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1. http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/a_martin.pdf
XMM-Newton Timing Monitoring Antonio Martin Carrillo Tutor: Marcus Kirsch July 24, 2006 Antonio Martin Carrillo 1 Overview XMM-Newton Pulsars Crab pulsar Relative time accuracy 2 epoch folding Conclusions Next steps Antonio Martin Carrillo 2 XMM-Newton · Launched in December 1999 · 3 independent CCD cameras called EPIC (European Photon Imaging Camera) · 2MOS and 1PN ...
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Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/a_martin.pdf -- 322.8 Кб -- 16.08.2006
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2. NSSC-I stored command processing
Command execution times have one second resolution . ... By convention, does not execute any commands which reconfigure SI hardware . Can shut off entire processor, cannot shut off by SI . ... Common Pool Command sequences (RTCSs) are routinely loaded from the ground . Some Common pool sequences are used for one-time execution (e.g. for a single exposure) . Some Common pool sequences are permanently on-board . ... Previous slide . Next slide . Back to first slide . ...
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Ссылки http://www.stsci.edu/hst/training/events/HowHSTWorks/SSD990225/tsld027.htm -- 2.7 Кб -- 23.12.2007
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3. http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2014.1.05/22Apr2014/spectral/TargetImages/20140422_160644/log_20140422_160644.txt
Start Data Acquisition - Selected Wavelengths - 22/Apr/2014 16:06:46.063 Observation Type - Target Images - 22/Apr/2014 16:06:46.088 22/Apr/2014 16:06:48.128 Begin Iteration #1 of 2 - Number of Frames : 17 - 22/Apr/2014 16:06:48.144 Filter : 6563 (Position 3) | ... Acquisition Time : 22/Apr/2014 16:06:48.273 | ... ExpTime (sec) : 0.030 | Stokes : I Filter : 6563 (Position 3) | ... Stokes : I Begin Iteration #2 of 2 - Number of Frames : 17 - 22/Apr/2014 16:06:50.942 Filter : 6563 (Position 3) | ...
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Ссылки http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2014.1.05/22Apr2014/spectral/TargetImages/20140422_160644/log_20140422_160644.txt -- 7.5 Кб -- 22.04.2014
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- http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2014.1.05/22Apr2014/spectral/TargetImages/20140422_161603/log_20140422_161603.txt
- http://www.arcetri.astro.it/~gcauzzi/SOLARNET/SN.2014.1.05/22Apr2014/spectral/GridImages/20140422_162807/log_20140422_162807.txt
- http://www.arcetri.astro.it/~gcauzzi/SOLARNET/24_april_2014/ibis/GridImages/20140424_180337/log_20140424_180337.txt
4. tickadj - set time-related kernel variables
... The particular variables it is concerned with are tick , which is the number of microseconds added to the system time during a clock interrupt, tickadj , which sets the slew rate and resolution used by the adjtime system call, and dosynctodr , which indicates to the kernels on some machines whether they should internally adjust the system clock to keep it in line with time-of-day clock or not. ... Set the kernel variable tickadj to an internally computed "optimal" value. -t tick . ...
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Ссылки http://www.sai.msu.su/~er/xntp/tickadj.html -- 4.0 Кб -- 21.12.2007
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5. http://zebu.uoregon.edu/~uochep/docs/docs01/TALKintersite.pdf
... Top 5: Livingston; bottom 5: Hanford Output from 560-580 Hz band: timing good to about 50 ms. fourth order butterworth filter 100.0 80.0 60.0 40.0 Relative Units 20.0 0.0 -20.0 -40.0 -60.0 -80.0 coincidence level H0:PEM-MX_V1 H0:PEM-MX_V2 H0:PEM-LVEA2_V1 H0:PEM-LVEA2_V2 H0:PEM-LVEA2_V3 L0:PEM-EX_V1 L0:PEM-EX_V2 L0:PEM-LVEA_V1 L0:PEM-LVEA_V2 L0:PEM-LVEA_V3 - 100.0 0.0 200.0 400.0 600.0 800.0 ... Time window of 25 bins gives 83 five sigma events in 10 hours. ...
