| LDR | | 00000nmm u2200205 4500 |
| 001 | | 000000332723 |
| 005 | | 20241205113008 |
| 008 | | 181129s2018 ||| | | | eng d |
| 020 | |
▼a 9780355939958 |
| 035 | |
▼a (MiAaPQ)AAI10810743 |
| 035 | |
▼a (MiAaPQ)asu:17961 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 049 | 1 |
▼f DP |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Davis, Kristina. |
| 245 | 10 |
▼a Instrument Design and Radiation Pattern Testing for Terahertz Astronomical Instruments. |
| 260 | |
▼a [S.l.] :
▼b Arizona State University.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 155 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B. |
| 500 | |
▼a Adviser: Christopher E. Groppi. |
| 502 | 1 |
▼a Thesis (Ph.D.)--Arizona State University, 2018. |
| 520 | |
▼a The Milky Way galaxy is a powerful dynamic system that is highly efficient at recycling material. Stars are born out of intergalactic gas and dust, fuse light elements into heavier elements in their cores, then upon stellar death spread material |
| 520 | |
▼a I begin this work with a description of radiation pattern measurements and their use in astronomical instrument characterization. I will introduce a novel technique to measure complex (phase-sensitive) field patterns using direct detectors. I su |
| 590 | |
▼a School code: 0010. |
| 650 | 4 |
▼a Astrophysics. |
| 650 | 4 |
▼a Electrical engineering. |
| 650 | 4 |
▼a Optics. |
| 690 | |
▼a 0596 |
| 690 | |
▼a 0544 |
| 690 | |
▼a 0752 |
| 710 | 20 |
▼a Arizona State University.
▼b Exploration Systems Design. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-10B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0010 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14997956
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자
▼b 관리자 |