... 2002 August 5 . Rays from an Unexpected Aurora . ... For starters, last Friday morning, no intense auroral activity was expected at all. Possibly more surprising, however, the aurora appeared to show an usual structure of green rays from some locations. ... Large sunspot groups indicate that activity from the currently active Sun is relatively likely, possibly causing other streams of energetic particles to cascade onto the Earth and so causing more auroras . ... About APOD | ...

Astronomy Picture of the Day . Unexpected Impact on Jupiter . ... 8.09.2009 . ... First discovered by an amateur astronomer Anthony Wesley on 2009 July 19, the impact was quickly confirmed and even imaged by the Hubble Space Telescope the very next day. ... It is now thought that a small comet -- perhaps less than one kilometer across -- impacted Jupiter on or before 2009 July 19. ... July . ... Publications with keywords: Jupiter - impact . Publications with words: Jupiter - impact . ...

Instrument Science Report WFC3 2005-23 Optical Properties of Blocking Glass in the WFC3 IR Channel D.F. Figer & S. Baggett August 16, 2005 ABSTRACT RG830 and IR80 will be used as the optical blocking glass in the WFC3/IR channel to ensure that short-wavelength (optical) light does not reach the detector. ... As can be seen, the transmission through RG830 is very low at wavelengths below about 760 nm, thus providing blocking at optical wavelengths. ... Characteristics of RG830 glass from Schott. ...

Chapter 10. Allocating DMA Buffers on 64-bit Platforms . ... This directly impacts DMA buffers, as a DMA buffer allocated in physical memory that is unaddressable by the NVIDIA GPU cannot be used (or may be truncated, resulting in bad memory accesses). ... On a system with greater than 4 GB of memory, allocating usable DMA buffers can be a problem. ... Newer kernels provide a simple way to allocate memory that is guaranteed to reside within the 32 bit physical address space. ...

... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...

... I.A.Dynnikov, Three-page approach to knot theory. ... Universal semigroup, Funktsional'nyi Analiz I Prilozhenija, 34 (2000), no.1, 29-40 (Russian); English translation in Functional Analysis and Its Appl. 34 (2000), no.1, 24-32. I.A.Dynnikov, Finitely presented groups and semigroups in knot theory. ... Math. 2000, no. ... English translation: Russian Math. ... A.Vershik, Numerical invariants of exponential groups, and a locally free approximation of braid groups (in Russian), Zapiski Nauchn. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . Spaceflights Chronology . Chronology of Extravehicular Activity . ISS 45/46 . ... Rocket Space Complexes . ... Launches Chronology . ... Automatic Space Systems . ... HISTORY . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

stable spacetime manifold Expected to propagate at speed of light Expected to have 2 independent polarizations Sources ­ ­ ­ ­ http ://www.johnstonsarchive.net/relativity/pictures.html Unmodeled bursts Binary Coalescence Periodic Sources Stochastic Background http ://mucholderthen.tumblr.com/post/55970198303/gravitational-waves-patterns-in-space-time-a 3 LIGO-VIRGO Interferometer Gaussian Noise: Coherent Signal vs. ...

... 314 Astronomical Data Analysis Software and Systems XIII, eds. F. Ochsenbein, M. Allen, & D. Egret (San Francisco: ASP), 812 . ... Abstract: The calculation of flux upper limits in the source-free ("background") regions of photon-limited images is complicated by instrumental and statistical modeling and requires non-trivial computational effort. ... The principal component in this is the time taken to pre-process and handle the 30 GB of RASS data rather than the calculation of each upper limit. ...

DISCLAIMER: The larger the aperture, the more light a telescope will gather and the fainter the object you can see. Here is a range of magnitudes you might expect to see. Given excellent sky conditions and good optics, a well trained eye can sometimes add up to 0.8 magnitude to these values. Limiting Magnitude depends on much more than the instruments aperture. ... One formula is for aperture in inches the other is for aperture in millimeters. ... Aperture (inches) . ... 15.2 . ...

... Magnetic storms online . ... Geomagnetic activity forecast . ... August : 2015 . ... No magnetic storm is expected . From 2 August 2015 to 28 August 2015 the following magnetic storms and disturbances are expected: . August 10, 2015 geomagnetic storm of level G1 (minor) . August 28, 2015 geomagnetic disturbances . ... August 06, 2015 geomagnetic disturbances 2 August 2015 - 28 August 2015 . 01.08.2015 . ... Probability of a magnetic storm . ... Probability of a strong magnetic storm . ...

