FT3DR/FT3DE Operating Manual
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Tr-Sas-076-All
NORTH ATLANTIC TREATY RESEARCH AND TECHNOLOGY ORGANISATION ORGANISATION AC/323(SAS-076)TP/430 www.rto.nato.int RTO TECHNICAL REPORT TR-SAS-076 NATO Independent Cost Estimating and the Role of Life Cycle Cost Analysis in Managing the Defence Enterprise (Estimation indépendante des coûts de l’OTAN et rôle de l’analyse des coûts globaux de possession au sein de l’OTAN) This Report presents the findings of Task Group SAS-076. Published August 2012 Distribution and Availability on Back Cover NORTH ATLANTIC TREATY RESEARCH AND TECHNOLOGY ORGANISATION ORGANISATION AC/323(SAS-076)TP/430 www.rto.nato.int RTO TECHNICAL REPORT TR-SAS-076 NATO Independent Cost Estimating and the Role of Life Cycle Cost Analysis in Managing the Defence Enterprise (Estimation indépendante des coûts de l’OTAN et rôle de l’analyse des coûts globaux de possession au sein de l’OTAN) This Report presents the findings of Task Group SAS-076. The Research and Technology Organisation (RTO) of NATO RTO is the single focus in NATO for Defence Research and Technology activities. Its mission is to conduct and promote co-operative research and information exchange. The objective is to support the development and effective use of national defence research and technology and to meet the military needs of the Alliance, to maintain a technological lead, and to provide advice to NATO and national decision makers. The RTO performs its mission with the support of an extensive network of national experts. It also ensures effective co-ordination with other NATO bodies involved in R&T activities. RTO reports both to the Military Committee of NATO and to the Conference of National Armament Directors. -
Optical – Near-Infrared Catalog for the AKARI North Ecliptic Pole Deep field
A&A 566, A60 (2014) Astronomy DOI: 10.1051/0004-6361/201322561 & c ESO 2014 Astrophysics Optical – near-infrared catalog for the AKARI north ecliptic pole Deep field Nagisa Oi1, Hideo Matsuhara1, Kazumi Murata1,2, Tomotsugu Goto3, Takehiko Wada1, Toshinobu Takagi1, Youichi Ohyama4, Matthew Malkan5, Myungshin Im6, Hyunjin Shim6,7, Stephen Serjeant8, and Chris Pearson8,9,10 1 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, 252-5210 Kanagawa, Japan e-mail: [email protected] 2 Department of Space and Astronautical Science, The Graduate University for Advanced Studies, 753-8511 Yamaguchi, Japan 3 Institute of Astronomy and Department of Physics, National Tsing Hua University No. 101, Section 2, Kuang-Fu Road, Hsinchu 30013, Taiwan, R.O.C. 4 Academia Sinica, Institute of Astronomy and Astrophysics, 11F of Astronomy-Mathematics Building, National Taiwan University, No.1, Sec. 4, Roosevelt Rd, 10617 Taipei, Taiwan R.O.C. 5 Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1547, USA 6 Department of Physics & Astronomy, FPRD, Seoul National University, Shillim-Dong, Kwanak-Gu, 151-742 Seoul, Korea 7 Department of Earth Science Education, Kyungpook National University, 702-701 Daegu, Republic of Korea 8 Astrophysics Group, Department of Physics, The Open University, Milton Keynes, MK7 6AA, UK 9 RAL Space, Rutherford Appleton Laboratory, Harwell Oxford, OX11 0QZ, UK 10 Oxford Astrophysics, Oxford University, Keble Road, Oxford OX1 3RH, UK Received 29 August 2013 / Accepted 18 March 2014 ABSTRACT ∗ Aims. We present an 8-band (u , g , r , i , z , Y, J, Ks) optical to near-infrared deep photometric catalog based on the observations made with MegaCam and WIRCam at the CFHT, and compute photometric redshifts, zp in the north ecliptic pole (NEP) region. -
For Each Service They Propose at the Time They File Their Applications, and to Preempt State Regulation to the Maximum Extent Possible
for each service they propose at the time they file their applications, and to preempt state regulation to the maximum extent possible. III. CONCLUSION Viacom submits that the assignment of fixed frequency pairs to PCS licensees will result in higher relocation costs and lengthy delays in the provision of PCS service. Accordingly, Viacom recommends that the FCC adopt the Spectral Zone Coordination approach, under which two PCS licensees in a market are each assured a fixed allocation of 25 MHz in the 1850-1990 MHz band. Under this approach, in the event there is blockage within any PCS licensee's fixed allocation, each PCS licensee would have the flexibility to select needed frequencies within any unused portion of the 1850-1990 MHz band (such unused portion totalling 70 MHz if the FCC allocates 20 MHz to unlicensed services) for any given cell site pending completion of voluntary negotiations or ultimately arbitration and involuntary relocation, thereby minimizing the need for the relocation of incumbents and producing a variety of options for the few required relocations. Alternatively, if the FCC decides, as it has proposed, to allocate three frequency blocks of 30 MHz each, Viacom recommends that the FCC apply the Spectral Zone Coordination technique to its proposed fixed block scheme, providing for a 30 MHz pool which can be accessed by PCS operators on a notification basis until incumbent users relocate as necessary. This type of - 22 - approach will retain most of the advantages of a fixed block scheme while adding much of the flexibility of the Spectral Zone Coordination methodology. -
Design and Development of a Ka-Band Interferometer for Cryospheric Applications Harish K
University of Massachusetts Amherst ScholarWorks@UMass Amherst Masters Theses 1911 - February 2014 2009 Design and Development of a Ka-band Interferometer for Cryospheric Applications Harish K. Vedantham University of Massachusetts Amherst Follow this and additional works at: https://scholarworks.umass.edu/theses Part of the Electrical and Electronics Commons, and the Electromagnetics and Photonics Commons Vedantham, Harish K., "Design and Development of a Ka-band Interferometer for Cryospheric Applications" (2009). Masters Theses 1911 - February 2014. 220. Retrieved from https://scholarworks.umass.edu/theses/220 This thesis is brought to you for free and open access by ScholarWorks@UMass Amherst. It has been accepted for inclusion in Masters Theses 1911 - February 2014 by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. DESIGN AND DEVELOPMENT OF A KA-BAND INTERFEROMETER FOR CRYOSPHERIC APPLICATIONS A Thesis Presented by HARISH VEDANTHAM Submitted to the Graduate School of the University of Massachusetts Amherst in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE IN ELECTRICAL AND COMPUTER ENGINEERING February 2009 Electrical and Computer Engineering DESIGN AND DEVELOPMENT OF A KA-BAND INTERFEROMETER FOR CRYOSPHERIC APPLICATIONS A Thesis Presented by HARISH VEDANTHAM Approved as to style and content by: Paul R. Siqueira, Chair Stephen J. Frasier, Member Daniel H. Schaubert, Member Christopher V. Hollot, Department Chair Electrical and Computer Engineering For my mother, father and sister This Earth is His, to Him belong those vast and boundless skies, Both seas within Him rest, and yet in that small pool He lies. Atharva Veda 12th century BC iv ACKNOWLEDGMENTS I have had an enjoyable and rewarding time working at the Microwave Remote Sensing Lab. -
Shanghai, China Overview Introduction
Shanghai, China Overview Introduction The name Shanghai still conjures images of romance, mystery and adventure, but for decades it was an austere backwater. After the success of Mao Zedong's communist revolution in 1949, the authorities clamped down hard on Shanghai, castigating China's second city for its prewar status as a playground of gangsters and colonial adventurers. And so it was. In its heyday, the 1920s and '30s, cosmopolitan Shanghai was a dynamic melting pot for people, ideas and money from all over the planet. Business boomed, fortunes were made, and everything seemed possible. It was a time of breakneck industrial progress, swaggering confidence and smoky jazz venues. Thanks to economic reforms implemented in the 1980s by Deng Xiaoping, Shanghai's commercial potential has reemerged and is flourishing again. Stand today on the historic Bund and look across the Huangpu River. The soaring 1,614-ft/492-m Shanghai World Financial Center tower looms over the ambitious skyline of the Pudong financial district. Alongside it are other key landmarks: the glittering, 88- story Jinmao Building; the rocket-shaped Oriental Pearl TV Tower; and the Shanghai Stock Exchange. The 128-story Shanghai Tower is the tallest building in China (and, after the Burj Khalifa in Dubai, the second-tallest in the world). Glass-and-steel skyscrapers reach for the clouds, Mercedes sedans cruise the neon-lit streets, luxury- brand boutiques stock all the stylish trappings available in New York, and the restaurant, bar and clubbing scene pulsates with an energy all its own. Perhaps more than any other city in Asia, Shanghai has the confidence and sheer determination to forge a glittering future as one of the world's most important commercial centers. -
Wynne Sworn in As 21St SECAF Col. Hyten Nominated for 1St Star
Ed Parsons The base has more than 6,200 personnel, counting employees of 50th Space Wing Public Affairs tenant organizations such as the Joint National Integration Center Col. Hyten and the Space Warfare Center. Col. John Hyten, commander of the 50th Space Wing here, was The 50th SW and Schriever are part of Air Force Space nominated by President George W. Bush for appointment to the Command, headquartered at Peterson Air Force Base, Colo. Two grade of brigadier general. other AFSPC colonel—Col. Everett Thomas, 341st Space Wing He is one of 32 Air Force colonels nominated Friday by the commander, Malmstrom AFB, Mont., and Col. Edward Bolton, nominated president to the Senate for appointment to the one-star grade. Material Wing Director Satellite and Launch Control at the Space Colonel Hyten assumed command of the 50th Space Wing and Missile Systems Center, Los Angeles AFB, Calif.—were April 4. As commander, he is responsible for nearly 3,600 military, nominated by the president to the one-star rank. Department of Defense civilian and contractor personnel serving Previous 50th SW commanders promoted to general officer at locations worldwide in support of more than 140 communica- ranks include Brig. Gen. (ret.) Lester Weber, Maj. Gen. (ret.) for 1st star tions, navigation and warning satellites with their associated sys- Jimmey Morrell, Lt. Gen. (ret.) Roger DeKok, Brig. Gen. (ret.) tems valued at more than $46 billion. Simon Worden, Lt. Gen. (ret.) Glen Moorhead, Brig. Gen. Larry Colonel Hyten is also the installation commander for Schriever. James and Brig. Gen. (sel.) Suzanne Vautrinot. -
(12) United States Patent (10) Patent No.: US 8,019,275 B2 Norin Et Al
USO080 19275 B2 (12) United States Patent (10) Patent No.: US 8,019,275 B2 Norin et al. (45) Date of Patent: *Sep. 13, 2011 (54) BAND UPCONVERTER APPROACH TO (52) U.S. Cl. ....................... 455/3.02:455/12.1; 455/427 KAAKU SIGNAL DISTRIBUTION (58) Field of Classification Search ........ 455/3.01-3.06, 455/427 430, 12.1-13.3, 168.1, 176.1, 190.1, (75) Inventors: John Norin, Redondo Beach, CA (US); 455/313, 334; 370/316 Kesse Ho, Westminster, CA (US) See application file for complete search history. (56) References Cited (73) Assignee: The DIRECTV Group, Inc., El Segundo, CA (US) U.S. PATENT DOCUMENTS 3,581,209 A 5, 1971 Zimmerman *) Notice: Subject to anyy disclaimer, the term of this 3,670,275 A 6, 1972 Kalliomaki et al. patent is extended or adjusted under 35 4,064,460 A 12/1977 Gargini 4,132,952 A 1/1979 Honguet al. U.S.C. 154(b) by 947 days. 4,354,167 A 10, 1982 Terreault et al. This patent is Subject to a terminal dis 4,382.266 A 5, 1983 Panzer claimer. 4,397,037 A 8, 1983 Theriault 4,403,343 A 9, 1983 Hamada 4,509, 198 A 4, 1985 Nagatomi (21) Appl. No.: 11/546,117 4.513,315 A 4, 1985 Dekker et al. (22) Filed: Oct. 11, 2006 (Continued) FOREIGN PATENT DOCUMENTS (65) Prior Publication Data CN 1413021 4/2003 US 2007/OO83898A1 Apr. 12, 2007 (Continued) Related U.S. Application Data OTHER PUBLICATIONS (60) Provisional application No. -
Absorption, Fluorescence and Emission Anisotropy Spectra of 4-Cyano-N,N-Dimethylaniline in Different Media and at Different Temperatures
Absorption, Fluorescence and Emission Anisotropy Spectra of 4-Cyano-N,N-dimethylaniline in Different Media and at Different Temperatures A. Kawski and G. Piszczek Luminescence Research Group, Institute of Experimental Physics, University of Gdansk, ul. Wita Stwosza 57, 80-952 Gdansk, Poland Z. Naturforsch. 52a, 409-414 (1997); received March 3, 1997 The effect of temperature on fluorescence and emission anisotropy spectra of 4-cyano-N,N- dimethylaniline (CDMA) was investigated in viscous (glycerol and paraffin oil) and rigid (polyvinyl alcohol) PVA and polyvinyl chloride) PVC) media. A strong effect of temperature on the intensity of a and b emission bands was observed. It was also found that the emission anisotropy, r, does not vary in the longwave emission band a at a fixed temperature but decreases in the emission band b together with the decreasing wavelength. The latter effect is due to the fact that the transition moment in this band is perpendicular to the long axis of the CDMA molecule. For CDMA in paraffin oil, a normal b band with negative emission anisotropy only occurs. In all other media used, the emission anisotropy has lower values, approaching zero, which results from the considerable covering of band b with a broad emission band a. 1. Introduction It was demonstrated in addition that the original 1 1 hypothesis [1, 5, 8] of solvated-induced Lb/ La state The investigations of Lippert et al. [1-4] concern- crossing may be combined with the twisted internal ing light polarization (emission anisotropy) in the ab- charge transfer (TICT) mechanism [9,10] to form a sorption and fluorescence bands of p-cyano-N,N- consistent intramolecular reaction model [3, 11]. -
I the 'II Log-Periodic Yagi Bandpass Beam Antenna
I the 7 LPY + this month cw transceiver 14 measuring antenna gain 26 solid-state crystal oscillators 33 * six-meter transverter 44 glass semiconductors 54 'II log-periodic yagi bandpass beam antenna ... but not for the KWM-2 At 100,000 miles, it's still the liveliest rig on the road. Amateurs punch through the QRM on 20 meters with Mosley's A-203-C, an optimum spaced 20 meter antenna designed for full power. The outstanding. maximum gain performance excells most four to six element arrays. This clean-I ine rugged beam incorporates a spe- cia1 type of element design that virtually eliminates element flutter and boom vibration. Wide spaced; gamna matched for 52 ohm ck"1, line with a boom length of 24 feet and\/ elements of 37 feet. Turning radius is 22 feet. Assembled weight - 40 Ibs. 5-401 for 40 meters A-31 5-C for 15 meters \ Full powered rotary dipole. Top signal for Full sized, full power. full spaced 3-element DX performance. 100% rustproof hardware. arrays. 100% rustproof all stainless steel Low SWR. Heavy duty construction. Link hardware; low SWR over entire bandwidth; cou~linaresults in excellent match. Lenath Max. Gain; Gamma matched for 52 ohm line . is 43' 15 3/8"; Assembled weight - 25 lk. - - - - - - -117. m lcatlons and pel e data, write De --"- -"6 4610 N. Lindbergh Blvd.. Bridgeton. h& july 1969 1 / A 5 BAND 260 WATT SSB r- TRANSCEIVER WITH BUILT-IN AC AND DC SUPPLY, AND LOUDSPEAKER, IN ONE PORTABLE PACKAGE. Thc Swii~lCv~liet IS the most versatile and portable transce~ver on the market, and certa~nlythe best posslble value. -
Antique Radio Charlotte an Annual Conference for Antique and Vintage Radio Collectors and Historians
Antique Radio Charlotte An annual conference for antique and vintage radio collectors and historians. 3rd Bi-annual Charlotte International Cryptologic Symposium Thursday, Friday & Saturday March 24-25-26, 2016 Sponsored by the Carolinas Chapter of the Antique Wireless Association Meet Results CAROLINAS CHAPTER OF THE AWA http://www.cc-awa.org/ PRESIDENT SECRETARY-TREASURER Ron Lawrence Clare Owens P O Box 3015 101 Grassy Ridge Ct. Matthews, NC 28106 Apex NC 27502 704-289-1166 919-363-7608 [email protected] [email protected] VICE PRESIDENT Richard Owens EXECUTIVE COMMITTEE R L Barnett Stephen Brown Kirk Cline Barker Edwards Robert Lozier Chip McFalls EDITORS Barker & Judy Edwards 116 East Front Street Clayton NC 27520 919 553-2330 [email protected] Membership in the Carolinas Chapter of the Antique Wireless Association (CC-AWA) is open to anyone with an interest in