the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Light scattering and microphysical properties of atmospheric bullet rosette ice crystals
Abstract. Cirrus clouds play a critical role in the Earth's radiative budget. The extent of the radiative impact of cirrus clouds is determined by a number of their physical properties, such as aspherical ice crystal composition. One of the most relevant cirrus ice crystal habits is a polycrystalline bullet rosette, where individual bullets are radiating from the same nucleation point. Here, the link between the crystal morphology of atmospheric bullet rosettes and their asymmetry parameter (g) is experimentally investigated using correlated high resolution in situ stereo-images of individual rosettes and their angular scattering functions measured by the airborne Particle Habit Imaging and Polar Scattering (PHIPS) cloud probe. Bullet rosette stereo-images are analyzed for their microphysical properties, including maximum dimension, bullet aspect ratio, number of bullets, projected area, bullet hollowness, derived mass, derived effective density and derived terminal velocity, as well as their optical properties such as g and optical complexity parameter. Results indicate that much lower g values represent real atmospheric bullet rosette crystals than what is expected by numerical calculations assuming solid or hollow bullets with smooth idealized surfaces, indicating higher levels of crystal complexity than have been previously incorporated within bullet rosette ray-tracing models.
Competing interests: Martin Schnaiter and Emma Järvinen are members of schnaiTEC GmbH, the PHIPS manufacturer. Martin Schnaiter is employed part-time by schnaiTEC GmbH.
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.-
Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
-
Preprint
(9088 KB)
-
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(9088 KB) - Metadata XML
- BibTeX
- EndNote
- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
- RC1: 'Comment on egusphere-2024-3316', Anonymous Referee #1, 18 Dec 2024
-
RC2: 'Comment on egusphere-2024-3316', Anonymous Referee #2, 02 Jan 2025
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3316/egusphere-2024-3316-RC2-supplement.pdf
- AC1: 'Comment on egusphere-2024-3316', Shawn Wagner, 08 Apr 2025
Interactive discussion
Status: closed
- RC1: 'Comment on egusphere-2024-3316', Anonymous Referee #1, 18 Dec 2024
-
RC2: 'Comment on egusphere-2024-3316', Anonymous Referee #2, 02 Jan 2025
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3316/egusphere-2024-3316-RC2-supplement.pdf
- AC1: 'Comment on egusphere-2024-3316', Shawn Wagner, 08 Apr 2025
Peer review completion


Journal article(s) based on this preprint
Viewed
HTML | XML | Total | BibTeX | EndNote | |
---|---|---|---|---|---|
320 | 87 | 193 | 600 | 19 | 38 |
- HTML: 320
- PDF: 87
- XML: 193
- Total: 600
- BibTeX: 19
- EndNote: 38
Viewed (geographical distribution)
Country | # | Views | % |
---|
Total: | 0 |
HTML: | 0 |
PDF: | 0 |
XML: | 0 |
- 1
Shawn Wendell Wagner
Martin Schnaiter
Guanglang Xu
Franziska Nehlert
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(9088 KB) - Metadata XML