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1. Pulsar Group PmWiki/Available Actions
... PmWiki . Summary: PmWiki group header. ... Summary: All PmWiki page actions (?action=) and other query parameters:) . ... Cookbook actions . ... See also site page actions . ... displays dialog for setting/changing password of the specified page or group of pages, see passwords , see also $EnablePostAttrClearSession if you do not want to have the session cleared after validating change { PmWiki /Passwords$:Summary} . ... edit the specified page, see basic editing { PmWiki/BasicEditing $:Summary} . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/pulsar/index.html?n=PmWiki.AvailableActions -- 34.1 Кб -- 01.03.2014
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2. The Effect of Relativistic Wind on Accretion Flow Parameters
... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node56.html -- 10.8 Кб -- 26.02.1997
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3. How precise are the parameters of my double star as measured in Transfer Mode?
... HST . How precise are the parameters of my double star as measured in Transfer Mode? ... Data . ... HST Peer Review Process . ... HST Overview . Overview . ... Retrieving HST Data . ... Data Analysis . ... HST Science Year in Review . ... FGS Data Handbook . ... A: Analysis of calibration and other data has shown that the separations obtained in the analysis the Transfer Functions of double stars have a precision of around 1 milli arc-second. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/fgs/faqs/measure2.faq -- 14.7 Кб -- 10.04.2016
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4. Documentation: LEDA: parameter: m21c
The HI line magnitude m21 has been corrected for self-absorption effect following Heidmann et al (1972) , with parameter kappa=0.031. The inclination needed to compute this correction is given as parameter incl . If inclination is higher than 89 deg the maximum correction is limited to -0.82 mag. Corrected flux at other wavelengths are given in the parameters: bt , it . The measured HI flux is m21 .
[ Сохраненная копия ]  Ссылки http://www.sao.ru/fetch/HL/leda/param/m21c.html -- 2.3 Кб -- 23.12.2013
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5. User-level errors and warnings
... Meta Index / Home Page / Errors . ... warning . ... For instance, if the PROPOSAL information record is missing the user can add a fake one to the SOSF without this having any effect on the data reduction. corrective action: Continue. ... For a certain exposure in the ODF one of the parameters was not found in the housekeeping data. ... RGS, EPN, OM : the current exposure is found to contain more than one distinct calibration mode. corrective action: In the summary file: MODE = UNDEFINED . ... error...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/odfingest/node16.html -- 15.0 Кб -- 08.07.2007
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6. East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...
[ Сохраненная копия ]  Ссылки http://rp.iszf.irk.ru/esceir/isr/ismodelen.htm -- 5.9 Кб -- 04.06.2001
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7. Space Research Institute (IKI) Seminar
... Future seminars . ... Relativistic magneto-active laser plasmas " . ... Generation of super-strong magnetic fields. ... This method is based on the observation of resonance interaction between the Landau levels in magnetic field and energy levels of plasma ions. ... The important peculiarity of the energy distribution of fast ions is their slow decreasing up to the energy of 1.4 MeV at the laser intensity of 2 10 18 W/cm 2 ; the effective temperature of fast ions is of the order of 350 keV. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/galeev/abs_eng/e120426.htm -- 57.5 Кб -- 18.04.2012
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/galeev/abs_eng/e120426.htm -- 57.5 Кб -- 18.04.2012
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8. A Python-based IRAF Task Parameter Editor
... As part of the development of a new Python-based CL for IRAF tasks by the Science Software Group at STScI, we have developed a GUI-based parameter editor for IRAF tasks using Tkinter. This new parameter editor is intended to provide the equivalent functionality of the IRAF EPAR task, but to make parameter editing easier by using appropriate user interface elements, such as menu choice lists, action buttons, and file browsers. ... Figure 1: The GUI-based Python/Tkinter IRAF task parameter editor. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P1-54/ -- 11.1 Кб -- 06.10.2000
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9. http://www.mso.anu.edu.au/~brian/A3002/lect11.pdf
... So at T 10 at T=10 10.5 (t 0.2s) 10.5 (t = 0.2s) (t 0.9s) So at T~10 10.14 End up with mainly protons, neutrons and electrons (some neutrinos) when Universe is 1 second old With ratio of N/P set as Neutrons decay with half-life of 887 seconds Formation/Destruction of Deuterium Neutrons converted to D at roughly 200s From Saha equation (but Neutron Except those neutrons that decay .. ... A bit less 28%*exp(-100s/900s) =24% when one takes into account neutron decay.. ...
[ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/lect11.pdf -- 1254.2 Кб -- 23.10.2006
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10. ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3
ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3 . ... The major objective of the P3-3 experiment is complex investigation the main parameters of ionospheric plasma with high time and spatial resolution. ... Measured parameters: . ... The experiment produce regular data - measured with fixed time interval and «packet» data - measured once per specific time interval and producing blocks of TM-information. ... If all parameters will be measured once per second, the experiment will produce 10 MB per orbit. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/projects/warning/p3-3.html -- 6.2 Кб -- 15.02.2000
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11. OptInt PmWiki : PmWiki / Debug Variables
OptInt PmWiki : Pm Wiki / Debug Variables . Basic Variables | Variables | ... EnableDiag . The following actions are available only if you set $EnableDiag = 1; in your configuration file. They can be used for debugging and should not be set in a production environment. ?action= ruleset . ... If you have a wiki that composes a HTML page from multiple pages, such as a normal layout with a sidebar, you'll get separate timings for each subpage and for the total page.) ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/PmWiki/DebugVariables?action=print -- 13.5 Кб -- 01.03.2014
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12. Cosmological parameters constraints
... WMAP7 -- 7 year WMAP data ( Larson at al., ... SPT -- CMB power spectrum from SPT ( Keisler et al., ... CDM -- flat Universe with cosmological constant . ... N eff 3.046 . ... WCDM -- flat Universe with dark energy . ... CDM, WMAP7+BAO+H0 +CL . CDM, WMAP7+BAO+H0+SPT +CL . ... CDM+f (1), WMAP7+SPT+BAO+H0 +CL . CDM+f (1)+N eff , WMAP7+SPT+BAO+H0 +CL . ... CDM+N eff , WMAP7+BAO+H0 +CL . ... CDM+dn/dlnk, WMAP7+BAO+H0 +CL . ... WCDM, WMAP7+SPT+BAO+H0 +CL . ... WCDM, WMAP7+SPT+BAO+H0+SNSYS +CL . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/x-ray-clusters/cosm/combined/en/ -- 7.1 Кб -- 02.10.2012
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13. S.P.Korolev RSC Energia - ECOLOGICAL MONITORING
AUTOMATIC STATION OF ECOLOGICAL CONTROL . ... BASIC PERFORMANCE SPECIFICATION . STATE OF ASEC DEVELOPMENT . AIR POLLUTION MONITORING . ... OF MEASURING CHANNELS . ... unit of measurement . ... Nitric oxide (NO) concentration, . ... power measured by ASEC . ... In particular, RSC Energia finalizes its work on measurement systems designed to measure dust, volumetric activity of radioactive gases and aerosols and other environmental parameters. ... Official WEB-site of S.P.Korolev RSC Energia . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/eng/conversion/ecology/metrology.html -- 14.2 Кб -- 02.10.2012
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14. Determination of the Detector Parameters
The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/desc/det_per.html -- 5.0 Кб -- 16.02.2000
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15. Cosmological Issues for Theorists
. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/cosmo.html -- 6.5 Кб -- 19.04.1999
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16. Solar modeling input physics (thermodynamics, opacity, nuclear reactions)
On this page you can compute thermodynamics, opacity and nuclear reaction rates for conditions which exist inside the Sun. ... Logarithmic partial derivative dlogP/dlogT (hi_t) . Logarithmic partial derivative dlogP/dlogRHO (hi_rho) . Logarithmic partial derivative dlogP/dlogX (hi_x) . Logarithmic partial derivative dlogU/dlogT (ksi_t) . ... Input field size does not limit the amount of data entered; you can type or paste thousands of lines (10,000 lines tested with output size over 5MB). ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/physics/phys.php -- 6.3 Кб -- 01.10.2012
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17. ALFA Performance
... Recent Band Averaged Measurements . Gain, SEFD, Tsys, and Beam width . ... This is the band averaged Gain, SEFD, Tsys, and Beam width for ALFA taken at regular intervals. ... For performance figures as a function of frequency, see the ALFA spectral scans . ALFA spectral parameters & calibration . ... The fit parameters for the spectral scans can be downloaded. ... Details are given in the memo by Desh: ALFA spectral parameters & calibration . ... Spectral scans across the full ALFA band. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/alfa/performance/ -- 7.2 Кб -- 01.10.2012
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18. Working with
Next: In case of trouble Up: Using Previous: What to do next? ... procedures are called from within the IDL environment. This is done from either the IDL command line by typing in the appropriate commands, or by invoking a widget, which provides buttons to click on for specific action. ... Note that widget buttons which bring up another widget are labeled in all caps, whereas the other type either displays a sub-menu (indicated by the arrow) or executes a procedure upon selection. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node14.html -- 6.4 Кб -- 28.04.2015
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19. Biosphere: Analysis of Value Parameters
... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/resources/sotrudniki/sosnina/mono14/ -- 80.9 Кб -- 10.04.2015
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20. Determination of atmospheric parameters and calculation of chemical composition
... We cannot use for this purpose equivalent widths and profiles of HI lines (well known criteria of atmospheric conditions for normal supergiants), since these lines are strongly distorted in the spectrum of IRAS04296 as seen in Fig. ... Figure: Upper: iron abundance FeI (circles) and FeII (crosses) calculated for IRAS04296+3429 with model parameters , and using lines with different excitation potentials EP of a low level; bottom: the same as a function of the equivalent width W . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/IRAS04296/node7.html -- 28.8 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node7.html -- 28.8 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node7.html -- 28.8 Кб -- 01.10.2012
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