old (antique) radios. Anyone who pays registration for the 2016 conference will automatically receive one year’s membership in the Carolinas Chapter of the AWA. This is only chapter membership and does not include membership in the Antique Wireless Association. If you are already a paid member in the chapter, your membership will be extended one year. Any correspondence, including any newsletters that are published, will be distributed electronically. Please make sure that the CC-AWA has a current email address on file. Old Equipment Contest Pictured are the 1st place winners. To view all the winners, please visit our web page at: www.cc-awa.org. HM-Honorable mention No Entries CATEGORY 1 PRE-1912 ELECTRICAL DEVICES NON RADIO No Entries CATEGORY 2 PRE-1920 RECEIVERS & TRANSMITTERS AND WIRE LINE TELEGRAPH ITEMS CATEGORY 3 1920s ERA BROADCAST RECEIVERS A. -
Modifications for the ICOM
Modifications for the ICOM created 28-03-2002 from www.mods.dk (AH-4) Icom, AH-4, AH-3 ( automatic antenna tuner ) connection to any radio. English language (AT-160) Using the AT-160 with the IC-706MKII English language (AT-500) AT-500 Automatic Antenna Tuner Modification English language (AT-500) ICOM AT-500 Tuner Hint English language (I290) Icom I290 scan modification English language (IC-02) Band expansion modification for IC-02AT English language (IC-02) Audio modification for IC-02 AND IC-04 English language (IC-02) IC-02A Modified PLL rigs English language (IC-02) Low audio speaker mike on IC2A, 3A, 4A OR 02AT English language (IC-02) ICOM 02/03/04 & Vox Unit English language (IC-02) Another band expansion mods for Icom IC-02 English language (IC-02) For increased receive audio and improved response English language (IC-02) To increase the memory scan and search scan speed English language (IC-02) ICOM HS-10SA VOX for IC-02AT Mods English language (IC-03) ICOM 02/03/04 & Vox Unit English language (IC-04) ICOM 02/03/04 & Vox Unit English language (IC-04) Out of band modification for IC-04 English language (IC-04) Audio modification for IC-02 AND IC-04 English language (IC-04) Low audio speaker mike on IC2A, 3A, 4A OR 02AT English language (IC-04) TX delay may be excessive at low temperatures English language (IC-04) IC-04E fuer 9k6 German language (IC-1200) Expanded RF 870 - 960 MHz for ICOM IC-1200 English language (IC-1271) VOX of an IC-271,471,1271 usable for FM English language (IC-1271) RAM Card Backup Battery Replacement Instructions English language (IC-1275) IC-1275 Freq. -
The Origin of UV / Optical Variability of AGN: Relationship to X-Ray Variability
The origin of UV / Optical Variability of AGN: Relationship to X-ray Variability Ian McHardy University of Southampton 1 Southampton Main Questions • What drives UV/optical variability in AGN? • How is the X-ray band related to UV/optical? • What do X-ray/UV/optical variations tell us about AGN inner structure? 2 Southampton Possible drivers of UV/optical Variability - Reprocessing of higher energy photons - which “high” energy? X-ray? Far-UV? - reprocessing off what? Disc? BLR? - Intrinsic disc variations 3 Southampton Observational Diagnostics • Reprocessing - High energies lead uv/optical by short (hour-days) light travel time. Allows ‘reverberation’ mapping of reprocessing structures. Measure lag from different temperature regions (different λ ). • Intrinsic disc variability – High energies lag: two possibilities – Long lag (months), viscous propagation timescale for perturbations to reach X-ray region from optical in disc – Short lag (hour-day), light travel time of UV seed photons to corona 4 REPROCESSING Southampton Wavelength dependence of lags For standard Shakura-Sunyaev DISC, 4 −1 −3 L(R)=σT ∝MBH . m! E R dissipating gravitational potential energy ! ( R in gravitational radii) −1/4 1/4 −3/4 i.e. T ∝ M m! R BH E Disc illumination from point source, height H above disc, also falls off as H R-3 So for reprocessing 4/3 Lag ∝Wavelength (eg Cackett et al 2007) from disc, we expect and Lag ∝M2/3m! 1/3 ! E For illumination of a shell-type structure, eg the BLR or torus, Illumination falls of as R-2 giving Lag ∝Wavelength2 5 Southampton