... The contribution of backgrounds in signal box is estimated using sideband region. data , Blinded Events / ( 0.025 ) 25 Events / ( 0.0275 ) P M data 30 P E data 25 P f f qq data = QE D 20 20 QE D ЗP + 15 15 10 З (1 - f QE D ) З Pq q + 10 5 5 (1 - fQE D - fqq З (1 - fQE D )) З P E 0 - 0.6 -0.5 - 0.4 -0.3 - 0.2 -0.1 -0 0.1 0.2 0.3 0.4 x: delta M 0 - 0.6 - 0.4 - 0.2 0 M 0.2 0.4 y: delta E E data , Blinded ... LF V tau decay s Olga Igonkina DPF 2004 12 ...

... 96.1655Garwood+ We presented results from a continuum VLA snapshot survey of the galactic plane in the longitude range 0d < l < 90d at 1.5 GHz. Observations were taken every 0.5^o in longitude at b=0^o. Most fields are complete to about 30 mJy peak density. The positions, peak, and total flux density of 471 compact sources (<30") have been measured. ... This catalog contains results from a continuum VLA snapshot survey of the galactic plane in the longitude range 0d < l < 90d at 1.5 GHz. ...

The overall efficiency (including atmospheric transmission, reflectivity of the telescope mirrors and overall efficiency of the optics and of the detector) for broad-band imaging should be about 25% in H and K, and about 15% in J. The main noise source for both broad- and narrow-band imaging should be the photon noise associated to the background+source flux. ... Flat fielding (and possibly background subtraction) might increase the noise by a factor 2 ? ...

Apriori edit data for v190 ! ... There is one flag per station per scan covering time from start of tape ! ... opcode = ' FLAG ' dtimrang = 1 timeoff = 0 ant_name ='Pa' timerang = 74,02,30,00, 74,02,40,00 reason ='Slew limits or horizon' / ant_name ='Pa' timerang = 74,02,40,00, 74,02,40,46 reason =' Slewing expected .' / ant_name ='Pa' timerang = 74,02,45,00, 74,02,45,09 reason =' Slewing expected .' / ant_name ='Pa' timerang = 74,02,50,00, 74,02,50,09 reason =' Slewing expected .' / ...

... The BL Lac objects found within DXRBS fall mostly in the range . ... A large fraction of the BL Lacs so far in our sample are at L X / L R < 10 -6.5 , the region of Figure 6 populated by LBLs. In this region of parameter space (to the left of the left-most dashed line in Figure 6), DXRBS includes objects up to two orders of magnitude fainter than the 1 Jy survey. ... For comparison, we have plotted the values for members of these three ROSAT-based surveys (DXRBS, HQS/RASS and RC) in Figure 7. ...

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2010 . ... Moon's topography is shown based on LOLA laser altimeter data, white contour shows a permanently shadowed region and a white rhomb indicates LCROSS spacecraft impact location. ... Ultra deep survey of the sky in hard X-rays, performed by INTEGRAL observatory . INTEGRAL observatory has completed the first and the most sensitive survey of the sky in hard X-ray energy band. ...

... Archive 2003: . As a result of development of image slicers, polarization analyzers and reduction technique, the limiting magnitude of spectral observations at BTA with high spectral resolution (up to R=80000) has been increased by 3 times, the limiting magnitude of spectropolarimetric observations increased from 3 to 8 times (in the red and UV ranges, respectively). ... Archive . ...

Next: Procedure for Dealing with Up: scientific Previous: Code of Good Practice . ... Any practice or conduct that seriously deviates from the ethical standards embodied in the Code of Good Practice for Scholarly and Scientific Research for proposing, conducting and publishing scientific research constitutes Scientific Misconduct, and if proven renders the offending member liable to the Observatory's disciplinary procedures. ...

Documentation for Delay Line Final Design Review - 12 Feb 2008 Notes: Anything marked in Status as [TBU] is definitely `To Be Updated' `Expected Date' refers to the expected date of release where this is likely to be different from the due date. ... TBU] INT-406-VEN-0112 MF/RCB/DMAW/EBS 22 Jan 08 22 Jan 08 Released. ... MF/XS/DMAW MF MF MF MF/XS/DMAW 22 Jan 08 29 Jan 08 Yet to be drafted 22 Jan 08 22 Jan 08 Yet to be drafted 22 Jan 08 22 Jan 08 Released. ... Document No. ...