{"id":4197,"date":"2018-01-10T23:06:37","date_gmt":"2018-01-10T19:06:37","guid":{"rendered":"http:\/\/sites.williams.edu\/kkwitter\/?page_id=4197"},"modified":"2018-02-28T23:46:09","modified_gmt":"2018-02-28T19:46:09","slug":"a402t-tutorial-week-4-atomic-processes-spectroscopic-notation","status":"publish","type":"page","link":"https:\/\/sites.williams.edu\/kkwitter\/astronomy-402-between-the-stars\/a402t-tutorial-week-4-atomic-processes-spectroscopic-notation\/","title":{"rendered":"A402T Tutorial Week #4: Atomic Processes &amp; Spectroscopic Notation"},"content":{"rendered":"<p style=\"text-align: center\"><strong>ASTRONOMY 402T &#8211; Spring 2018<br \/>\nProblems for Tutorial Week #4<\/strong><\/p>\n<p><em>For all tutorial assignments you should come to your tutorial session prepared to work quantitative problems on the board. Bring your calculator so we can review and correct any errors. Remember to leave adequate room on your submitted work for your in-class additions, and for me to write comments and corrections. Thanks!<\/em><\/p>\n<p><strong>1<\/strong>. a) What is meant by a \u201cresonance line\u201d and why are these lines relevant in ISM studies?<\/p>\n<p>b) Give examples of resonance lines observed in the ISM and include spectra (a URL is fine; we&#8217;ll look at it together in tutorial session.)<\/p>\n<p>c) What can be learned from these lines?<\/p>\n<p><strong>2.<\/strong> What is meant by an \u201cisoelectronic sequence\u201d and how is such a concept useful?<\/p>\n<p><strong>3.<\/strong> What are \u201cfine structure lines&#8221;? Explain how emission in those lines affects a nebula.<\/p>\n<p><strong>4.<\/strong> Explain the reason for neutral helium&#8217;s two families of energy levels.<\/p>\n<p><strong>5.<\/strong> a) What is \u201ctwo-photon emission,\u201d where do we see it, and why? What kind of spectrum does it produce?<\/p>\n<p><a href=\"https:\/\/sites.williams.edu\/kkwitter\/files\/2018\/02\/2-photon.png\"><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-4364\" src=\"https:\/\/sites.williams.edu\/kkwitter\/files\/2018\/02\/2-photon.png\" alt=\"\" width=\"399\" height=\"288\" srcset=\"https:\/\/sites.williams.edu\/kkwitter\/files\/2018\/02\/2-photon.png 743w, https:\/\/sites.williams.edu\/kkwitter\/files\/2018\/02\/2-photon-300x216.png 300w\" sizes=\"auto, (max-width: 399px) 100vw, 399px\" \/><\/a><\/p>\n<p><a href=\"https:\/\/sites.williams.edu\/kkwitter\/files\/2018\/02\/img36.gif\"><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-4368\" src=\"https:\/\/sites.williams.edu\/kkwitter\/files\/2018\/02\/img36.gif\" alt=\"\" width=\"363\" height=\"317\" \/><\/a><\/p>\n<p>Above (top) is the graph of the two-photon emission spectrum from the class PowerPoint, which plots the flux (in frequency units) vs. wavelength. \u00a0Above (bottom) is the graph of the probability of emitting a photon at any particular frequency, given in units of \u03bd<sub>0<\/sub>, the frequency of Lyman \u03b1. (Ignore the dashed lines.)<\/p>\n<p>b) Why are these graphs different, aside from the obvious fact that one plots wavelength and one plots frequency. Explain why each has the shape it does.<\/p>\n<p><strong>6.<\/strong> What do we mean by a \u201cforbidden\u201d transition? Explain, quantitatively, \u00a0how it differs from an ordinary, \u201cpermitted\u201d transition.<\/p>\n<p><strong>7.<\/strong> a) Draw a Grotrian diagram of the 5 lowest energy levels in a doubly ionized oxygen atom (O<sup>++<\/sup>). Label each level with its spectroscopic notation, and be ready to explain it. Also include the wavelengths of photons making transitions between pairs of these levels.<\/p>\n<p>b) Do the same for singly ionized oxygen (O<sup>+<\/sup>).<\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>ASTRONOMY 402T &#8211; Spring 2018 Problems for Tutorial Week #4 For all tutorial assignments you should come to your tutorial session prepared to work quantitative problems on the board. Bring your calculator so we can review and correct any errors. Remember to leave adequate room on your submitted work for your in-class additions, and for [&hellip;]<\/p>\n","protected":false},"author":198,"featured_media":0,"parent":793,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-4197","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/pages\/4197","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/users\/198"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/comments?post=4197"}],"version-history":[{"count":18,"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/pages\/4197\/revisions"}],"predecessor-version":[{"id":4389,"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/pages\/4197\/revisions\/4389"}],"up":[{"embeddable":true,"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/pages\/793"}],"wp:attachment":[{"href":"https:\/\/sites.williams.edu\/kkwitter\/wp-json\/wp\/v2\/media?parent=4197"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}