3D cloud geometry

Dataset description

The cloud reconstruction is performed by using the images of the two polarization resolving cameras of the specMACS instrument. The algorithm is based on identifying points on the clouds surface and to re-find them in following images. As a first result, point clouds are obtained. Furthermore, a Poisson surface reconstruction is used to derive the cloud surfaces.

For each flight segment three NETCDF4 files are provided. Their ideas are briefly described in the following:

For some flight segments, an extra "mesh_flight-id.nc" file is added. This provides the results of the Poisson surface reconstruction with the original points as an input. If there is no such file, the data had to be reduced for the actual surface reconstruction. In general, the obtained surfaces should be very similar and should not lead to large differences in further computations.

Important notes and known problems:

Changes

The algorithm developed to reconstruct the clouds in three dimensional space from the specMACS data is described in the following paper: Kölling, T., Zinner, T., and Mayer, B.: Aircraft-based stereographic reconstruction of 3-D cloud geometry, Atmos. Meas. Tech., 12, 1155–1166. It can be found under this DOI. Next to the actual point clouds, the centroids were added to reduce the data to work with.

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HALO-0205

HALO-0130

Help needed?

If you have any questions concerning the provided data please feel free to contact us! This could be, e.g., by sending an e-mail to Lea Volkmer.

Literature