... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . ... rotatelogs is a simple program for use in conjunction with Apache's piped logfile feature. It supports rotation based on a time interval or maximum size of the log. ... For example, if the rotation time is 3600, the log file will be rotated at the beginning of every hour; if the rotation time is 86400, the log file will be rotated every night at midnight. ... date and time (localized) . ...

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• Solar System Cosmology
• Reading the Data
• Magnetic-field orientation

Precession/Nutation Solution Consistent with the General Planetary Theory . ... In the present paper the equations of the translatory motion of the major planets and the Moon and the Poisson equations of the Earth's rotation in Euler parameters are reduced to the secular system describing the evolution of the planetary and lunar orbits (independent of the Earth's rotation) and the evolution of the Earth's rotation (depending on the planetary and lunar evolution). ...

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• Annotation_157
• list1
• Keywords_145

Magnetic Fields around Radio Galaxies Robert Laing (ESO) Laing et al. ... 2008) Negligible depolarization and 2 rotation Almost all Faraday effects must be due to foreground material How to fit depolarization caused by foreground Faraday rotation Complex polarization Rotation measure Integrate over a beam Observed RM for 0 2 rotation and depolarization Faraday rotation and depolarization 5.5 arcsec FWHM Faraday effects at high resolution FWHM = 1.5 ...

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• http://www.mrao.cam.ac.uk/~mh475/poster.pdf
• http://www.mrao.cam.ac.uk/wp-content/uploads/2014/05/DHomeier.pdf
• De-convolution of a Gaussian beam from planetary observations Bojan Nikolic web

Extended time series of Solar Activity Indices (ESAI) is database including observational, synthetic and simulated sets to study Solar magnetic field variations and their influence on the Earth. ESAI extend the ordinary lengths of some traditional indices of solar activity: sunspot areas, Wolf numbers (equatorial component of magnetic field of the Sun), polar faculae numbers (polar component), mean latitudes, N-S asymmetry of hemispheres (location of activity). Series . ...

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• Journees 2014
• Пашкевич Владимир Витальевич
• Pulkovo database of sunspot magnetic fields

Next: A Universal Diagram for Up: ``Ecology'' of Magnetic Rotators Previous: The Corotation Radius . The interaction of a magnetic rotator with the surrounding plasma to a large extent depends on the relation between the four characteristic radii: the stopping radius, , the gravitational capture radius,   , the light cylinder radius,   , and the corotation radius,   . ... Hence, the classification of the interaction regimes may well mean the classification of magnetic rotators. ...

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• The Corotation Radius
• ``Ecology'' of Magnetic Rotators
• The Environment of the Rotator

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• http://zebu.uoregon.edu/51peg.html
• Astronomy Plus CCD Images of Galaxies
• Astronomy HyperText Book: Planetary Motion

Raquel Salmeron The mechanism(s) responsible for generating the angular momentum transport required for star/planet formation remain poorly understood. ... In recent times it has been realised that the answer may lie in the complex interaction of gas and magnetic fields present in the flattened disc of material that surrounds the star in formation (e.g., Balbus Hawley 1998) . ... COALA : Universe Galaxy AGN Star Planet ...

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• Dopita Papers
• RSAA Honours Courses (2006)
• GSAOI Magellanic Cloud Planetary Nebulae Science Page

... White Dwarf Spectra . ... My conception of a white dwarf with a dusty disk. The dust must sublimate and will accrete onto the surface of the white dwarf, possibly through streamers of gas that follow the white dwarf's magnetic field lines. As in Saturn's rings, there might be streaks in the dust due to material that is darker than the surrounding dust, or perhaps caused by shadows of rocky bodies with sizes larger than the scale height of the disk. ...

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• CSPICE Routines: AXISAR_C
• A Compact Instrument to Detect and Study Seismological Doppler Signals from
• Planetary Nebulae

... B.D. Shelting . ... webmaster@izmiran.ru . ... V.N. Obridko, B.D. Shelting . ... Makarov V.I., Tlatov A.G., Callebaut D.K., Obridko V.N., Shelting B.D. Large scale solar magnetic field and sunspot cycles . Solar Physics, 2001, V.198, 409 . ... Journal of.Atmospheric and Solar-Terrestrial Physics, 2001, 63, 1923-1929 . A.V. Belov, Shelting B.D., Gushchina R.T., Obridko V.N., Yanke V.G. Long-term variations of galactic cosmic rays and the relation to the solar magnetic field parameters . ...

