... also take data with dewar monitoring turned off. a2010 alfalfa data from the last year was used to get an idea when the problem started. ... You can see the oscillations clearly in beam2a,b . ... The oscillation does not show much frequency dependence. 16feb11: . ... A 2.5 MHz oscillation was seen at the dewar bias voltages when a spectrum analyzer was attached at the dewar. 21jan11 (.ps) ( .pdf) . ... Turning the dewar bias monitoring off caused the oscillation to disappear. ...

... Data from various satellite missions concerning emission lines formed at temperatures of 7 x 10 4 K to 1.3 x 10 5 K show oscillations in sunspots with frequencies in the range of 5.8-7.8mHz. ... All the observational data clearly indicate the presence of 3-minute oscillations in sunspots in spectral lines covering a vast temperature range from the low chromosphere to those lines normally associated with coronal temperatures. ...

Next: Inverse transform Up: No Title Previous: Analysis of a . As pointed out earlier, if the data are periodic, Fourier analysis is best and there is no need for wavelet transforms. ... First, we show the graph of with its Mexican-hat wavelet transform (Fig 12). Figure 12: g2-wavelet map of showing the gradual shift to shorter durations. ... Figure 13: g2-wavelet map of a strongly modulated oscillation. ... Figure 14: g2-wavelet map of an intermittent signal. ...

... Toward this goal, the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey -III (SDSS-III) has measured slight recurring density enhancements in galaxy densities up to six billion light years away ( redshift 0.7), when the universe was about half its current age. ... BOSS's measurements of this size scale indicate a strong universe component of dark energy , and so bolsters previous indications of this unusual composition. ... NASA Official: Jay Norris. ...

... 2014 January 20 . Baryon Acoustic Oscillations from SDSS-III . Illustration Credit: Zosia Rostomian ( LBNL ), SDSS-III , BOSS . ... Toward this goal, the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey -III (SDSS-III) has measured slight recurring density enhancements in galaxy densities up to six billion light years away ( redshift 0.7), when the universe was about half its current age. ... About APOD | ... NASA Official: Phillip Newman Specific rights apply . ...

... Posts tagged ?Solar Oscillation? ... ArXiv] 2nd week, Apr. ... Tags: Classification , GRB , Hubble constant , K-S test , kurtosis , mask , maximum likelihood , SDSS , skewness , Solar Oscillation , Vicent Martinez . ... 3 Comments . ... Entries RSS . Comments RSS . ... General comments . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ... Alfred Inselberg on [MADS] Parallel Coordinates . ... SAMSI AstroStat Prog. ... Entries (RSS) and Comments (RSS) . ...

... It is important for formulation of the main targets of the “Cosmological Gene” of RAS, which is under way at RATAN-600 radio telescope, as ground based support of the PLANCK Experiment. Scientific Organizing Committee . ... SAO RAS), Varshalovich D. (Ioffe Institute), Kardashev N. (ASC FIAN RAS), Novikov I. (ASC FIAN RAS), Rubakov V. (INR RAS), Starobinsky A. (Landau Institute for Theoretical Physics) Local Organizing Committee . ... Last name: . ... Your institute: . ... Last update 13.09.2007 ...

This lecture is based on the end of chapter 5 in the text (Chapter 4 in the 2nd edition) . You will be introduced to this in labs, but feel free to install and play with it yourself: link is http://www.vpython.org/ .

... Based on observations with the NASA/ESA Hubble Space Telescope , obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., ... Lower limits derived from blackbody (stellar atmosphere) model fits to these data are 95,000 K ( 85,000 K); the corresponding upper limits on the projected area of this source are all < 2% of the WD surface area. ... huizinga@stsci.edu . ...

... Dymova M., Ruderman M. S., Non-axisymmetric oscillations of thin prominence fibrils // Solar Phys. - 2005 - V. 229, P. 79-94. ... Dymova M., Ruderman M. S., Resonantly damped oscillations of longitudinally stratified coronal loops // Astron. ... Dymova M., Ruderman M. S., The geometry effect on transverse oscillations of coronal loops // Astron. ... Astrophys. ... Ruderman M. S., The effect of flow on transverse oscillations of coronal loops // Solar Phys. - 2010 - V. 267, P. 41­54. ...

