WSIA organized the first parasail operators symposium in January 2011, numerous parasail operators attended, along with various members of the US Coast Guard, FAA and NOAA.

The WSIA has played a major role in developing the ASTM best practices for weather standards for parasailing.

At the 2012 WSIA Summit in Snow board of directors meeting the creation of a parasail committee chaired by Daytona Beach Parasail's president, Matthew Dvorak was created.

Initial work was produced through the joint efforts of the Web Services for Interactive Applications ( WSIA ) and Web Services for Remote Portlets ( WSRP ) OASIS Technical Committees.

The religious quest is often intense and deep, and there are students on every campus who are seriously wrestling with the most profound questions of meaning and value.

A low-power, `` carrier-current '' broadcasting station, KARL, heard only in the campus dormitories, is owned and operated by the students to provide an outlet for student dramatic, musical, literary, technical, and other talents, and to furnish information, music, and entertainment for campus listeners.

A president is frequently besieged to serve in non-academic civic and governmental capacities, to make speeches to lay groups, and to make numerous ceremonial appearances on and off campus.

Surrounded by ancient elms, the campus is spacious and beautiful.

In itself there is nothing wrong with this form of `` participation '': the only difficulty on the Catholic campus is that those faculty members who are in a position to implement policy, i.e., members of the religious community which owns and administers the institution, have their own eating arrangements.

The AFI Digital Content Lab is a research and development facility for digital media located on the LA campus.

Since 2007, the Kelheim Berufsschule has had a campus in Abensberg, and outside the state sector is the St. Francis Vocational Training Centre, run by a Catholic youth organisation.

It is located on the campus of the University of Houston.

One of the more substantial collections of Aldine Press books and Aldine imitations in North America is at the Harold B. Lee library on the campus of Brigham Young University in Provo, Utah.

ASU Online is headquartered at ASU's Skysong campus in Scottsdale, Arizona.

ASU's faculty and students are served by two dedicated general-topic libraries: Hayden Library, which is the largest of the ASU libraries and is located on the Tempe campus, and Fletcher Library, located on the west campus.

@ west news is an independent, student-run newspaper covering news and events on ASU's west campus.

The purpose of RHA is to enhance the quality of residence hall life and provide a cohesive voice for the residents by addressing the concerns of the on-campus populations to university administrators and other campus organizations ; providing cultural, diversity, educational, and social programming ; establishing and working with individual hall councils.

The Sir Alexander Fleming Building on the South Kensington campus was opened in 1998 and is now one of the main preclinical teaching sites of the Imperial College School of Medicine.

There are also two religious university campuses in Canberra: Signadou is a campus of the Australian Catholic University and St Mark's Theological College is a campus of Charles Sturt University.

ADFA teaches military undergraduates and postgraduates and is officially a campus of the University of New South Wales while Duntroon provides Australian Army Officer training.

There is a sophisticated security system with highly sensitive motion detectors, remote cameras, and the latest in card readers and key pad security locks bind the campus.

Years ago this was true, but with the replacement of wires or runners by radio and radar ( and perhaps television ), these restrictions have disappeared and now again too much is heard.

A Philadelphia distiller is currently breaching the customary prohibition against hard-liquor advertising on TV and radio.

High sensitivity in radio telescopes is achieved by reducing the bandwidth of the receiver ; ;

therefore, only with precise foreknowledge of the line frequencies is an astronomical search for the radio spectra of these molecules feasible.

As soon as the shelter is completed a radio reception check must be made.

A battery-powered radio is essential.

This is a phenomenon familiar to all radio listeners, resulting from reflection of skywave signals at night from the ionized layer in the upper atmosphere known as the ionosphere.

The rules and policies to be applied in this process of course must be based on objectives which represent what is to be desired if radio service is to be of maximum use to the Nation.

`` It is as though '', I said on the historic three-hour, coast-to-coast radio broadcast which I bought ( following Father Coughlin and pre-empting the Eddie Cantor, Manhattan Merry-go-round and Major Bowes shows ) `` That Man in the White House, like some despot of yore, insisted on reading my diary, raiding my larder and ransacking my lingerie!!

The observed intensity of the radio emission of Venus is much higher than the expected thermal intensity, although the spectrum indicated by measurements at wave lengths near 3 cm and 10 cm is like that of a black body at about 600-degrees.

For the case of Jupiter, the radio emission spectrum is definitely not like the spectrum of a black-body radiator, and it seems very likely that the radiation reaching the earth is a combination of thermal radiation from the atmosphere and non-thermal components.

Of the remaining planets, only Mars and Saturn have been observed as radio sources, and not very much information is available.

No attempts to measure the radio emission of the remaining planets have been reported, and, because of their distances, small diameters, or low temperatures, the thermal radiation at radio wave lengths reaching the earth from these sources is expected to be of very low intensity.

and that the maximum of the radio emission came about 3-1/2 days after Full Moon, which is again in contrast to the infrared emission, which reaches its maximum at Full Moon.

The infrared emission could then be assumed to originate at the surface of the moon, while the radio emission originates at some depth beneath the surface, where the temperature variation due to solar radiation is reduced in amplitude and shifted in phase.

This is much smaller than the highest resolution of even the very large reflectors now under construction, and consequently the radio emission of different regions of the disk cannot be resolved.

Other than this very significant result, most of the information now available about the radio emission of the planets is restricted to the intensity of the radiation.

The radio radiation of the sun which is reflected from the moon and planets should be negligible compared with their thermal emission at centimeter wave lengths, except possibly at times of exceptional outbursts of solar radio noise.

We know that the number of radio and television impulses, sound waves, ultra-violet rays, etc., that may occupy the very same space, each solitary upon its own frequency, is infinite.

Whatever the long-range impact of integration, the owners of Negro-appeal radio stations these days know they have an audience and that it is loyal.