INDOOR LOCATION USING ULTAWIDEBAND CHAOTIC RADIO PULSES Andrey A. Dmitriev Institute of RadioEngineering and Electronics, Russian Academy of Sciences, Mokhovaya St. 11-7, K-9, GSP-9, 125009, Moscow, Russia, E-mail: chaos@cplire.ru Abstract ­ The report is devoted to the problem of indoor location using ultrawideband chaotic signals. ... In the receiver the moment of pulse (pack of radio pulses) emission and the duration of chaotic radio pulse are supposed known. The duration of CRP is fixed. ...

... 13, Moscow 119992, Russian Federation, e-mail: busarev@sai.msu.ru; 2 Research Institute Crimean Astrophysical Observatory, p/o Nauchnyi, Crimea 334413, Ukraine, e-mail: prok@crao.crimea.ua Summary: We propose a combined method of astronomical investigations of small or distant planets incorporating registration of a set of integral spectra of an object and their frequency analysis. ... An application of the method is shown on example of asteroid 21 Lutetia. ... 6] Busarev V. V. (2002), Solar Sys. ...

... Oleg V. Verkhodanov . ... The last few years have changed our view on the evolution of galaxies: the most distant galaxies (i.e. systems having stellar population) have been found at redshift z=6.68 (Chen H.-W., Lanzetta, K. M., Pascarelle, S. 1999, Nature, 398 , 586) and radio galaxy at z=5.19 (van Breugel W., De Breuck C., Stanford S. A., Stern D., Rottgering H., Miley G. 1999. astro-ph/9904272 ). ... Redshifts and age of stellar systems of distant radio galaxies from multicolour photometry data. ...

... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

This is to help you migrate from Mail::Bulkmail 2.x to Mail::Bulkmail 3.x change use Mail::Bulkmail 2.05 to use Mail::Bulkmail 3.03 "/path/to/conf/file"; change $bulk->allow_duplicates(1); to $bulk->Trusting('duplicates' => 1) (should be in the conf file as Trusting @= duplicates) change $bulk->safe_banned(1) to $bulk->Trusting('banned' => 0); (should just not be specified, since it defaults to 0. ... Headers from message (HFM) is no longer supported. ...

... In less then one day "Mir" station will finish its flight. ... Besides, the operability of motion control systems will be tested to ensure further dynamic operation at the final stage of "Mir" complex. ... The final third burn is given in daily orbit 2 using the "ProgressM1-5" 8 control engines and its main engine with the trust of 300 rg/s. Thus, to peform deorbit maneuver the OC"MIr" real-time tested manuevers involving control engines and their combination with the main engine are used. ...

... The mount is also adjustable so you can orient the axis of rotation to make it parallel with the Earth's axis of rotation (see the section on Polar Alignment). ... Locate the opening in the equatorial mount on the DEC axis. ... To mount the telescope tube: 1. ... ADJUSTING THE MOUNT FOR POLAR ALIGNMENT In order for the clock drive to track accurately, the telescope's axis of rotation must be parallel to the Earth's axis of rotation, a process known as polar alignment. ... R.A. & DEC axis ! ...

LAUNCHING . The first launch of LV Energia . ... The first launch . ... The launch vehicle was first launched from the versatile "Stand-Start" complex on May 15, 1987, at 21:30 Moscow time. ... The first successful launch of LV Energia proved that a versatile, heavy-lift LV Energia having no analogs in the world rocket building has been developed. The second launch of LV Energia carrying the Buran Orbiter was scheduled on October 29, 1988. ... Official WEB-site of S.P.Korolev RSC Energia . ...

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... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...