... Institute of Radioengineering and Electronics of the Russian Academy of Sciences . Mokhovaya st., 11, Moscow, 103907, Russia . Email: chaos@mail.cplire.ru . ... Proceedings of International Conference on Control of Oscillations and Chaos (COC-2000 ), St.Petersburg, Russia, July 5-7, 2000 , vol. 3, pp. ... Here we describe a method for separating the sum of chaotic signals into the individual components, using the inherent underlying dynamics of the chaotic sources. ...

Irregular phenomena in the Earth Pole oscillation process and temporal variations of geopotential Valery Bondarenko, Vadim Perepelkin s The observed irregular phenomena in the Earth Pole oscillation process are very variety. ... These phenomena indicated in the IERS data are the "abnormal" fluctuation of the Earth Pole coordinates which owing to changing of the geodynamical parameters gives negative result in interpolation and forecast of the first approximation mathematical model. ... Fig. ...

... The curve of the photoconductivity of n -GaAs versus the magnetic field during monochromatic infrared illumination reveals oscillations consisting of two series of extrema which are periodic along the inverse-field scale. One series of extrema stems from the nonmonotonic field dependence of the impurity magnetoabsorption coefficient, the other stems from a sharp step in the distribution function of nonequilibrium electrons. PACS: 72.40.+w, 72.80.Ey, 78.20.Ls ...

... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to E-ELT Armazones . ... ESO . ... Survey Telescopes . ... Star Clusters . ... Stars@ESO . ... ESO Science Newsletter . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... ESO 1-metre Schmidt telescope . ... ESO Science Outreach Network . ... This image is a graphical representation of resonating acoustic waves in the interior of a solar-like star. ...

... V.N. Obridko . ... Oscillations . ... Solar cycle . ... Solar Corona . ... webmaster@izmiran.ru . ... B.A. Ioshpa, V.N. Obridko, B.D. Shelting . ... Solar Physics 29 (1973) 385-392. ... Quasi-biennial oscillations of the global solar magnetic field . ... Quasi-biennial oscillations of the solar global magnetic field . ... Quasi-biennial oscillations of the Solar magnetic fields . Proc. 10th European solar physics meeting",Solar variability: from core to outer frontiers", Prague, Czech. ...

... Irregular, damped ULF range magnetic pulsations occurring in connection with magnetospheric substorms are called Pi 2 pulsations (T = 40 - 150 s; Saito, 1969). ... Since the waves can be detected with little time delay over a wide range of latitude and longitude, they have been used for the ground based determination of the substorm onset time. ... Lester, M., W. J. Hughes, and H. J. Singer, Polarization patterns of Pi 2 magnetic pulsations and the substorm current wedge, J. Geophys. Res., ...

... AXPs (McGill catalogue) SGR Bursts Peak luminosity reaches 1041 erg/s (Eddington ~ 1038 erg/s) Power law burst energies, log normal waiting times (e.g. earthquakes, solar flares, avalanches) time (seconds) (Woods Thompson 2006) bursts per 10 day interval 103 counts/second year (Hurley 2010) Giant Flares Initial hard spike ~ 0.1 s Pulsating tail 100-300 s Total Energy 44 - 1046 erg 10 March 1979 SGR 0526-66 counts/second k-counts/second counts/second August 1998 ...

... Equilibria occur when €аa €аthey may be stable ( €а), unstable ( €а) or half-stable ( €а). ... c. €а €аtranscritical bifurcation . d. €а €аpitchfork bifurcation . ... Abstract to €аcontrol-space diagram and bifurcation set. ... No oscillation possible . 7. тАЬTo and froтАЭ oscillations (librations) vs тАЬover the topтАЭ oscillations (rotations). ... Two equilibria €аone stable and one unstable. ...

... On Thursday, 11/12, Bill Boroski, Bob Nagel, Steve Bastian and John Davis continued to pursue the oscillation in the windscreen and lubricating the cone bearings. Bill was able to install the bar coder for the altitude drive. ... On Friday, 11/13, Charlie Briegel continues to work on motion controls. ... Bill has also installed the bar coder for the azimuth drive. And Steve along with Bob Nagel clean the bearings with mineral spirits in preparation for applying the new lubricant. ...

. The Oscillation Project with Emulsion-tRacking Apparatus (OPERA) is an experiment to test the phenomenon of neutrino oscillations. It exploits CERN Neutrinos to Gran Sasso (CNGS), a high-intensity and high-energy beam of muon neutrinos produced at the CERN Super Proton Synchrotron in Geneva, Switzerland, and pointing to the Laboratori Nazionali del Gran Sasso (LNGS) underground laboratory, 455 miles (730 kilometers) away at Gran Sasso in central Italy.