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Spanish Language Broadcasting Collection
Spanish Language Broadcasting Collection NMAH.AC.1404 IrMarie Fraticelli, Edwin A. Rodriguez, and Justine Thomas This collection received Federal support from the Latino Initiatives Pool, administered by the Smithsonian Latino Center. Archives Center, National Museum of American History P.O. Box 37012 Suite 1100, MRC 601 Washington, D.C. 20013-7012 [email protected] http://americanhistory.si.edu/archives Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Arrangement..................................................................................................................... 2 Biographical / Historical.................................................................................................... 2 Scope and Contents........................................................................................................ 2 Names and Subjects ...................................................................................................... 2 Container Listing ............................................................................................................. 4 Series 1: Gilda Mirós, (bulk 1950 - 2016, undated) (bulk 1950 - 2016, undated).................................................................................................................... 4 Series 2: Hector Aguilar, 1940 - 2002, undated.................................................... -
Before the FEDERAL COMMUNICATIONS COMMISSION Washington, D.C. 20554 in the Matter of Bright House Networks, LLC for Determinatio
Before the FEDERAL COMMUNICATIONS COMMISSION Washington, D.C. 20554 In the Matter of ) ) Bright House Networks, LLC ) CSRNo. _ ___ ) For Determination of Effective Competition in: ) Brevard County, FL (FL0014) ) Grant-Valkaria, FL (FL1348) To: Office of the Secretary Attn: Chief, Media Bureau PETITION FOR SPECIAL RELIEF Bright House Networks, LLC, ("Bright House Networks" or the "Company"), pursuant to Sections 76.7 and 76.907 of the Commission's rules, 1 requests that the Commission find that it faces "effective competition" in the above-referenced Florida franchise areas (the "Franchise Areas"). The Communications Act of 1934, as amended (the "Act"), and the Commission's rules provide that cable television rates may be regulated only in the absence of effective competition.2 Cable operators are entitled to demonstrate that effective competition exists on a franchise-by- franchise basis. 3 When a cable operator demonstrates that effective competition is present within a franchise area, cable rates in the affected area are no longer subject to regulation. 4 1 47 C.F.R. §§ 76.7 and 76.907. 2 47 U.S.C. § 543(a)(2); 47 C.F.R. § 76.905(a). 3 47 C.F.R. § 76.907. 4 See Implementation ofSections ofthe Cable Television Consumer Protection and Competition Act of 1992, Rate Regulation, 8 FCC Red. 5631, 5664-5665 (1993) ("Rate Order"). DWT 21 18866lvl 0102538-000001 Under the "competing provider" test set forth in Section 623(1)(l)(B) ofthe Act and Section 76.905(b)(2) of the Commission's rules (the "Competing Provider Test"), a cable system will be deemed subject to effective competition if the franchise area is: (i) served by at least two unaffiliated multichannel video programming distributors, each of which offers comparable programming to at least 50 percent of the households in the franchise area; and (ii) the number of households subscribing to multichannel video programming other than the largest multichannel video programming distributor exceeds 15 5 percent of the households in the franchise area. -
DISH Network Adds MTV S to DISH Latino Package
