The Use of Digital Audio Workstations and the Impact on Music

Author(s):  
Julian Ashbourn
Keyword(s):  
1999 ◽  
Vol 91 (1) ◽  
pp. 33-42 ◽  
Author(s):  
David B. Soothill

The Asia-Pacific is the world's largest region and it has a huge range of potential radio uses that analogue terrestrial broadcasting simply cannot meet. This article explores the impact that digital radio transmission will have on the region, and the importance of satellite broadcasting and multichannel broadcasting for better coverage and quality of services.


2017 ◽  
Vol 11 (2) ◽  
pp. 64-75
Author(s):  
Laura Uglean Jackson ◽  
Matthew McKinley

In October 2014, the University of California Irvine (UCI) Special Collections and Archives acquired a born digital collection of 2.5 terabytes – the largest born digital collection acquired by the department to date. This case study describes the challenges we encountered when applying existing archival procedures to appraise, store, and provide access to a large born digital collection. It discusses solutions when they could be found and ideas for solutions when they could not, lessons learned from the experience, and the impact on born-digital policy and procedure at UCI Libraries. Working with a team of archivists, librarians, IT, and California Digital Library (CDL) staff, we discovered issues and determined solutions that will guide our procedures for future acquisitions of large and unwieldy born digital collections. 


2015 ◽  
Vol 13 ◽  
pp. 181-188
Author(s):  
F. Pfeiffer ◽  
M. Rashwan ◽  
E. Biebl ◽  
B. Napholz

Abstract. Nowadays, customers expect to integrate their mobile electronic devices (smartphones and laptops) in a vehicle to form a wireless network. Typically, IEEE 802.11 is used to provide a high-speed wireless local area network (WLAN) and Bluetooth is used for cable replacement applications in a wireless personal area network (PAN). In addition, Daimler uses KLEER as third wireless technology in the unlicensed (UL) 2.4 GHz-ISM-band to transmit full CD-quality digital audio. As Bluetooth, IEEE 802.11 and KLEER are operating in the same frequency band, it has to be ensured that all three technologies can be used simultaneously without interference. In this paper, we focus on the impact of Bluetooth and IEEE 802.11 as interferer in presence of a KLEER audio transmission.


Author(s):  
Ofirenty Elyada Nubatonis

The problem faced by teachers in East Nusa Tenggara is the limited use of technology in producing instructional media or digital audio-visual teaching materials. The impact of this limitation was most felt during the Covid-19 pandemic, online learning did not work effectively. Finally, the Network learning process is carried out which happens to the extent that the teacher sends the assignment and the students do the given assignment and then sent it back via the messenger application. When the teacher sends teaching materials in the form of instructional videos to explain certain concepts, most of the videos are taken from the internet and are not written by themselves. Therefore, it is necessary to hold training in making learning videos using applications that are easy to master, do not require money, and simply use a laptop. In this activity, teachers are provided with the knowledge and practice of making instructional videos using the Bandicam and Screencast O-Matic applications. The form of this activity is online training. The methods used are seminars, lectures, discussions, and mentoring. The results of this activity were 1) increased teacher knowledge about the use of the Bandicam and Screencast O-Matic applications in making instructional videos, 2) teachers were able to develop instructional videos using Bandicam and Screencast O-Matic


1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


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