Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revision
Previous revision
science:publications:tao [2026/10/14 16:23] – [Publications on THEMIS Adaptive Optics] etiennescience:publications:tao [2026/10/14 16:24] (current) – [Publications on the THEMIS Adaptive Optics] etienne
Line 2: Line 2:
 <html><font color="#ff0000" size="2.5"> Page in construction ; Last Update December 2024</font></html> <html><font color="#ff0000" size="2.5"> Page in construction ; Last Update December 2024</font></html>
  
-====== Publications on THEMIS Adaptive Optics ===== +====== Publications on the THEMIS Adaptive Optics (TAO) =====
  
   * Tallon M., Thiébaut É., Langlois M., Gelly B., Douet R., Béchet C., Denis L., Moretto G.; //[[ https://ui.adsabs.harvard.edu/abs/2021arXiv210102892T | The wavefront sensing making-of for THEMIS solar telescope]]//; arXiv e-prints, arXiv:2101.02892, (2021).  DOI:10.48550/arXiv.2101.02892 \\    * Tallon M., Thiébaut É., Langlois M., Gelly B., Douet R., Béchet C., Denis L., Moretto G.; //[[ https://ui.adsabs.harvard.edu/abs/2021arXiv210102892T | The wavefront sensing making-of for THEMIS solar telescope]]//; arXiv e-prints, arXiv:2101.02892, (2021).  DOI:10.48550/arXiv.2101.02892 \\ 
   * Tallon M., Thiébaut É., Tallon-Bosc I., Gelly B., Denis L.; //[[ https://ui.adsabs.harvard.edu/abs/2022SPIE12185E..2JT | Solar wavefront sensing at THEMIS with self-calibrated reference image and estimation of the noise covariance]]//; Proceedings of the SPIE, Vol. 12185, 121852J (2022).  DOI:10.1117/12.2630379 \\    * Tallon M., Thiébaut É., Tallon-Bosc I., Gelly B., Denis L.; //[[ https://ui.adsabs.harvard.edu/abs/2022SPIE12185E..2JT | Solar wavefront sensing at THEMIS with self-calibrated reference image and estimation of the noise covariance]]//; Proceedings of the SPIE, Vol. 12185, 121852J (2022).  DOI:10.1117/12.2630379 \\ 
   *  Thiébaut É., Tallon M., Tallon-Bosc I, Gelly B., Douet R., Langlois M., ; Moretto G.; //[[ https://ui.adsabs.harvard.edu/abs/2022SPIE12185E..2JT | Closing the loop as an inverse problem: the real-time control of Themis adaptive optics]]//; Proceedings of the SPIE, Vol. 12185, 1218507 (2022). doi:10.1117/12.2630497 \\     *  Thiébaut É., Tallon M., Tallon-Bosc I, Gelly B., Douet R., Langlois M., ; Moretto G.; //[[ https://ui.adsabs.harvard.edu/abs/2022SPIE12185E..2JT | Closing the loop as an inverse problem: the real-time control of Themis adaptive optics]]//; Proceedings of the SPIE, Vol. 12185, 1218507 (2022). doi:10.1117/12.2630497 \\  
-  * Béchet C., Thiébaut É., Tallon M., Tallon-Bosc I., Gelly B., Douet R.; ; //[[https:doi.org/10.1117/12.3104993 | Self-calibration of an adaptive optics system and its application to THEMIS solar telescope ]]// ; Proceedings of the SPIE, Volume 14150, 141502N, 10 pp. (2026); doi:10.1117/12.3104993 \\+  * Béchet C., Thiébaut É., Tallon M., Tallon-Bosc I., Gelly B., Douet R.; //[[ https://doi.org/10.1117/12.3104993 | Self-calibration of an adaptive optics system and its application to THEMIS solar telescope ]]// ; Proceedings of the SPIE, Volume 14150, 141502N, 10 pp. (2026); doi:10.1117/12.3104993 \\
  
  
  
science/publications/tao.1791995005.txt.gz · Last modified: by etienne
Recent changes RSS feed Debian Powered by PHP Valid XHTML 1.0 Valid CSS Driven by DokuWiki