DISH Network Adds MTV S to DISH Latino Package LITTLETON, Colo.--(ENTERTAINMENT WIRE)--Aug. 25, 1999-- EchoStar's 20-Channel DISH Latino Package Offers the Most Comprehensive Spanish-Language Programming Package in the United States EchoStar Communications Corp. (NASDAQ: DISH, DISHP) is pleased to announce that DISH Network™ will add MTV S to DISH Latino, the most complete Spanish-language television and audio programming package ever offered in the United States. DISH Latino offers Spanish-speaking customers a variety of television and audio programming from Latin America. Already a leading provider of Spanish-language TV programming, DISH Network is proud to be the first satellite television provider to offer the fast-growing U.S. Spanish-speaking audience the most extensive selection of news, sports, movies, music and other entertainment. "For the first time ever in the U.S., Latin music programming takes center stage," Eric Sherman, Director of Operations at MTV S. "An entire generation of U.S.-born Spanish-speaking young people will find the music of their lives and their culture represented only at MTV S. But beware, this isn't their parents' music. MTV S' mix of Latin Pop and Rock en Espanol represents the newest sounds of today." "MTV S is a great addition to DISH Latino by appealing to the interests of the young Hispanic community," said Michael Schwimmer, vice president of Programming at EchoStar. "The U.S. Hispanic population is over 31 million, and growing, yet this community has been largely disregarded by a majority of television providers. DISH Latino offers 20 television channels to millions of Spanish-speaking homes." MTV S targets the unique character and voice of the American Hispanic community. -
Re-Os ISOTOPIC CONSTRAINTS on the CRYSTALLIZATION HISTORY of IIAB IRON METEORITES
Lunar and Planetary Science XXVIII 1258.PDF Re-Os ISOTOPIC CONSTRAINTS on the CRYSTALLIZATION HISTORY of IIAB IRON METEORITES. M.I. Smoliar, R.J. Walker, J.W. Morgan. Dept. of Geol., Univ. MD, College Park, MD 20742 The IIAB group represents one of the clearest cases of face bet-ween IIA and IIB subgroups [4]. It also shows an fractional crystallization of metallic magma during core intermediate struc-ture - roughly half of this 2700 kg iron is formation. The Ni-Ir trend in the IIAB group (Fig. 1) has a a single hexahedral crystal of kamasite (typical for IIA sub- very steep negative slope which indicates a correspon- group), while the other part has the coarsest octahedral dingly high Ir distribution coefficient, and, consequently, structure, very similar to Navajo and Mount Joy - the neigh- high sulfur content in the parental metallic magma [1]. Sta- bors of Old Woman from IIB subgroup [5]. Specimens from tistical analyses of the IIAB Ni-Ir trend indicates that the both octahedral and hexahedral parts of Old Woman were observed scatter of datapoints along the ideal crystalli- analyzed. zation line is mostly due to analytical uncertainty. This Fig. 2 shows the Re-Os experimental results for the IIB implies that the Ni-Ir distribution pattern in IIAB irons re- meteorites along with previously publisued IIA isochron flects fractional crystallization, with no significant parallel ([7], age = 4.537 ± 8 Ga, initial 187Os/188Os ratio = 0.09550 or subsequent processes. Originally two separate groups ± 7, MSWD = 1.15). Low age uncertainty and low MSWD were recognized (IIA and IIB) on the basis of their different value imply that the whole IIA subgroup crystallized in a crystallographic structure and the prominent hiatus in the Ir narrow time interval not exceeding 16 m.y. -
Lost Lake by Robert Verish
Meteorite-Times Magazine Contents by Editor Like Sign Up to see what your friends like. Featured Monthly Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Meteorite Market Trends by Michael Blood Bob’s Findings by Robert Verish IMCA Insights by The IMCA Team Micro Visions by John Kashuba Galactic Lore by Mike Gilmer Meteorite Calendar by Anne Black Meteorite of the Month by Michael Johnson Tektite of the Month by Editor Terms Of Use Materials contained in and linked to from this website do not necessarily reflect the views or opinions of The Meteorite Exchange, Inc., nor those of any person connected therewith. In no event shall The Meteorite Exchange, Inc. be responsible for, nor liable for, exposure to any such material in any form by any person or persons, whether written, graphic, audio or otherwise, presented on this or by any other website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. does not endorse, edit nor hold any copyright interest in any material found on any website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. shall not be held liable for any misinformation by any author, dealer and or seller. In no event will The Meteorite Exchange, Inc. be liable for any damages, including any loss of profits, lost savings, or any other commercial damage, including but not limited to special, consequential, or other damages arising out of this service. © Copyright 2002–2010 The Meteorite Exchange, Inc. All rights reserved. No reproduction of copyrighted material is allowed by any means without prior written permission of the copyright owner. -
