... Solar System . ... Comets and Asteroids . ... Vision of Vesta: a dark feature with a diameter of approximately 100 kim near the asteroid's equator can be seen in this image from Dawn (Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA) . Between Mars and Jupiter lies the Asteroid Belt. ... The Dawn space probe is expected to go into orbit around Vesta on 16 July, from there it will return some detailed images and other data, staying at the asteroid for about a year before setting off to visit Ceres. ...

... Home Articles Mars Attacks: First Anniversary of the Great Approach . ... Beyond New York City . ... Mars Attacks: First Anniversary of the Great Approach . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Our own two Amateur Astronomers Association events were a resounding success. ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

В начале статьи авторы представляют для обсуждения основные концепции и первоначальную систему аксиом, которые могут быть использованы для дальнейших исследований в области SETI. Одним из основных свойств Вселенной ученые, занимающиеся поиском сигналов, называют жизнь. ... а) жизнь существует во Вселенной (аксиома существования); . ... Авторы утверждают, что данные оценки не являются причиной для пессимизма, и формулируют требования для Глобальной Стратегии Поиска (ГСП) ВЦ. ...

... Routines for accessing I/O ports are in /usr/include/asm/io.h (or linux/include/asm-i386/io.h in the kernel source distribution). ... Before you access any ports, you must give your program permission to do so. This is done by calling the ioperm() function (declared in unistd.h , and defined in the kernel) somewhere near the start of your program (before any I/O port accesses). ... For example, ioperm(0x300, 5, 1) would give access to ports 0x300 through 0x304 (a total of 5 ports). ...

Next: Mission Operations Data Transfer . ... VLBI Tape Management . VLBI Tapes . ... When: As soon as the correlator is satisfied with the correlator output. back to top . ... What: Each correlator will maintain a data base including the status of all VLBI tapes under its control. ... The correlators will distribute tapes to mission elements based on the Observation Summary File produced by the RSOG ( Observation Summary File ) to ensure each element has enough tapes to support SVLBI observations. ...

Gamma-rays from the GC . M.Chernyakova (DIAS), D.Malyshev (DIAS), F.Aharonian (DIAS, MPIK), R.M.Crocker(MPIK), D.I.Jones(MPIK) 1 10°x10° Count and TS maps (>300 GeV) Gamma-rays from the GC 2 TS maps of the GC at different energies 300 MeV ­ 3GeV 3 GeV ­ 30 GeV 30 GeV ­ 300 GeV Gamma-rays from the GC 3 4 Gamma-rays from the GC Lightcurve 5 Gamma-rays from the GC Source spectrum Model X-ray and low-energy emission come from the central object, probably SMBH accretion disk. ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... A most promising problem is to investigate the interaction of two VHF powerful radiowave beams in the ionosphere, whose difference frequency is equal to the plasma frequency in some ionospheric area (that is, the difference frequency is taken in the range 1-8 MHz). ... Two-frequency interaction effects are based on radiowave non-linear mixing, which is rather complicated when describing and modelling the experiment. ...

See SBIG or APOGEE for instructions on building and installing the software for your camera. It helps to have a recent Linux operating system installed. ... Edit protocol.h for the filter wheel and maximum filter count in your system. With recent versions of Linux, ds9, and xpa you must add this to the local profile (e.g. in /etc/profile.local for global use): export XPA_METHOD=local Otherwise, you will see an error message when ds9 starts, and xmccd and ds9 cannot communicate. ...

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