MenuMENU

CLOUDS on BEXUS-38

A student experiment using a dual microspectrometer is on its way to the stratosphere

A group of young scientists from Giessen is currently setting up an experiment that will be flown on a stratospheric balloon as part of the BEXUS-38 mission. The project name: CLOUDSCalcium carbonate Light Observation Under stratospheric Dynamics and Scattering«).

Objective: to measure how calcium carbonate particles (CaCO₃) spectrally alter incident sunlight—and what this reveals about scattering effects. A dual microspectrometer from Eureca is planned as the central measuring instrument.

Esrange Launch Site: A stratospheric balloon ready for launch—the platform for BEXUS experiments. (©CLOUDS-Team)

  • Program: BEXUS-38 (Cycle 17)
  • Launch site: Esrange Space Center, Kiruna (Sweden)
  • Planned campaign: October 2026
  • Typical flight duration: approx. 2–5 hours
  • Measuring instrument: Dual microspektrometer with beam splitter
  • Spectral range: 350 – 850 nm
  • Spectral resolution: approx. 10 nm

e9u-SPMD-350/850-10-Duo dual microspectrometer (350 – 850 nm): Two optical paths for measurement and reference. (©EURECA)

Beam splitter: splits the light into a measurement path and a reference path. (©CLOUDS-Team)

Project Status

As of May 2026

The CLOUDS team is currently in the »system fine-tuning« phase: the visual design, reference concept (dual-path), and testing strategy are being finalized. On this page, we’ll document our journey to launch with regular updates—including interim progress reports, integration updates, and lessons learned.

Next milestone (planned)

  • Integration Progress Reviews: July 2026
  • Experiment Acceptance Review: Aug/Sep 2026
  • Launch Campaign: October 2026

What is BEXUS?

BEXUS stands for »Balloon Experiments for University Students«. Here, students have the opportunity to conduct their own scientific experiments using stratospheric balloons. The launch site is the Esrange Space Center in Kiruna. The launch campaign for BEXUS-38 is scheduled for October 2026, and the flight typically lasts about 2 to 5 hours.

»REXUS/BEXUS Student Experiment Programme«; Credit: DLR/SNSA

CLOUDS examines a specific research question

How does the presence of CaCO₃ particles alter the incident solar spectrum under stratospheric conditions—and what can be inferred from this about the scattering properties of these particles?

Conceptual diagram: SRM reflects a portion of the sun's radiation via aerosols in the stratosphere – CLOUDS measures the spectral effects. (©CLOUDS-Team)

Why is this relevant to climate change?

The Earth’s climate depends heavily on how much sunlight the atmosphere scatters back into space and how much radiation ultimately reaches the ground. Aerosols in the stratosphere can influence this radiation balance—but it is not just »how much« light is scattered or absorbed that matters, but also »at which wavelengths.« This is exactly where CLOUDS comes in: Spectral measurements reveal how calcium carbonate particles alter incoming sunlight and how strong the scattering is across different spectral ranges. Such data are crucial for improving physical models of particle-radiation interactions and for estimating effects more realistically. In addition, the experiment makes a practical contribution to atmospheric research because it demonstrates how spectroscopy can be robustly implemented as a measurement method under near-stratospheric conditions (low pressure, low temperatures, vibrations).

Why Calciumcarbonat?

The team cites calcium carbonate (CaCO₃) for its high scattering efficiency, low absorption in the thermal infrared, favorable chemical properties, and potentially longer atmospheric lifetime, among other reasons. Furthermore, different wavelengths contribute differently to warming—and CaCO₃ can behave differently depending on the wavelength. This is precisely why spectral measurements are so fascinating: they show how light changes as it passes through the particles and how strong the scattering is.

Measurement principle: Dual microspectrometer

The CLOUDS configuration includes a dual microspectrometer with a beam splitter. The specified spectral range is 350 – 850 nm, with a spectral resolution of approximately 10 nm. The dual-path approach is more than just a »nice-to-have«: A reference path can help control typical sources of interference that occur in complex setups (coupling fluctuations, drift, aging/contamination of optical components). This is an enormous advantage, especially in an experiment that must run reliably as a complete system.

Block diagram of the experiment: chamber containing CaCO₃ aerosol, sensor array, and light-tight optics leading to the dual microspectrometer (350 – 850 nm).

Caption: (1) (Dual) spectrometer • (2) Light guides / Collimator • (3) Optical filters • (4) Chamber with stratospheric conditions • (5) Camera / particle sensor • (6) Sensors • (7) Membrane • (8) Calcium carbonate (CaCO₃) • (9) Mirror • (10) Focusing lens • (11) Light-tight shielding • (12) Axicon • (13) Sunlight • (14) Fiber • (15) Beam splitter

Join in the excitement and don't miss a thing

This page is updated regularly. If you’d like to follow our progress, you can check the updates here on the website—and keep up with selected milestones on our social media channels as well.

EURECA
Eureca@LinkedInEureca@Instagram

CLOUDS
CLOUDS@LinkedInCLOUDS@Instagram


Here you can easily ask a question or inquiry about our products:

Product inquiry

Request for: