Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 158038 (161 сайтов) ---- Время поиска: 0.38сек.   

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf.

1. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf
Magnetic Stars, 2011, pp. 153 ­ 156 Ab out the Dep endence of the Rotation Velo city of CP Stars on the Magnetic Field Glagolevskij Yu. ... Based on the observational data of the average magnitudes of the surface magnetic field strength Bs for a number of chemically peculiar stars we investigate the dependence of the rotation period on the magnetic field. ... Now the periods of rotation P and the average values of the surface magnetic field Bs are known for more than 50 magnetic stars. ...
[ Текст ]  Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf -- 95.3 Кб -- 11.08.2011
[ Текст ]  Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf -- 95.3 Кб -- 11.08.2011
Похожие документы
Еще в разделе: (Показать все результаты (>242) - mavr.sao.ru/ )

2. Is the Crab Pulsar Showing A 60-second Periodic Modulation?
... We Fourier analysed Hubble Telescope Crab pulsar data obtained with the High Speed Photometer in October 1993. A weak modulation at frequency Hz is detected. We found a strong correlation between this result and the Fourier transform result of stroboscopic Crab pulsar data obtained in December 1994 at the 1.82m telescope of Asiago observatory (University of Padua, Italy). ... We found that both data show a weak modulation at the period of 60 seconds. ... The corresponding frequency is Hz . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/cadeza.html -- 12.0 Кб -- 15.06.2005
Похожие документы

3. http://mavr.sao.ru/hq/lizm/conferences/pdf/1991/1992_2_p12-p16.pdf
... SHTOL ' Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz 357147, Russia The investigation of such a phenomenon as the magnetic field variability at long times (years - decennials) is very interesting. If the explanation of the magnetic field variability with rotation period by the oblique rotator model is evident, then the reason of the long-period variability is not clear yet, despite the existence of some assumptions on its nature. ... Fig.2. ... 213 Fig.3. ...
[ Текст ]  Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1991/1992_2_p12-p16.pdf -- 57.5 Кб -- 24.02.2010
[ Текст ]  Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/1991/1992_2_p12-p16.pdf -- 57.5 Кб -- 24.02.2010
[ Текст ]  Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1991/1992_2_p12-p16.pdf -- 57.5 Кб -- 24.02.2010
Похожие документы

4. Concerning Steady State Corotation of the Io Plasma Torus
... In recent years, substantial information concerning the Io torus has been published. ... Explaining the observed steady state rotation of the torus seems to be difficult. The angular velocity of the torus must be in accordance with the celestial mechanics laws, of the same orders as Io's one. ... We wish to straighten out the situation describing the main geometric and kinematic features of the Io torus using a steady state model based on some of Alfven's ideas [Alfven, 1981]. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/papers/iotor/iotor.htm -- 9.5 Кб -- 02.02.1999
Похожие документы

5. http://www.ipa.nw.ru/conference/2002/sovet/PS/GUSEV2.PS
... 8, ``Celestial Mechanics'', 2002 FCN -- period dependence on dynamic characteristics of a lunar core A. Gusev 1 , N. Petrova 1 , N. Kawano 2 , and RISE group 2 1 Kazan State University, Kazan, Russia 2 National Astronomical Observatory, Mizusawa, Iwate, Japan Two modes in a polar oscillation are obtained when a free rotation of the two--layer Moon was studied: 1 PCW = 2\Omega A Am p fffi ё 1 74yr 1 P FCN = \ Gamma \Omega A 2Am ` C c \ ...
[ Текст ]  Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/GUSEV2.PS -- 40.0 Кб -- 19.08.2002
Похожие документы

6. Correlating Spectral Data with Spatial Gain Variations
Next: Quantum Efficiency Correction (a.k.a. Up: ROSAT HRI Recipes Previous: Appearance of new HRI . The mean pulse height analyzer channel (PHA) of a spectral distribution will vary depending on its location on the detector. Below is a method to compare observed data with that of preflight calibration measurements. ... For temporal gain variations, see The HRI Calbration Report . ... Retrieve the gain maps (mean PHA) from anonymous ftp at SAO. ... But don't forget temporal gain variations!] ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node206.html -- 8.2 Кб -- 01.10.2012
Похожие документы
Еще в разделе: (Показать все результаты (>1896) - hea-www.harvard.edu/ )

7. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The formation process of a MBF and the associated BP (No. 1 in Table 1), which is formed by bipolar emergence. The top row gives the BP region as seen in AIA 193 at the indicated time. ... The bottom row shows the normalised AIA 193 lightcurve (left), and the positive (middle) and negative (right) magnetic fluxes obtained in the blue and yellow boxes marked in the top two rows. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2015/685.html -- 6.8 Кб -- 18.01.2016
Похожие документы
Еще в разделе: (Показать все результаты (>2237) - star.arm.ac.uk/ )

8. Magnetic mapping
The magnetic mapping is fulfilled by the magnetic field line tracing from the satellite position up to the Ionosphere (stop trace at the altitude 110 km). ... As a rule the Tsyganenko [1987] external magnetic field model and IOPT = 3 (Kp = 2) are used. ... The output file includes the following information: . ... For example the file with name aa9610d1.geo contains the information corresponding to the aposteriory magnetic mapping for INTERBALL Auroral Probe for the first decade of October 1996. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/descr/mapping.htm -- 4.6 Кб -- 12.05.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/descr/mapping.htm -- 4.6 Кб -- 12.05.1999
Похожие документы

9. Processing OM Image mode data
... OM grism data are obtained as image mode data. However the different nature of this type of data, spectra of the objects in the field of view instead of their "sky" image, makes that a special processing must be applied to the grism images. ... They are concatenated in a perl script, omgchain , which works in a similar way to the image and fast mode chains. ... All necessary corrections are applied to the grism data files. ... As we have pointed out OM grism data are image mode data. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/omg_thread.html -- 15.4 Кб -- 21.08.2006
Похожие документы

10. Polarization properties (transmitted radiation)
Next: Polarization efficiency: size/shape/orientation effects Up: Optical properties of cosmic Previous: The 2175? feature . To model the interstellar polarization one needs to calculate the forward-transmitted radiation for an ensemble of non-spherical aligned dust grains. ... Let non-polarized stellar radiation passes through a dusty cloud with a homogeneous magnetic field. ... The angle between the line of sight and the magnetic field is ( ). ... where the angle is connected with and ( ). ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node5.html -- 24.1 Кб -- 19.11.2010
Похожие документы

11. http://www.izmiran.rssi.ru/~ichertok/Forbush/ECRC12_paper.pdf
... We analyze relations between characteristics of an extended ensemble of Forbush decreases (FDs) caused by CMEs from the central zone of the solar disk during the 23rd solar cycle, on the one hand, and such solar eruption parameter as a summarized unsigned magnetic flux of CME-associated EUV dimmings and arcades, on the other hand. ... FD magnitude Figure 1a shows the relationship between the magnetic flux and the FD magnitude AF for events unambiguously identified with concrete solar eruption. ...
[ Текст ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/Forbush/ECRC12_paper.pdf -- 373.2 Кб -- 15.05.2012
Похожие документы

12. http://www.gao.spb.ru/english/personal/malkin/publ/zm131.pdf
... In result, we obtained the GA constant. ... So, we use the results of the observations of Galactic ob jects to improve A. Our previous estimate of the GA constant (Malkin 2011) yields the values of R0 = 8.2 kpc, 0 = 29.5 km s-1 kpc-1 , and A = 5.02 µas/yr. ... So, the results published in 2008­2013 were used to derive the final estimate of the GA constant. ... We have applied several statistical techniques mostly used in physics and metrology to these data, as described in Malkin (2012, 2013). ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm131.pdf -- 40.5 Кб -- 02.01.2015
Похожие документы

13. Determination of the 'diffusion coefficient'.
Next: Determination of the stellar Up: Results. ... Their values taken from Lipunov (1992) are shown in table 1. ... For Vela X-1 and Her X-1 values of magnetic field, B , coincides with the values that we used when radii of NS's are and correspondently. ... Characteristic time for the wind-accreting systems can be determined from the equation: . ... These velocities are close to obtained using estimates of the 'diffusion coefficient'. These characteristic time scales are also shown in table 3. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/html/publications/sissa065/node3.html -- 5.6 Кб -- 21.06.1996
Похожие документы

14. Method of search of flare current sheets in the magnetic field obtained by MHD
. Секция «Солнце» . Предварительная повестка дня . Пятница,   29 мая . 14:00–14:15 А. И. Подгорный, И.М. Подгорный.   Солнечная вспышки – модель и сравнение с наблюдениями. 14:15–14:30   Ю .В. Думин , Б.В. Сомов. Топологическое инициирование быстрого магнитного пересоединения . 14:30–14:45 П.А.   Грицык ,   Б.В. Сомов. Модель толстой мишени с обратным током и современные наблюдения солнечных вспышек. 14:45–15:00 Н.П.   Колесников, С.И. Безродных, Б.В. Сомов. Расчет течений плазмы в приближении сильного
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/EAAS/rus/confs/sun.htm -- 31.9 Кб -- 22.05.2015
Похожие документы
Еще в разделе: (Показать все результаты (>68) - sai.msu.ru/ )

15. Joint Processing of Radio Data Produced by the SSRT Together With Data of Other
... Up: Data Analysis and Processing Techniques . ... Some techniques and a set of IDL programs and routines were developed to process data obtained by the Siberian Solar Radio Telescope (SSRT) together with data of other spectral ranges. ... Thus, the study of the solar activity based on the radio observations suggests the involvement of multi-spectral data. ... We present a set of IDL programs and routines which process data obtained by the Siberian Solar Radio Telescope (SSRT) (Smolkov et al. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/grechnevvv2/ -- 16.3 Кб -- 16.07.1999
Похожие документы

16. The magnetic fields of neutron stars
Next: Radio pulse characteristics Up: An overview Previous: The structure of neutron . Typically Gauss for normal pulsars . Consistent with flux conservation during stellar collapse . ... Gravity dominates stellar structure . B field dominates exterior . Stellar surface is so small that observed emission is dominated by the magnetic field. ... Only field lines inside light cylinder are closed . Particles are constrained move along field lines . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/pulsar/Tutorial/tut/node11.html -- 4.1 Кб -- 04.02.2013
Похожие документы

17. http://www.sao.ru/cats/~satr/RFSymp/abs/09_Efimov.ps
THE STUDY OF A MAGNETIC FIELD STRUCTURE IN BLAZAR JETS BY OPTICAL PHOTOPOLARIMETRIC DATA Yu.S. Efimov 1 , E.Yu. ... Besides the Faraday rotation of polarization plane there are observational param­ eters which are connected directly with the intensity of magnetic field and its structure: a polarization degree and a spectral index. ... Moreover, such a comparison allows to follow the variations of the magnetic field intensity from observed variations of polarization degree and spectral index. ...
[ Текст ]  Ссылки http://www.sao.ru/cats/~satr/RFSymp/abs/09_Efimov.ps -- 62.0 Кб -- 09.10.2006
Похожие документы

18. http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/plates2.pdf
New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...
[ Текст ]  Ссылки http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/plates2.pdf -- 1667.0 Кб -- 05.01.2013
Похожие документы

19. http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf
... 2009) 0 Fig.1 · Max-Planck-Institute for Radioastronomy, Bonn , VLBI ESO, COMPONENTS PARAMETERS FROM INTERFEROMETRY · Following S.Kraus et al. ... Using i=105o , we obtain v sini = 32 km/s. BEST MODEL FIT 1OriC 1 · Mass, M · Luminosity, log L · Radius, R · Teff, K · log g · Equatorial rotation velocity, km/s · Magnetic field , G · The time of life, yrs 35.8 5.20 10.0 37000 4.01 5.4 500-1500 150 000 1OriC 2 10.0 4.69 8.2 30000 3.60 96.2 moves to MS 1 OriC ...
[ Текст ]  Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf -- 453.0 Кб -- 26.01.2011
Похожие документы

20. IBIS - Flat Fielding
IBIS Data Analysis . ... IBIS . ... Flat Fielding - Introduction . The images obtained by IBIS will have intensity variations across the field of view that are not due to the solar image, but rather caused by instrumental effects that alter the observed intensity in each point of the field of view. ... IBIS Flat Fielding Techniques . ... Therefore, it is desirable to obtain the flat field measurements center on a point along the equator near the heliographic center of the solar disk. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solare/IBIS/flat.fields.html -- 13.5 Кб -- 01.09.2003
Похожие документы

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | След.


Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда

Rambler's Top100 RFBR Яндекс цитирования