... From the chain visibility point of view, it is very recommended to look at the Javascript movies , especially if the frame rate can be not regulated in your MPEG player. ... The non-CH-associated large-scale chains visible on the SOHO/EIT images at three wavelengths of 171, 195 and 284 as well as on the MLSO/HAO He I 10830 spectroheliogram of December 16, 1997. ... The SOHO/EIT movies at 171 and 195 show the chain dynamics on June 1-3, 1998. ... Javascript movie (230 KB), SOHO/EIT, 171 . ...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

Next: The Quasi--Newton Method. Up: Outline of the Previous: The Newton--Raphson Method. ... At each iteration, one computes . ... Neglecting the second derivatives matrix , we obtain the ``normal equations'' and the Gauss--Newton direction . This so--called Gauss--Newton method is intended for problems where is small. ... The algorithm implemented here is a modification of that Gauss--Newton method, that allows convergence even for rank deficient Jacobians or for large residuals. ...

XMM-Newton Science Analysis System . ... CORR_RATE - The count rate after the following corrections have been applied; . 1) A further point-spread function correction may be applied, to extrapolate the counts from 12 to 35 pixels (presently only done for UV observations) 2) Correction for dead-time. 3) Correction for the OM sensitivity-degradation. A key-word TDS_CORR is added to the table to record the correction value. ... XMM-Newton SOC/SSC -- 2008-07-02 ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Low cost beginner eyepieces. Send SASE for price list. ... Listed Since October 26, 2004 . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

Home - News - Download - Documentation - Search - FTP . About NEdit . ... Download . Get NEdit . ... nedit man page . ... Mirror Sites . ... Christian Denat . ... Back ] . ... Select word/line/file ( modified ) . ... Project macros ( modified ) ( new ) . ... Find definition ( new ) ( new ) . Find definition dialog ( new ) ( modified ) . ... Trace IF / ELSE / END IF ( modified ) ( new ) . Fold C/C++ ( modified ) ( modified ) . ... Element functions ( modified ) [ Back ] . ...

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Geomagnetic disturbances can be monitored by ground-based magnetic observatories recording the three magnetic field components. The global Kp index is obtained as the mean value of the disturbance levels in the two horizontal field components, observed at 13 selected, subauroral stations . ... Geomagnetic activity is the occurrence of K variations. ... But K still remains a local index, describing disturbances in the vicinity of each observatory. ...

... Parent Directory 04-Apr-2014 22:30 - He2-10a_obs.txt 04-Apr-2014 22:30 18k He2-10b_obs.txt 04-Apr-2014 22:30 18k IC3639_obs.txt 04-Apr-2014 22:30 27k IRAS08339+6517_obs.txt 04-Apr-2014 22:30 34k IZw18-NW_HIIR_obs.txt 04-Apr-2014 22:30 25k IZw18-SE_HIIR_obs.txt 04-Apr-2014 22:30 25k IZw18_obs.txt 04-Apr-2014 22:30 25k NGC1068-knot2_obs.txt 04-Apr-2014 22:30 40k NGC1068-pos1_obs.txt 04-Apr-2014 22:30 ...

... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...

. Comment on J1842+7946 . Comparing the brightnesses of the two main features seen in our 5 GHz image with higher frequency VLBI images available in the literature (at 8.4 GHz from the USNO database and at 15 GHz by Kellermann et al. (1998)), one can conclude that the NW component has a steeper spectrum since the SE one becomes relatively stronger as the observing frequency increases. VLBApls home page . Last modified: 16 Oct 2000

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... ISS Russian Segment . Steps of ISS Assembly . ... Five new devices of the total mass of ~42 kg (instead of 6 devices of the total mass of ~101 kg) are installed in the guidance, navigation and control system of the new series vehicle. ... liquid thermostatting of GN OC devices is provided by installation of three cold plates in the vehicle instrument module (IM); . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

... The IRAF environment provides three coordinates systems: . physical: image pixel coordinates used in the reference (original) image. logical: image pixel coordinates, relative to the current section and size of the image. ... 22:13:53.7 44:28:53.9 - the usual representation of RA, Dec . ... Logical, physical and world coordinate systems are all supported in the PROS software, and regions can be specified with any combination of them. ... c 22:13:53.7 44:28:53.9 8 . ... physical: 6930 9390 240 . ...

... Galaxy Evolution home . Cavendish Astrophysics . Cavendish Laboratory . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . Radio sources and their environments . ... Publications . ... Submitted . ... Calendar . ... Paul Alexander . P.Alexander@mrao.cam.ac.uk . ...

... gradients dependencies on solar wind parameters and IMF; . ... fate of thermal plasma at the dayside magnetopause. velocity-dispersed injections of the thermal and superthermal ions from LLBL at cusp and cleft (lowest energy VDIS-2 events); . ... outer cusp processes, role of outer cusp indentation, plasma entry (laminar reconnection, turbulent diffusion, others), role of turbulent boundary layer; . how is the magnetosheath plasma heated near magnetopause and cusp? . ... cusp/cleft wave emissions. ...

Name Last modified Size Description . Parent Directory - JOBS_HEALTH 10-Apr-2016 00:00 1.6K JOBS_NAVBAR 10-Apr-2016 00:00 1.2K JOBS_TREND 10-Apr-2016 00:00 4.3K crontab_giraffe 10-Apr-2016 00:00 4.1K .

. In this image, the colors and contrasts were modified to emphasize the planetтАЩs atmospheric features. The winds in NeptuneтАЩs atmosphere can reach the speed of sound or more. NeptuneтАЩs Great Dark Spot stands out as the most prominent feature on the left. Several features, including the fainter Dark Spot 2 and the South Polar Feature, are locked to the planetтАЩs rotation, which allowed Karkoschka to precisely determine how long a day lasts on Neptune. Erich Karkoschka

Last modified on March 19, 1997 by A. Richichi . ADC cards and filter/clock box. The ADC card traditionally used with FIRPO I at CA has been used also for FIRP OII in Russia. ... At the same time, the new PCMCIA ADC card (DASCard 1000) has been succesfully installed on the TM-5000 notebook, and used for instance to record the Alpha Tau occultation at Arcetri on March 14, 1997. ... In der Filter/Clock Box war durch den Transport die Leiterplatte abgegangen und hatte einige Kontakte abgerissen. ...

... Dialog box. ... At this point you should explain briefly what happens when changes are made to the options in the dialog box. For example, the following lines explain what happens with the Sparkle Plug-In when the options have been modified by the user: . Changes to the options effect the current image. ... Changes to the various options do not have an immediate effect on the image. ... Here would be the description of what the first option does and how to make changes with it. ...