... ASTEROID’S MOONS : DISCOVERY BY RADAR . ... Moons of known asteroids have a low position ambiguity, which makes their discovery with powerful ground-based radar much easier than the discovery of new asteroids or other objects of Solar System. ... The other technique is a direct detection of radar echo from an asteroid moon. ... However, the diameter of a ground-based fully-steerable reflector is limited by 120-150 m to make it possible to perform two different functions: focusing and tracking (fig. ...

Parkes Future Receiver Discussions Naomi McClure Griffiths 11 July 2012 Parkes Receivers Interim (2012 2014?) Need to address an:cipated receiver usage · Group of Astros met in May to brainstorm future projects · Assume current instrumenta6on Fig 1, from CarreA & Bock report Feb 2012 2 Parkes Receiver Discussions | ... Naomi McClure Griffiths Advice on prioriGes ATCA For later, but start thinking now ­ the case for going to 12.2 GHz on the Compact Array 8 Parkes Receiver Discussions | ...

Radio Interferometry Principles . Radio Interferometry Signal Processing . ... A radio interferometer consists of a pair of directional antennas that are tuned to receive radio emissions from a source in a desired RF band. ... The antennas are pointed at the radio source of interest and are set up to receive the signal and process it into a form suitable for transmission to the correlator. ... In connected element interferometry, the digital signal goes directly to the correlator. ...

... USSR Venus Orbiters . ... Each spacecraft consisted of a synthetic aperture radar (SAR) and a radio altimeter. ... The Venera 15 and 16 synthetic aperture radar (SAR) systems were identical, and were used to map the surface of Venus at a resolution of 1 to 2 kilometers (.6 to 1.2 miles) over a period of 8 months. ... The Venera 15 and 16 radar (radio) altimeter systems were identical, and were used to determine the topography of the surface of Venus from the north pole down to about 30њN latitude. ...

Here we report our discovery of a band of blue luminescence (BL) in the Red Rectangle nebula. ... The spectrum of this newly discovered BL is most likely fluorescence from small neutral polycyclic aromatic hydrocarbon (PAH) molecules. ... If the carriers of this near-UV/blue fluorescence are PAHs, they are most likely neutral PAH molecules consisting of three to four aromatic rings such as anthracene (C14H10) and pyrene (C16H10). ...

... Jade morton (now at colorado state) brought a novatel multi frequency gps receiver to ao. ... The cpu will be placed in the antenna test shack while the active antenna will be on the roof of the shack. ... An rf cable out to the 904 antenna probe . ... the red lines show the 10 sweep peak hold. 904 probe at the antenna (.pdf) . 904 probe at the front of the cpu (.pdf) . 904 probe at the back of the cpu (.pdf) . 904 probe with antenna, cpu off (.pdf) . ... near 425 Mhz . ...

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

Peremennye Zvezdy", . ... USNO-B1.0 1413-0363790, 2MASS 20315512+5119384 . ... During our work, we have discovered a previously unknown variable star, a possible dwarf nova USNO-B1.0 1413-0363790. Our observations were carried out between May and August, 2012 with the Master-URAL system consisting of two parallel optical telescopes on the same mount (40-cm aperture, 1:2.5 focal ratio) and equipped with two Apogee Alta U16M CCD cameras (Kodak KAF16803 chip, Peltier cooled) (Lipunov et al. ...