<html>
<head>
<meta http-equiv="Content-Type" content="text/html; charset=utf-8">
</head>
<body>
<div style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
*** Reminder in 1 hour ***</div>
<div style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Best,</div>
<div style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Tutku, Jesse & Luke</div>
<div style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div id="mail-editor-reference-message-container">
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr;">
</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="text-align: left; padding: 3pt 0in 0in; border-width: 1pt medium medium; border-style: solid none none; border-color: rgb(181, 196, 223) currentcolor currentcolor; font-family: Aptos; font-size: 12pt; color: black;">
<b>From: </b>Astro <astro-bounces@lists.nottingham.ac.uk> on behalf of Tutku Kolcu (staff) <Tutku.Kolcu@nottingham.ac.uk><br>
<b>Date: </b>Monday, 16 March 2026 at 11:09<br>
<b>To: </b>Nottingham Astro Group <astro@nottingham.ac.uk><br>
<b>Subject: </b>[Astro] Astronomy Seminar - 18th of March<br>
<br>
</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Dear All,</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
This week we are welcoming Lucy Oswald from University of Southampton. Please find the talk’s abstract below.</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<b></b>*****************</div>
<p class="MsoNormal" style="direction: ltr; text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);"><b>Radio pulsars: a polarized perspective</b></span></p>
<p class="MsoNormal" style="text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);"> </span></p>
<p class="MsoNormal" style="text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);">Radio pulsars are used as high precision tools to probe extremes of physics, reveal hidden galaxy structures and search for gravitational waves. However, we do not yet fully
understand the physics driving their radio emission, which is fundamental to advancing these areas of science. </span></p>
<p class="MsoNormal" style="text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);"> </span></p>
<p class="MsoNormal" style="text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);">Studying the polarimetry of pulsar radio emission provides a unique way to address this problem. In 1969, Radhakrishnan and Cooke proposed the "rotating vector model" to
explain the polarization of radio pulses from the Vela pulsar, and in doing so opened up a wealth of possibility for mapping neutron star magnetic field geometries. </span></p>
<p class="MsoNormal" style="text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);"> </span></p>
<p class="MsoNormal" style="text-align: left; text-indent: 0px; text-transform: none; margin: 0cm;">
<span style="font-family: Aptos, sans-serif; font-size: 12pt; color: rgb(33, 33, 33);">With modern telescopes we can now probe pulsar radio polarimetry with greater sensitivity and frequency resolution than ever before. In this talk, I will discuss my work
in this area in the context of polarimetric studies of radio pulsars over the last half-century, explain what pulsar polarization reveals to us about the neutron star magnetosphere, and look forward to future possibilities in our new era of broad-band polarimetry.</span></p>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<b></b>*****************</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
The Seminar will start at the usual time, <b>15:45 at Physics C4</b>, followed by the
<span style="font-family: "Apple Chancery", Arial, Helvetica, sans-serif;">Wine and Cheese
</span>in the Physics break room.</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<b><br>
</b></div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Best,</div>
<div class="ms-outlook-mobile-reference-message skipProofing" style="direction: ltr; font-family: Aptos, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Tutku, Jesse & Luke</div>
<div dir="ltr" id="ms-outlook-mobile-signature">
<p class="MsoNormal"><span style="font-family: "Aptos Light", sans-serif; font-size: 11pt; color: rgb(59, 125, 35);"><br>
</span></p>
</div>
</div>
</body>
</html>