Найдено документов: 336860 (178 сайтов) ---- Время поиска: 0.98сек. |
Показаны документы, содержащие фрагменты текста из документа
http://www.iki.rssi.ru/mirrors/stern/earthmag/planetmg.htm.
http://www.iki.rssi.ru/mirrors/stern/earthmag/planetmg.htm.
1. Planetary Magnetism
... The planets differ greatly in size and properties, and their fields differ too. ... In 1959, after the Earth's radiation belt had been discovered, Frank Drake observed Jupiter and concluded from the relative intensities in a range of wavelengths that the signal was probably emitted by electrons trapped in a strong magnetic field. Then in 1973 the space probe Pioneer 10 passed by Jupiter and found there, sure enough, an enormous planetary magnetic field and a very intense radiation belt. ...
[
Сохраненная копия
]
Ссылки http://www.iki.rssi.ru/mirrors/stern/earthmag/planetmg.htm -- 13.1 Кб -- 21.12.2007
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/mirrors/stern/earthmag/planetmg.htm -- 13.1 Кб -- 22.12.2007
Похожие документы
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/mirrors/stern/earthmag/planetmg.htm -- 13.1 Кб -- 22.12.2007
Похожие документы
Еще в разделе:
(Показать все результаты (>1732) - www.cosmos.ru/ )
2. Solar Energetic Particles
... Magnetic Storms . ... Cosmic Rays . ... Energetic Particles . ... Solar fast Particles . We cannot observe the way the distant universe accelerates cosmic rays or produces energetic photons, but acceleration processes also occur on our Sun , though on a much more moderate scale. ... That is why such events are often missed by cosmic ray detectors near the equator, where the lowest energies are excluded by the Earth's magnetic field. ... Should we be concerned about solar energetic radiation? ...
[
Сохраненная копия
]
Ссылки http://www.iki.rssi.ru/mirrors/stern/Education/wsolpart.html -- 12.1 Кб -- 21.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>875) - www.iki.rssi.ru/ )
3. Linear polarization: wavelength dependence
... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...
[
Сохраненная копия
]
Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node7.html -- 18.9 Кб -- 19.11.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>380) - www.astro.spbu.ru/ )
4. Supersonic Motions in the Upper Atmosphere of Jupiter Detected at Ly- with GHRS
... The related observations clearly evidence both global motions and turbulence in the upper Jovian atmosphere. Keywords: solar system, giant planets, atmospheres, Jupiter . To explain both an upper atmospheric thermal excess observed in the Jupiter atmosphere by the Voyager missions and a permanent enhancement of the H Ly- brightness observed near the equator (Clarke et al. ... These Doppler shifts appear as being the signature of global H motions in the upper atmosphere of Jupiter. ...
[
Сохраненная копия
]
Ссылки http://www.stsci.edu/stsci/meetings/shst2/emerichc.html -- 14.5 Кб -- 15.06.2005
Похожие документы
Похожие документы
5. Direct Monitoring of Rotational Modulation
Next: Rotation Periods of ZAMS stars Previous: T Tauri Stars . ... The first attempts to directly measure periodic modulation of T Tauri stars occurred in the early 1980s. Rydgren & Vrba (1983) observed four PMS stars using photoelectric photometry over a period of seven consecutive photometric nights. ... Because the spot lifetime is much longer than the rotational period, the observed effect will be a modulation of the light from the star synchronously with the rotation period. ...
[
Сохраненная копия
]
Ссылки http://hea-www.harvard.edu/~swolk/thesis/intro/node3.html -- 6.4 Кб -- 02.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2143) - hea-www.harvard.edu/ )
6. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p440.pdf
... The results of radio observations of GRB 080319B in the spectral range of 8.45 GHz are presented. ... Key words: Gammarays bursts: observations radio: individual: GRB 080319B 1 Intro duction Gammaray bursts (GRBs) are the most luminous explosions currently known in the Universe. ... Smooth angular scanning was used not only in GRB 080319B observations, but to specify the primary standard source radio flux density as well (Kharinov et al., ...
[
Текст
]
Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p440.pdf -- 765.1 Кб -- 11.08.2011
[ Текст ] Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p440.pdf -- 765.1 Кб -- 11.08.2011
Похожие документы
[ Текст ] Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p440.pdf -- 765.1 Кб -- 11.08.2011
Похожие документы
Еще в разделе:
(Показать все результаты (>324) - mavr.sao.ru/ )
7. http://www.naic.edu/vscience/schedule/tpfiles/BergertagA2005tp.ps
... A2005 Date Received: 2004Sep29 18:51:13 Technical Page Proposal Type: Regular General Category: Astronomy SubCategory: Continuum Observation Category: Galactic Total Time Requested: 42 Hours Proposal Title: The Origin of Magnetic Activity in SubStellar Objects ABSTRACT: The processes of magnetic field generation, amplification and dissipation in substellar objects are not understood, but could provide direct information on the internal convection and the structure of the atmosphere. ...
[
Текст
]
Ссылки http://www.naic.edu/vscience/schedule/tpfiles/BergertagA2005tp.ps -- 95.4 Кб -- 04.11.2004
Похожие документы
Похожие документы
8. SCORPIO: Direct images
Direct images gallery. Here we have presented some images obtained on SAO telescopes by using SCORPIO. ... NGC 6951 . ... This color image are combined from the frames in the filters V ("blue"), R ("green") and middle-band filter SED755 ("red"). ... The true color image is constructed from three frames in B (Texp=600 sec), V (Texp=480 sec) and R (Texp=400 sec) filters. ... The true color image is constructed from three frames in B (Texp=180 sec), V (Texp=120 sec) and R (Texp=90 sec) filters. ...
[
Сохраненная копия
]
Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_im.html -- 4.5 Кб -- 04.02.2013
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lon/SCORPIO/galleries/gal_im.html -- 4.5 Кб -- 28.02.2014
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_im.html -- 4.5 Кб -- 02.10.2012
Похожие документы
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lon/SCORPIO/galleries/gal_im.html -- 4.5 Кб -- 28.02.2014
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_im.html -- 4.5 Кб -- 02.10.2012
Похожие документы
Еще в разделе:
(Показать все результаты (>985) - jet.sao.ru/ )
9. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/VBourrier.pdf
Magnesium : a new probe of the thermosphere / exosphere region V. Bourrier, A. Lecavelier des Etangs, A. Vidal-Madjar Institut d'Astrophysique de Paris/CNRS, Paris, France Atmospheric escape from HD209458b Transit observations in the Lyman- line of neutral Oxygen, carbon and silicium were also found in its Schlawin et al. 2010), carried away to high altitudes heavy species at high altitude: neutral ... 2003, Nature, 422, 143 Vidal-Madjar, A., DИsert, J.-M., et al. ...
[
Текст
]
Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/VBourrier.pdf -- 1381.2 Кб -- 17.04.2014
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2353) - www.mrao.cam.ac.uk/ )
10. PPTA Dashboard | Log Entry
This page allows the current observer to add to the session log for the current PPTA observing session. To start a new session, click 'start new observing session'. The last observer in the session must end the session by clicking on 'finish current observing session' - the observer will be redirected to a form. ... Current observer: . ... Note that all windparks, failures etc. should also be recorded through the standard observing webpages (click on "Links" tab at the top of the dashboard) . ...
[
Сохраненная копия
]
Ссылки http://www.atnf.csiro.au/research/pulsar/ppta-obs/dashboard/log.html -- 10.9 Кб -- 10.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>27668) - www.atnf.csiro.au/ )
11. Supernova Explosions
Next: Radiopulsars as Sources of Up: Cosmic Rays and Evolution Previous: Cosmic Rays and Evolution . Presently, there is little doubt that galactic CR can be generated at rapidly expanding shock fronts produced by supernova explosions. ... Statistical properties of radiopulsars in our Galaxy indicate a formation rate of NS of about 1 per 10-20 years in the present cosmological epoch, while direct astronomical observations have so far not detected supernova explosions at this high rate. ...
[
Сохраненная копия
]
Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node70.html -- 9.6 Кб -- 03.03.1997
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>554) - xray.sai.msu.ru/ )
12. Procedures for Observations
... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...
[
Сохраненная копия
]
Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/doc/proc_ob.html -- 7.9 Кб -- 16.02.2000
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>9670) - www.arcetri.astro.it/ )
13. ESO - Science Announcements
... Public . Science . ... Science Users Information > Science Publications > Science Announcements . ... ALMA . ... Observing with ESO Telescopes . ... Data Handling and Products . ... ESO Data . ... Science Announcements . ... Published: 18 Aug 2015 . ... New reduced data (spectra and images) resulting from the Public ESO Spectroscopic Survey of Transient Objects ( PESSTO ) are now available via the dedicated Phase 3 query interface at the ESO Science Archive Facility . ... Published: 29 Jul 2015 . ...
[
Сохраненная копия
]
Ссылки http://www.eso.org/sci/publications/announcements.page6.html -- 42.5 Кб -- 09.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>24717) - www.eso.org/ )
14. J.G. Doyle, Research Astronomer
Next: C.S. Jeffery, Research Astronomer Up: Research Previous: J.E. Chambers, Research Astronomer Contents . ... We examine spectral time-series of two lower-chromospheric lines observed with SUMER/SOHO (N I and C II ). ... Two examples of explosive events observed with SUMER/SOHO in transition region spectral lines are reported here; one detected in C IV 1548?, in a region within the northern polar coronal hole, and the other in O VI 1032?, in an active region. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/annrep/annrep99/node12.html -- 14.0 Кб -- 05.05.2000
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3075) - star.arm.ac.uk/ )
15. Publications of Astronomy and Space Physics Department
Verkhoglyadova O.P., V.N. Ivchenko, K. Kudela, M. Slivka, V.N. Lutsenko, S.A. Romanov "Approach to identification of the tail plasma regimes using INTERBALL-1 data" // Czech. ... Yermolaev "Observation of vortical motions and compressional waves in the dawn low-latitude sheet" // Journal of Technical Physics, 1999, v.XL, No 1, p.325-328. ... Martiushov V. "A point explosion inside a cavity with power-law density distribution" // 6 th Open Young Scientists' Conference on Astronomy and Space Physics. ...
[
Сохраненная копия
]
Ссылки http://space.univ.kiev.ua/article/article99.html -- 13.4 Кб -- 23.01.2004
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>137) - space.univ.kiev.ua/ )
16. Spacecraft capture an Earth-directed coronal mass ejection | Astronomy.com
... Observing . ... Spacecraft capture an Earth-directed coronal mass ejection . ... On August 20, 2013, at 4:24 a.m. EDT, the Sun erupted with an Earth-directed coronal mass ejection (CME), a solar phenomenon which can send billions of tons of particles into space that can reach Earth one to three days later. ... Only registered members of Astronomy.com are allowed to comment on this article. ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/news/2013/08/spacecraft-capture-an-earth-directed-coronal-mass-ejection -- 67.9 Кб -- 10.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>6451) - www.astronomy.com/ )
17. TESIS has recorded new sizeable mass ejections from the Sun's atmosphere
... One of this year's largest mass ejections from the Sun's atmosphere was recorded last Sunday by TESIS telescopes aboard the CORONAS-PHOTON satellite ( video - wmv 4.3 MB ). ... Over the course of a week, two gigantic solar prominences were simultaneously ejected from the surface of the Sun. ... Earth will not feel the Sun's influence either. ... The TESIS observatory ї TESIS: www.tesis.lebedev.ru . ... One of this year's largest mass ejections from the Sun's atmosphere (movie WMV, 4.3 MB) . ...
[
Сохраненная копия
]
Ссылки http://www.tesis.lebedev.ru/en/info/mass_ejection_20090614_en.php -- 10.4 Кб -- 01.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>19486) - www.tesis.lebedev.ru/ )
18. Observers Instructions for filling out the ARCSAT nightlog
... The schedule assigned id (example: AS05) for your observing program. ... Use the time you started using the telescope including when you started taking calibrations. The time you opened for on sky observations can be entered later in the activity log. UTC End Time: . ... Focus Log: . ... The focus position can be obtained under the Telescope column of the System Status in ACP or from the run log. ... When all fields are filled out press this button to email the log to the ARCSAT and community. ...
[
Сохраненная копия
]
Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObservingAids/nightlogInstructions.html -- 5.9 Кб -- 16.05.2014
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>584) - www.apo.nmsu.edu/ )
19. http://lnfm1.sai.msu.ru/neb/nss/coorb/coorb_anno.doc
OBSERVATIONS OF COORBITAL SATELLITES OF SATURN Emel'yanov N., Varfolomeev M. Sternberg State Astronomical Institute, Moscow, e-mail : emelia@sai.msu.ru Institut de MИcanique CИleste et de Calcul des иphИmИrides, Paris, e-mail : emelia@imcce.fr Abstract. To improve the orbital parameters and masses of coorbital satellites of Saturn, Janus and Epimetheus, new observations of these satellites are necessary. ... IN: Saturn. ... New observations of Saturn's coorbital satellites" - Icarus. ...
[
Текст
]
Ссылки http://lnfm1.sai.msu.ru/neb/nss/coorb/coorb_anno.doc -- 90.5 Кб -- 15.04.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>521) - lnfm1.sai.msu.ru/ )
20. Accuracy of World positional CCD observations of the numbered minor planets
... Advises . Contact Advises . As an advise for amateurs we would like to underline: if it's possible, try to observe 3 asteroid positions per night and do not neglect to observe the Numbered Minor Planets in your telescope field of view as a "by product" of your observational programs. ... We think such estimations ought to be produced every morning after CCD observations of the moving celestial objects by observer himself. ...
[
Сохраненная копия
]
Ссылки http://www.accuracy.puldb.ru/ADVISES.HTM -- 2.8 Кб -- 05.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>104) - www.accuracy.puldb.ru/ )
Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
Комментарии, вопросы? Пишите: info@astronet.ru или сюда