NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
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musical properties like pitch <strong>and</strong> biological parameters. such as the percent of muscle usage. This study explores the reliability<br />
of EMG in quantifying the activities of Rectus Abdominis, two muscles essential to respiration during singing. Such a<br />
quantitative method is desired by practitioners for identifying one s innate singing abilities, or talent. This study also proposes<br />
a method of quantitatively identifying efficient pedagogy by comparing pre-training <strong>and</strong> post-training EMG. Our goals were<br />
to validate the method <strong>and</strong> to provide reliable criticisms for analysis of strengths <strong>and</strong> weaknesses in singing. A NORAXON<br />
wireless EMG was used to measure the muscle activities of a female voice professor as she sang the notes F3 (low pitch), F,<br />
(medium pitch) <strong>and</strong> F5 (high pitch). The results showed a non-linear, but noteworthy <strong>and</strong> consistent increase in muscle<br />
activity. as the pitches became higher. They confirmed our hypothesis that EMG can be used as a quantitative assessment of<br />
singing <strong>and</strong> showed that there exists a reliable connection between the level of muscle activity <strong>and</strong> musical pitch. Most<br />
importantly, this study showed that EMG has the potential for better teaching method <strong>and</strong> could increase the reliability of<br />
talent searches in singing.<br />
Author<br />
Activity (Biology); Electromyography; Muscular Function; Hypotheses; Acoustics; Audio Frequencies<br />
72<br />
ATOMIC AND MOLECULAR PHYSICS<br />
Includes atomic <strong>and</strong> molecular structure, electron properties, <strong>and</strong> atomic <strong>and</strong> molecular spectra. For elementary particle physics see 73<br />
Nuclear Physics.<br />
20060001801 California Univ., Santa Barbara, CA USA<br />
Biological Sensing with Terahertz Circular Dichroism Spectroscopy<br />
Plaxco, Kevin W.; Allen, S. J.; May 31, 2005; 18 pp.; In English; Original contains color illustrations<br />
Contract(s)/Grant(s): DAAD19-02-1-0080<br />
Report No.(s): AD-A440274; ARO-42628-EL.2.00; No Copyright; Avail.: Defense <strong>Technical</strong> Information Center (DTIC)<br />
We have developed a circular dichroism spectrometer working in the terahertz (THz) frequency regime. As THz<br />
spectroscopy is specific to collective vibrational modes in macromolecules (<strong>and</strong> collective modes in condensed, polar media<br />
such as water), the spectrometer should provide spectral fingerprints of biological materials. Moreover, by focusing on circular<br />
dichroism the spectrometer should provide fingerprints of these materials uncontaminated by the strong background<br />
absorbance of water <strong>and</strong> other polar materials. We have built this spectrometer <strong>and</strong> have pushed its signal to noise down to<br />
1 part in 10^4. While this is more than sufficient to detect the strong circular dichroism of macroscopic, chiral objects, it is<br />
apparently insufficient to observe circular dichroism arising from common biological materials. Current efforts are aimed at<br />
1-2 orders of magnitude improvements on this detection limit.<br />
DTIC<br />
Detection; Dichroism; Spectroscopy; Warfare<br />
74<br />
OPTICS<br />
Includes light phenomena <strong>and</strong> the theory of optical devices; for specific optical devices see also 35 Instrumentation <strong>and</strong> Photography.<br />
For lasers see 36 Lasers <strong>and</strong> Masers.<br />
20060000072 Gemini Observatory, Hilo, HI, USA<br />
ALTAIR Upgrades Report<br />
Rignaut, Francois; Gemini Focus: Newsletter of the Gemini Observatory; December 2005, pp. 61-63; In English; See also<br />
20060000060; Copyright; Avail.: Other Sources<br />
There has been a flurry of activity on <strong>and</strong> around the ALTAIR adaptive optics (AO) system during 2005A. First <strong>and</strong><br />
foremost, we have been commissioning the laser <strong>and</strong> launch systems (described on page 34 of the June 2005 issue of<br />
GeminiFocus), <strong>and</strong> upgraded ALTAIR to work in Laser Guide Star (LGS) mode. This effort continued into 2005B with two<br />
runs, in August <strong>and</strong> September. ALTAIR’S upgrade included a tip-tilt/focus wavefront sensor system, designed at the Herzberg<br />
Institute of Astrophysics (HIA) in Canada, <strong>and</strong> installed by Gemini personnel. All of the work to date has concentrated on<br />
commissioning the many new functions necessary for LGS AO. We have proven that we can efficiently acquire both the laser<br />
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