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Ссылки http://zebu.uoregon.edu/~uochep/docs/docs01/TALKintersite.pdf -- 962.7 Кб -- 14.09.2001
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6. MAO NASU :: Topic: The third-order space-by-time relation (1/1)
... Recent Topics . ... MAO main . ... The third-order space-by-time relation . ... Тема: The third-order space-by-time relation . ... The mass m experiences a gravity force toward the sun and . ... will experience the Coriolis force or Coriolis acceleration. ... differentiated space-by-time twice and discovered equation2. ... time differentiation of space-by-time. ... to be described by differentiated forces. ... third-order space-by-time relation. ... understand the third-order space-by-time relation....
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Ссылки http://www.mao.kiev.ua/index.php/ua/forum/info/193-the-third-order-space-by-time-relation -- 24.4 Кб -- 11.04.2016
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7. Historical Notes
Next: RELATED WORK Up: INTRODUCTION Previous: INTRODUCTION . ... In 1985, Grossman and Paulgrossmann-paul rigorously formulated some of these important ideas in terms of affine canonical coordinate transformations to a coherent space representation. ... In 1989 and early 1990, we formulated the chirplet transform, a multidimensional parameter space whose coordinate axes correspond to the pure parameters of planar affine coordinate transformations in the time-frequency plane. ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Chirplet.dir/node2.html -- 9.1 Кб -- 15.04.1998
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8. http://observ.pereplet.ru/images/GRB081102/grb_film.html
... 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., ...
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Ссылки http://observ.pereplet.ru/images/GRB081102/grb_film.html -- 8.2 Кб -- 01.10.2012
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9. Linux I/O port programming mini-HOWTO: High-resolution timing
... First of all, I should say that you cannot guarantee user-mode processes to have exact control of timing because of the multi-tasking nature of Linux. ... However, for most applications using I/O ports, this does not really matter. To minimise this, you may want to nice your process to a high-priority value (see the nice(2) manual page) or use real-time scheduling (see below). ... Linux 2.x kernels have soft real time support; see the manual page for sched_setscheduler(2) for details. ...
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Ссылки http://mavr.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-4.html -- 8.3 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-4.html -- 8.3 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-4.html -- 8.3 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-4.html -- 8.3 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-4.html -- 8.3 Кб -- 02.10.2012
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10. High time resolution bin-mode observations
Next: Pulsar bin-mode observations Up: ATCA Bin Mode Observations Previous: ATCA Correlator Bin Modes . Miriad 's atlod task has an option, options=hires which converts a RPFITS file observed in high time resolution bin-mode into an apparently normal dataset with fine time resolution. ... In high resolution time mode, the time difference between consecutive integrations might be smaller than this tolerance. ... Miriad manager . ...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node220.html -- 3.9 Кб -- 10.04.2016
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11. Time Series Analysis of Unequally Spaced Data: Intercomparison Between
... Previous: Determination of Variable Time Delay in Uneven Data Sets . ... It is shown that the likeness of the periodogram and the LS-spectrum (both estimators of the power spectrum are widely used in the spectral analysis of time series), depends on the properties of the spectral window corresponding to the distribution of time points. ... Present day theory and practice of the spectral analysis of unequally spaced time series are based on two approaches. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/vityazevv1.html -- 12.9 Кб -- 23.06.1998
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12. Lynxx Time Sheet
. Next: PC To VAX Up: Help Sheets For Previous: Help Sheets For . When using the PC out of the WINDOWS mode, use this conversion sheet to run the Lynxx camera. To get any time that is not printed here, you can add, subtract, multiply and divided at will to get the desired time. i.e.) 2.5 min=2 min+30 sec= 456+114=570 so you would type in 570 for a 2.5 min exposure. You must be out of windows for these times to work. Scott J. Wolk . Mon Nov 25 15:41:03 EST 1996
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/node82.html -- 2.8 Кб -- 01.10.2012
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13. Basic principles of time series analysis
Next: Signals and their Up: Time Series Analysis Previous: Introduction . The practical problems in the analysis of time series concern . the detection of a signal against noise, . the estimation of the parameters characterizing the signal, and . the presentation of the results. Presentation and/or evaluation of the results involves a function of the time series called statistics. ... Signal detection . ... Time domain analysis . Presentation and inspection of results . ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node223.html -- 3.8 Кб -- 23.02.1996
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14. Cosmic ray variations sites
Neutron Monitors ] [ Solar Neutrons ] [ Muon Telescopes ] [ Base Potchefstroom University ] [ Magnetometers ] [ GPS systems ] [ Ionosphere ] [ Related Data ] [ Space Weather ] . ... All Cosmic Ray Stations + InterPlanetary Data: WorldNet . Alma-AtaB (Mt.Tien Shan) DataBase of Kazakhstan Spectrograph Alma-AtaB (Mt.Tien Shan) new . ... Nagoya Muon Telescope and DATA or mail . ... Belgrade Muon Telescopes and DATA or ">mail . ... Real-Time database for Cosmic Ray Anisotropy (DB10) . ...
