<html><head><meta http-equiv="Content-Type" content="text/html; charset=utf-8"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; line-break: after-white-space;">Poštovane kolegice i kolege,<br class=""><br class="">pozivam Vas na IRBov seminar:<br class=""><br class=""><span class="Apple-tab-span" style="white-space:pre"> </span>“Magnetsko polje Mlijecne staze”<br class=""><br class=""><span class="Apple-tab-span" style="white-space:pre"> </span>prof. dr.sc. Marijke Haverkorn<br class=""><span class="Apple-tab-span" style="white-space:pre"> </span>(Radboud University Nijmegen, Nizozemska)<br class=""><br class="">koji ce se odrzati u srijedu (4. rujna 2019.) u 14:15 u predavaonici u I. krilu (IRB, Bijenicka c. 54, Zagreb).<br class=""><br class="">*******************<br class="">Dear colleagues,<br class=""><br class="">We are pleased to invite you to the RBI seminar:<br class=""><br class=""><span class="Apple-tab-span" style="white-space:pre"> </span>“The Magnetic Field of the Milky Way”<br class=""><br class=""><span class="Apple-tab-span" style="white-space:pre"> </span>prof. dr.sc. Marijke Haverkorn<br class=""><span class="Apple-tab-span" style="white-space:pre"> </span>(Radboud University Nijmegen, The Netherlands)<br class=""><br class="">on Wednesday (Sep 4, 2019) at 14:15 in I Wing Lecture Hall (RBI, Bijenicka c. 54, Zagreb).<br class=""><br class="">*******************<br class=""><br class="">Title: The Magnetic Field of the Milky Way<br class=""><br class="">Abstract:<br class="">The Milky Way's magnetic field has coherent structures on Galactic scales, following spiral arms, <br class="">but also Galactic outflows. It has a turbulent component as well which influences the galactic <br class="">ecosystem in many ways, such as delaying star formation, isotropizing Galactic cosmic rays, <br class="">and providing a significant pressure component.<br class=""><br class="">These magnetic field components can only be detected indirectly, through the signature <br class="">they leave on various kinds of radiation and particles, observations of which are fitted to <br class="">models of the Galactic magnetic field. Traditionally, radio polarimetry is most used to probe <br class="">Galactic magnetic fields, with radio detectors in frequency ranges from LOFAR to Planck <br class="">giving unique information.<br class=""><br class="">I will discuss some of the recent progress in this field, and our new project called IMAGINE, <br class="">which aims to combine all different observational tracers and prior information to build a <br class="">next-generation model of the Galactic magnetic field. <br class=""><br class=""><img apple-inline="yes" id="BC6027F1-15F9-43A1-8C28-C7C40C6DA77F" class="" src="cid:62338F88-8049-4713-9E63-7AF9230D207A@zef.irb.hr"><br class=""><br class=""><br class=""><br class=""><div class="">--<br class="">----------------------------------------------------------------------------<br class="">Vibor Jelić<br class=""><br class="">Ruđer Bošković Institute<br class="">Division of Experimental Physics<br class="">Laboratory for astroparticle physics and astrophysics<br class=""><br class="">Bijenička cesta 54<span class="Apple-tab-span" style="white-space:pre"> </span><span class="Apple-tab-span" style="white-space:pre"> </span><span class="Apple-tab-span" style="white-space:pre"> </span>Phone: +385 1 4571 378<br class="">10 000 Zagreb, Croatia<span class="Apple-tab-span" style="white-space:pre"> </span> Fax: +385 1 4680 239<span class="Apple-tab-span" style="white-space:pre"> </span><br class=""><br class="">Also affiliated with ASTRON <br class="">- Netherlands Institute for Radio Astronomy<br class="">----------------------------------------------------------------------------</div><br class=""></body></html>