Chemical Composition and Petrogenetic Implications of Eudialyte-Group Mineral in the Peralkaline Lovozero Complex, Kola Peninsula, Russia
minerals Article Chemical Composition and Petrogenetic Implications of Eudialyte-Group Mineral in the Peralkaline Lovozero Complex, Kola Peninsula, Russia Lia Kogarko 1,* and Troels F. D. Nielsen 2 1 Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, 119991 Moscow, Russia 2 Geological Survey of Denmark and Greenland, 1350 Copenhagen, Denmark; [email protected] * Correspondence: [email protected] Received: 23 September 2020; Accepted: 16 November 2020; Published: 20 November 2020 Abstract: Lovozero complex, the world’s largest layered peralkaline intrusive complex hosts gigantic deposits of Zr-, Hf-, Nb-, LREE-, and HREE-rich Eudialyte Group of Mineral (EGM). The petrographic relations of EGM change with time and advancing crystallization up from Phase II (differentiated complex) to Phase III (eudialyte complex). EGM is anhedral interstitial in all of Phase II which indicates that EGM nucleated late relative to the main rock-forming and liquidus minerals of Phase II. Saturation in remaining bulk melt with components needed for nucleation of EGM was reached after the crystallization about 85 vol. % of the intrusion. Early euhedral and idiomorphic EGM of Phase III crystalized in a large convective volume of melt together with other liquidus minerals and was affected by layering processes and formation of EGM ore. Consequently, a prerequisite for the formation of the ore deposit is saturation of the alkaline bulk magma with EGM. It follows that the potential for EGM ores in Lovozero is restricted to the parts of the complex that hosts cumulus EGM. Phase II with only anhedral and interstitial EGM is not promising for this type of ore. -
Foreign Satellite & Satellite Systems Europe Africa & Middle East Asia
Foreign Satellite & Satellite Systems Europe Africa & Middle East Albania, Austria, Belarus, Belgium, Bosnia & Algeria, Angola, Benin, Burkina Faso, Cameroon, Herzegonia, Bulgaria, Croatia, Czech Republic, Congo Brazzaville, Congo Kinshasa, Egypt, France, Germany, Gibraltar, Greece, Hungary, Ethiopia, Gabon, Ghana, Ivory Coast, Kenya, Iceland, Ireland, Italy, Luxembourg, Macedonia, Libya, Mali, Mauritania, Mauritius, Morocco, Moldova, Montenegro, The Netherlands, Norway, Mozambique, Namibia, Niger, Nigeria, Senegal, Poland, Portugal, Romania, Russia, Serbia, Somalia, South Africa, Sudan, Tanzania, Tunisia, Slovakia, Slovenia, Spain, Sweden, Switzerland, Uganda, Western Sahara, Zambia. Armenia, Ukraine, United Kingdom. Azerbaijan, Bahrain, Cyprus, Georgia, Iran, Iraq, Israel, Jordan, Kuwait, Lebanon, Oman, Palestine, Qatar, Saudi Arabia, Syria, Turkey, United Arab Emirates, Yemen. Asia & Pacific North & South America Afghanistan, Bangladesh, Bhutan, Cambodia, Canada, Costa Rica, Cuba, Dominican Republic, China, Hong Kong, India, Japan, Kazakhstan, Honduras, Jamaica, Mexico, Puerto Rico, United Kyrgyzstan, Laos, Macau, Maldives, Myanmar, States of America. Argentina, Bolivia, Brazil, Nepal, Pakistan, Phillipines, South Korea, Chile, Columbia, Ecuador, Paraguay, Peru, Sri Lanka, Taiwan, Tajikistan, Thailand, Uruguay, Venezuela. Uzbekistan, Vietnam. Australia, French Polynesia, New Zealand. EUROPE Albania Austria Belarus Belgium Bosnia & Herzegovina Bulgaria Croatia Czech Republic France Germany Gibraltar Greece Hungary Iceland Ireland Italy -
American Broadcasting Company from Wikipedia, the Free Encyclopedia Jump To: Navigation, Search for the Australian TV Network, See Australian Broadcasting Corporation
