... The Clouds of Jupiter . ... Credit: Voyager Project , JPL , NASA Explanation: What makes the colors in Jupiter's clouds ? With a mean temperature of 120 degrees Kelvin (-153 degrees Celsius) and a composition dominated by hydrogen (about 90%), and helium (about 10%) with a smattering of hydrogen compounds like methane and ammonia, the blue, orange, and brown cloud bands and the salmon colored "red" spot are hard to explain. ... NASA Official: Jay Norris. ... Publications with keywords: Jupiter . ...

Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... September . ... Posted on September 27, 2010 | 11 Comments In the early 1960s, the sky had no limits for NASA . ... Continue Reading.. ... 69 Comments ?Rods from God? is the nick-name given to a hypothetical orbital weapon for bombarding targets on the Earth from space. ... No Comments Dark matter and its part in the evolution of the Universe is revealed by new data collected by the Hubble Space Telescope. ...

. Sergei and keyboard, photo by A.Yuferov .

... Posts tagged ?Skilling? ... Tags: arXiv , likelihood , MCMC , Nested Sampling , posterior , probability , Skilling . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

... R. Cesaroni, F. Massi, C. Arcidiacono, M.T. Beltr\'an, D. McCarthy, C. Kulesa, K. Boutsia, D. Paris, F. Quir\'os-Pacheco, M. Xompero . 2012, A , in press . Different evolutionary stages in massive star formation . A. Sanchez-Monge, M.T. Beltran, R. Cesaroni, F. Fontani, J. Brand, S. Molinari, L. Testi, M. Burton . ... Massive star-formation toward G28.87+0.07 (IRAS18411-0338) investigated by means of maser kinematics and radio to infrared, continuum observations . ... 2012, ApJ, in press . ...

The spatial power spectra of Galactic . ... Neutral hydrogen is an important constituent of the interstellar medium, and has been widely studied at 21 cm line emission. Within the Galactic plane, structure of HI emission is seen over wide range of angular scales, down to tens of milliarc seconds. ... In the high galactic latitudes an alternative approach is seen more reasonable - to describe HI emission in terms of an angular power spectrum over a range of scales. ... Figure 1. ...

... Circumstellar disc of beta Pictoris: constraints on grain properties from polarization. To appear in the Astronomy & Astrophysics . abs , src , ps ] . ... Dust influx to Titan from Hyperion . ... abs ] . ... Characteristics of bulges and disks in interacting galaxies . ... Dust grains around Herbig Ae/Be stars: porous, cometary-like grains? ... To appear in the Astronomy & Astrophysics Supplement . ... Finally, Links may lead you to more options (e.g. via the LANL preprint system). ...

. Last updated 18 Mar 1999 . The ported software list for XFree86/OS2 is currently under construction. You can find the old pages at this link . In the future, you might find it likely here Trouble that the URLs below are not reachable? Try to look at alternative sites that archive stuff: . set.gmd.de . crydee.sai.msu.su . www.powerusersbbs.com . Reply to: Holger.Veit@gmd.de .

... as the contribution number (if you have several contributions, e.g. 1, 2, 3): /p p First submission: /p form method=get action= http :// hea.iki.rssi.ru / integral06 -perl-bin/proceedings.pl input type =text name =email SIZE=26 MAXLENGTH =200 input type =text name =number SIZE=2 MAXLENGTH =5 value=1 INPUT type = submit value= Submit / ...

... We have been upgrading the software front-end to WASP (Wideband Autocorrelating SPectrometer, operating from 800 to 4000 MHz) from Lynx-OS to Real-Time Linux and will discuss Real-Time software aspects. We are using a standard parallel ``PIO'' card to receive data from the spectrometer and standard GPIB interfaces that drive a frequency synthesizer for bandpass calibration. WASP and its front-end computer are fully mobile and can be taken to any suitable radio telescope. ...

Прохождения БКП . через центральный меридиан Юпитера . в сентябре 2003г: . ... В указанные моменты времени вы увидите Большое Красное Пятно вблизи центра диска Юпитера. Это уникальное образование в атмосфере планеты легко доступно наблюдениям в пределах +/- полутора часов от указанного момента. ... Астрокалендарь | ...