| _version_ | 1866902269883056128 |
|---|---|
| author | Vadim Uritsky |
| author_facet | Vadim Uritsky |
| contents | <p>The Quasi-Radial Field-line Tracing (QRaFT) image segmentation package enables a detection of solar coronal features indicating the orientation of the steady-state open magnetic field. The methodology has been tested using synthetic coronagraph images generated by a three-dimensional magnetohydrodynamic (MHD) model, as well as STEREO/COR1, MLSO/K-cor, and ground-based eclipse coronal images. The MHD tests show that the extracted optical features are typically aligned within ~4−7 degrees with the local magnetic field.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_16970789 |
| institution | Zenodo |
| language | |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | QRaFT: The Quasi-Radial Field-line Tracing image analysis package Vadim Uritsky <p>The Quasi-Radial Field-line Tracing (QRaFT) image segmentation package enables a detection of solar coronal features indicating the orientation of the steady-state open magnetic field. The methodology has been tested using synthetic coronagraph images generated by a three-dimensional magnetohydrodynamic (MHD) model, as well as STEREO/COR1, MLSO/K-cor, and ground-based eclipse coronal images. The MHD tests show that the extracted optical features are typically aligned within ~4−7 degrees with the local magnetic field.</p> |
| title | QRaFT: The Quasi-Radial Field-line Tracing image analysis package |
| url | https://doi.org/10.5281/zenodo.16970789 |