Our ultimate aims are to reconstruct the HRT data by deconvolving with the HRT point spread function (PSF) and to correct for the. Future observations by using space-and ground-based coordinated data, such as those from the PHI instrument (Solanki et al.
More details about the meeting like structure, venue (for on-site participants), on-line participation, registration, and abstract submission can be found in the meeting Web pages. Polarimetric and Helioseismic Imager (PHI) on board the Solar Orbiter mission. The Solar Orbiter ( SolO) 8 is a Sun -observing satellite developed by the European Space Agency (ESA).Aims: We use wavefront sensing to characterise the image quality of the High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager (SO/PHI) data products during the second remote sensing window of the Solar Orbiter (SO) nominal mission phase.
The (hybrid) meeting will be held in Granada (Spain) and on-line on the 26th and 27th of January, 2022. The flyby captured the closest images ever taken of the Sun.
The meeting is especially aimed at researchers who want to do science with SO/PHI data from the first science orbit, in particular if they want to receive the data before the end of the embargo period. 9, 2020, Solar Orbiter turned on all 10 of its instruments together for the first time in mid-June as it made its first close pass of the Sun.
The focus of the meeting will be on describing SO/PHI and on bringing to the attention of the community the many topics that can be addressed with the help of the instrument either stand-alone or together with other instruments on Solar Orbiter or elsewhere (ground-based, Earth-orbit, etc.). PHI is a diffraction limited, wavelength tunable, quasi-monochromatic. Identifying projects for collaboration between the SO/PHI team and colleagues in general is the main goal of this meeting. Polarimetric and Helioseismic Imager (PHI) on board the Solar Orbiter mission. We would like to invite the broad scientific community to a SO/PHI science meeting dealing with the first science orbit of Solar Orbiter. Aims: We use wavefront sensing to characterise the image quality of the High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager (SO/PHI) data products during the second remote sensing window of the Solar Orbiter (SO) nominal mission phase.
0 kommentar(er)
