Stephens, IanIanStephensLi, Zhi-YunZhi-YunLiYang, HaifengHaifengYangKataoka, AkimasaAkimasaKataokaLooney, LeslieLeslieLooneyHull, CharlesCharlesHullFernández-López, ManuelManuelFernández-LópezSadavoy, SarahSarahSadavoyKwon, WoojinWoojinKwonOhashi, SatoshiSatoshiOhashiTazaki, RyoRyoTazakiLi, DanDanLiHoang, ThiemThiemHoangBertrang, Gesa H. -M.Gesa H. -M.BertrangCarrasco-González, CarlosCarlosCarrasco-GonzálezDent, WilliamWilliamDentTakahashi, SatokoSatokoTakahashiBACCIOTTI, FrancescaFrancescaBACCIOTTIAlves, Felipe O.Felipe O.AlvesGirart, Josep M.Josep M.GirartZhang, QizhouQizhouZhangRao, RamprasadRamprasadRaoPohl, AdrianaAdrianaPohlPadovani, MarcoMarcoPadovaniGALLI, DanieleDanieleGALLILee, Chin-FeiChin-FeiLeeSegura-Cox, DominiqueDominiqueSegura-Cox2021-02-262021-02-2620192330-9458http://hdl.handle.net/20.500.12386/30663This white paper discusses how disk polarization observations can be used to study disk and grain properties during the planet formation process. Such studies require very sensitive and high resolution multi-wavelength observations.ELETTRONICOenArticlehttps://arxiv.org/pdf/1903.05478.pdfhttps://baas.aas.org/pub/2020n3i246/release/12019BAAS...51c.246SFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering