BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Stereoscopic disambiguation of vector magnetograms: first applicat ions to HRT data DTSTART;VALUE=DATE-TIME:20230509T122500Z DTEND;VALUE=DATE-TIME:20230509T124000Z DTSTAMP;VALUE=DATE-TIME:20240704T115653Z UID:indico-contribution-304@meetings.aip.de DESCRIPTION:Speakers: Gherardo Valori (MPS - Max Planck Institute for Sola r System Research)\nSpectropolarimetric reconstructions of the photospheri c vector magnetic field are intrinsically limited by the 180-degree-ambigu ity in the orientation of the transverse component. So far\, the removal of such an ambiguity has required assumptions about the properties of the photospheric field\, which makes disambiguation methods model-dependent.\n \nThe successful launch and operation of Solar Orbiter have made the remov al of the 180-ambiguity possible solely using observations of the same loc ation on the Sun obtained from two different vantage points. To that purpo se\, the Stereoscopic Disambiguation Method was recently developed and suc cessfully tested on numerical simulations.\n\nHere we present the first ap plication of the SDM to data obtained by the High Resolution Telescope (HR T) onboard Solar Orbiter during the March 2022 campaign\, when the angle w ith Earth was 27 degrees. The method is successfully applied to remove the ambiguity in the transverse component of the HRT vector magnetogram solel y using observations (from HRT and from the Helioseismic and Magnetic Imag er-HMI)\, for the first time.\n\nThe SDM is proven to provide observation- only disambiguated vector magnetograms that are spatially homogeneous and consistent.\nWhile we present here an application combining PHI with HMI d ata\, the same method can be applied to magnetic information from Solar Or biter together with any Earth-bound observatory.\n\nhttps://meetings.aip.d e/event/24/contributions/304/ LOCATION:Haus H\, Telegrafenberg URL:https://meetings.aip.de/event/24/contributions/304/ END:VEVENT END:VCALENDAR