercury.

Item Type:

Journal Article (Original Article)

Division/Institute:

08 Faculty of Science > Institute of Astronomy
08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences
08 Faculty of Science > Physics Institute
10 Strategic Research Centers > Center for Space and Habitability (CSH)
08 Faculty of Science > Physics Institute > NCCR PlanetS

UniBE Contributor:

Hosseiniarani, Seyed Alireza; Arnold, Daniel; Beck, Thomas; Herny, Clémence Emilie Lucile; Pommerol, Antoine; Jäggi, Adrian and Thomas, Nicolas

Subjects:

500 Science > 520 Astronomy
600 Technology > 620 Engineering

ISSN:

0032-0633

Publisher:

Elsevier

Language:

English

Submitter:

Dora Ursula Zimmerer

Date Deposited:

25 Mar 2021 15:06

Last Modified:

28 Mar 2021 03:58

Publisher DOI:

10.1016/j.pss.2020.105088

BORIS DOI:

10.7892/boris.152809

URI:

https://boris.unibe.ch/id/eprint/152809

Actions (login required)

Edit item Edit item
Provide Feedback