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Ссылки http://cgm.iszf.irk.ru/irkt/links.htm -- 27.0 Кб -- 25.06.2012
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15. GALFA Integration Times
... All seven spectrometer boards are synchronized together by the observatory 1 PPS tick and the observatory 100 MHz clock. Integration time for both the coarse and fine spectrometer is 0.9863168 seconds (860 frames). A frame is the time for one spectra from the fine spectrometer: . ... 100 MHz . ... During each integration, 860 fine resolution spectra are added together, and 385280 coarse resolution spectra are added together (860 * 14 * 8192/256 = 385280) . ...
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Ссылки http://www.naic.edu/alfa/galfa/docs/galspect/system/integration.html -- 2.4 Кб -- 26.08.2004
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16. MAKEPRFCORR (Nov98) --- nictools --- MAKEPRFCORR (Nov98)
makeprfcorr -- Compute the pixel response function for an image created with asncombine makeprfcorr association . association . ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/makeprfcorr.hlp.html -- 2.6 Кб -- 06.06.2006
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17. http://www.gao.spb.ru/english/publ-s/viii-rfs/p011.pdf
The Sun 11 Solar radio bursts study with high spatial and temporal resolution V.A. Alexeev, A.F. Dementyev, B.N. Lipatov, V.F. Melnikov, M.B. Nechaeva, S.D. Snegirev, Yu.V. Tikhomirov Radiophysical Research Institute NIRFI, Nizhny-Novgorod, Russia Theoretical and experimental researches of the energy release fragmentation in solar ares need observations with high spatial 0.01 1 arcsec and temporal 1 ms resolution. ... Several VLBI stations all over the Russia were supplied by this set of equipment. ...
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Ссылки http://www.gao.spb.ru/english/publ-s/viii-rfs/p011.pdf -- 65.3 Кб -- 21.05.2007
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18. Laboratory of spectroscopy of defect structures ISSP RAS
... For SIMS (Secondary Ion Mass Spectrometry) analysis, a solid surface is bombarded by primary ions of some keV energy. ... The subsequent mass analysis of the emitted ions provides detailed information on the elemental and molecular composition of the surface. ... Extremely short ion pulses with a duration below . ... By rastering a fine-focussed ion beam over the surface, like an electron beam in an electron microprobe, mass resolved secondary ion images (chemical maps) can be obtained...
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Ссылки http://www.issp.ac.ru/lsds/en/methods/sims.html -- 10.6 Кб -- 10.04.2016
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19. http://star.arm.ac.uk/~ambn/abstract265.html
HD185510 (=V1379 Aql) is an eclipsing double-lined RS CVn binary containing a K0 III/IV giant and a hot subluminous companion. ... This was sufficient to resolve all four times of contact and, with data from previous work on this system, to derive a solution for the absolute dimensions of the system. ... Neglecting Ly-alpha, an alternative solution of Teff=31000+/-1500 K, log g=6.5+/-0.2, and E(B-V)=0.1+/-0.03 is obtained from the orbital solution below. ...
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Ссылки http://star.arm.ac.uk/~ambn/abstract265.html -- 3.3 Кб -- 15.04.1997
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20. Apache module mod_expires
This module provides for the generation of Expires HTTP headers according to user-specified criteria. ... This module controls the setting of the Expires HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... ExpiresByType . ExpiresDefault . The ExpiresDefault and ExpiresByType directives can also be defined in a more readable syntax of the form: . ... Module: mod_expires . ...
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Ссылки http://neptun.sai.msu.su/manual/mod/mod_expires.html -- 10.9 Кб -- 25.01.2002
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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