tmp tp57543bbf_555e_4b1b_ab37_f8e035b7f7c0.ps - Stellar astronomy - Document - PDFSEARCH.IO

First Page		Document Content
Date: 2015-04-23 09:36:54 Spectroscopy Radio astronomy Stellar astronomy Astrophysics Black-body radiation Special sensor microwave/imager Cosmic microwave background radiation Star Zeeman effect Physics Electromagnetic radiation Radiometry		/tmp/tp57543bbf_555e_4b1b_ab37_f8e035b7f7c0.ps Add to Reading List Source URL: www.atmos-meas-tech-discuss.net Download Document from Source Website File Size: 2,36 MB Share Document on Facebook

	Final Exam (221A), due Dec 15, 4pm 1. The sodium D-lines are two separate emission lines for 3p → 3s transitions. In a weak magnetic field, consider the Zeeman effect and discuss quantitatively (a) how the 3s and 3p le DocID: 1llDm - View Document
	1 final.nb Final 1. Zeeman effect DocID: 1krAv - View Document
	/tmp/tp57543bbf_555e_4b1b_ab37_f8e035b7f7c0.ps DocID: 1aJon - View Document
	PHYSICAL REVIEW B VOLUME 61, NUMBER 21 1 JUNE 2000-I DocID: 18O04 - View Document
	PHYSICAL REVIEW A VOLUME 58, NUMBER 3 SEPTEMBER 1998 DocID: 17YY1 - View Document