Scholarship applications are invited for Wiki Conference India being held from 18- <="" 20 November, 2011 in Mumbai. Apply here. Last date for application is August 15, > 2011. American Broadcasting Company From Wikipedia, the free encyclopedia Jump to: navigation, search For the Australian TV network, see Australian Broadcasting Corporation. For the Philippine TV network, see Associated Broadcasting Company. For the former British ITV contractor, see Associated British Corporation. American Broadcasting Company (ABC) Radio Network Type Television Network "America's Branding Broadcasting Company" Country United States Availability National Slogan Start Here Owner Independent (divested from NBC, 1943–1953) United Paramount Theatres (1953– 1965) Independent (1965–1985) Capital Cities Communications (1985–1996) The Walt Disney Company (1997– present) Edward Noble Robert Iger Anne Sweeney Key people David Westin Paul Lee George Bodenheimer October 12, 1943 (Radio) Launch date April 19, 1948 (Television) Former NBC Blue names Network Picture 480i (16:9 SDTV) format 720p (HDTV) Official abc.go.com Website The American Broadcasting Company (ABC) is an American commercial broadcasting television network. Created in 1943 from the former NBC Blue radio network, ABC is owned by The Walt Disney Company and is part of Disney-ABC Television Group. Its first broadcast on television was in 1948. As one of the Big Three television networks, its programming has contributed to American popular culture. Corporate headquarters is in the Upper West Side of Manhattan in New York City,[1] while programming offices are in Burbank, California adjacent to the Walt Disney Studios and the corporate headquarters of The Walt Disney Company. The formal name of the operation is American Broadcasting Companies, Inc., and that name appears on copyright notices for its in-house network productions and on all official documents of the company, including paychecks and contracts. -
Sly Fox Buys Big, Gets Back On
17apSRtop25.qxd 4/19/01 5:19 PM Page 59 COVERSTORY Sly Fox buys big, The Top 25 gets back on top Television Groups But biggest station-group would-be Spanish-language network, Azteca America. Rank Network (rank last year) gainers reflect the rapid Meanwhile, Entravision rival Telemundo growth of Spanish-speaking has made just one deal in the past year, cre- audiences across the U.S. ating a duopoly in Los Angeles. But the 1 Fox (2) company moved up several notches on the 2 Viacom (1) By Elizabeth A. Rathbun Top 25 list as Univision swallowed USA. ending the lifting of the FCC’s owner- In the biggest deal of the past year, News 3 Paxson (3) ship cap, the major changes on Corp./Fox Television made plans to take 4 Tribune (4) PBROADCASTING & CABLE’s compila- over Chris-Craft Industries/United Tele- tion of the nation’s Top 25 TV Groups reflect vision, No. 7 on last year’s list. That deal 5 NBC (5) the rapid growth of the Spanish-speaking finally seems to be headed for federal population in the U.S. approval. 6 ABC (6) The list also reflects Industry consolidation But the divestiture 7 Univision (13) the power of the Top 25 doesn’t alter that News Percent of commercial TV stations 8 Gannett (8) groups as whole: They controlled by the top 25 TV groups Corp. returns to the control 44.5% of com- top after buying Chris- 9 Hearst-Argyle (9) mercial TV stations in Craft. This year, News the U.S., up about 7% Corp. -
Meteorite Fall
Meteorite Times Magazine Contents by Editor Featured Monthly Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Meteorite Market Trends by Michael Blood Bob’s Findings by Robert Verish IMCA Insights by The IMCA Team Micro Visions by John Kashuba Norm’s Tektite Teasers by Norm Lehrman Meteorite Calendar by Anne Black Meteorite of the Month by Editor Tektite of the Month by Editor Terms Of Use Materials contained in and linked to from this website do not necessarily reflect the views or opinions of The Meteorite Exchange, Inc., nor those of any person connected therewith. In no event shall The Meteorite Exchange, Inc. be responsible for, nor liable for, exposure to any such material in any form by any person or persons, whether written, graphic, audio or otherwise, presented on this or by any other website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. does not endorse, edit nor hold any copyright interest in any material found on any website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. shall not be held liable for any misinformation by any author, dealer and or seller. In no event will The Meteorite Exchange, Inc. be liable for any damages, including any loss of profits, lost savings, or any other commercial damage, including but not limited to special, consequential, or other damages arising out of this service. © Copyright 2002–2012 The Meteorite Exchange, Inc. All rights reserved. No reproduction of copyrighted material is allowed by any means without prior written permission of the copyright owner. -
Advancing Children's Learning Through Personalized Media Experiences
CONTENT, COMMUNITY, AND COLLABORATION: ADVANCING CHILDREN'S LEARNING THROUGH PERSONALIZED MEDIA EXPERIENCES A READY TO LEARN TELEVISION GRANT PROPOSAL FROM THE CORPORATION FOR PUBLIC BROADCASTING AND THE PUBLIC BROADCASTING SERVICE I. PROJECT OVERVIEW The Corporation for Public Broadcasting (CPB) and the Public Broadcasting Service (PBS) seek a Ready To Learn Television grant (RTL) to create a groundbreaking and comprehensive media initiative that will help to close the achievement gap for young learners from low-income households and contribute meaningful practice and research to the early learning field. Forming powerful collaborations within and across organizations devoted to early learning, media, and community engagement, the Project Team will address both invitational priorities from the Department of Education, producing and delivering comprehensive multi-platform educational media experiences to improve school readiness by focusing on science and literacy learning among low-income children ages 2-8, and combining media assets into dynamic new learning adventures that use embedded analytics and assessments to personalize the learning experience for users and provide meaningful information to parents, caregivers and educators. The Project emphasizes the importance of content, community, and collaboration: the power of adaptive learning experiences, the amplifying effects of family engagement, and the critical role of partnerships to move the needle for children from America’s lowest income communities. The Project’s primary innovation -
VLASOVITE, Na2 Zr (Si4o11), from the KIPAWA ALKALINE COMPLEX, QUEBEC, CANADA: CRYSTAL-STRUCTURE REFINEMENT and INFRARED SPECTROSCOPY
1349 The Canadian Mineralogist Vol. 44, pp. 1349-1356 (2006) VLASOVITE, Na2 Zr (Si4O11), FROM THE KIPAWA ALKALINE COMPLEX, QUEBEC, CANADA: CRYSTAL-STRUCTURE REFINEMENT AND INFRARED SPECTROSCOPY ELENA SOKOLOVA§, FRANK C. HAWTHORNE AND NEIL A. BALL Department of Geological Sciences, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada ROGER H. MITCHELL Department of Geological Sciences, Lakehead University, Thunder Bay, Ontario P7B 5E1, Canada GIANCARLO DELLA VENTURA Dipartimento di Scienze Geologiche, Università Roma Tre, Largo S. Leonardo Murialdo 1, I-00146 Roma, Italy ABSTRACT The crystal structure of vlasovite, Na2 Zr (Si4O11), from the Kipawa alkaline complex, Quebec, Canada, monoclinic, a 11.0390(5), b 10.0980(3), c 8.5677(4) Å,  100.313(1)°, V 939.6(1) Å3, space group C2/c, Z = 4, D (calc.) = 3.008 g.cm–3, was refi ned to an R1 index of 1.9% based on 1352 observed [|Fo| > 4F] unique refl ections measured with MoK␣ X-radiation on a Bruker P4 diffractometer equipped with a 4K CCD detector. An electron-microprobe analysis gave the composition Na1.98 Zr1.00 (Si4O11) based on 11 O apfu. In the crystal structure, there are two tetrahedrally coordinated Si sites with a grand <Si–O> distance of 1.612 Å, and one octahedrally coordinated Zr site with <Zr–O> = 2.085 Å. There are two Na sites: the Na(1) site is [7]-coordinated with <Na(1)–O> = 2.620 Å. The Na(2) site is split into two subsites, Na(2A) and Na(2B), with a separation of 0.829 Å, and the symmetry-related Na(2B) sites are separated by 1.525 Å.