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• Oct-Nov 2003

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 ( ). ...

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• List of publications

A tale of two planets: the history of Earth and Mars compared 4.54 billion years ago 4.527 billion years ago 4.5-4 billion years ago Earth Forms in Sun's proto-planetary disc Collision with other planet; Formation of the Moon Mainly carbon dioxide atmosphere , surface water , molten core and magnetic field Mars Forms in Sun's proto-planetary dis c 4 billion years ... Atmosphere becoming rich in oxygen Earliest life in oceans? ...

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• Kepler-11: a strange and crowded planetary system | Astronotes
• Immanuel Velikovsky's weird astronomical theories | Astronotes
• Kepler-10c: the First Mega-Earth | Astronotes

... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...

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• New concept of cosmogony
• The new circuit of global tectonics of the Earth, planets and satellites.

... 323, P 659-673 (1997). Abstract . ... 323, P 674-684 (1997). ... Number counts and optical identifications of faint IRAS sources . ... 323, P 685-696 (1997). ... 323, P 697-706 (1997). ... 323, P 707-716 (1997). ... 323, P 717-726 (1997). ... 323, P 727-738 (1997). ... 323, P 739-748 (1997). ... 323, P 749-761 (1997). ... The [Fe/H] distribution of a volume limited sample of solar-type stars and its implications for galactic chemical evolution . ... helpdesk@link.springer.de . ...

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• Springer LINK:A&A-EE: Table of Contents Volume 318 Number 2 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 325 Number 3 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 317 Number 3 (1997)

A year is a time interval approximately equal to the period of the Earth's rotation around the Sun. ... 2) a tropical year is a time interval between the Sun's two centre successive passing through the medium point of the vernal equinox (365,2422 days); . 3) anomalistic year is a time interval between the Sun's two centre successive passing through the perihelion of its visible heliocentric orbit (365,2596 days); . ... 6) lunar year includes 12 lunar synodic months (about 354, 367 days); . ...

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• earthe
• timekeepe
• moone

Клуб Скептиков] [Конференция] . ... Прохожий : re: Кое что о Венере.. ... Вероятно он Венеру с Ураном перепутал. ... Venus Earth . Sidereal rotation period (hrs) -5832.5 23.9345 . ... Любопытствующий Венера Прохожий re: Венера 13-Ноя (17:10) Любопытствующий re: Венера 14-Ноя (06:20) Alex re: Венера 14-Ноя (10:32) Любопытствующий re: Венера 14-Ноя (14:22) Артем re: Венера 15-Ноя (18:28) Любопытствующий re: Венера 16-Ноя (12:29) Артем re: Венера 16-Ноя (13:47) . ...

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The Laboratory of Electronic Kinetics ( LEK ) has powerful radio-frequency, microwave , cryogenic and high- magnetic - field sets of equipment , allowing to carry out precision phase-sensitive measurements of current and voltage in a frequency range 0-10 MHz and the microwave response of crystalline materials in cm-and mm- wavelength range in the temperature interval (0.1-300) K and in magnetic fields up to 18 T. Methodical principle of ... Magnetic field up to 18 T . ... Equipment . ...

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• LHPP ISSP RAS
• SPECIALITY 01.04.07 - CONDENSED MATTER PHYSICS ADMISSION EXAMINATION PROGRAM
• SPECIALITY 01.04.07 - CONDENSED MATTER PHYSICS HIGHER CERTIFICATION COMMITTEE

ARCSAT ID NUMBER: AS04 DESCRIPTIVE TITLE: Constraining the magnetic fields of transiting exoplanets through ground-based near-UV observations PI: Jake Turner OBSERVER(S): Jake Turner (Graduate Student: University of Virginia) Apurva Oza (Graduate Student: University of Virginia) Robin Leiter (Undergraduate Student The magnetic field of a transiting exoplanet can be constrained by observing asymmetries in their near-UV light curves (Vidotto, Jardine Helling 2011a; Vidotto et al. ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS09.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS08.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2015/AS02.html

... 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 ...

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• http://hea.iki.rssi.ru/conf/hea2010/Presentations/21/Levin.pdf
• http://hea.iki.rssi.ru/conf/hea2010/Presentations/22/Tsupko.pdf
• Гусев Анатолий Александрович (ИКИ РАН)

... In typical nightly use, the wide field and planetary telescope and cameras record images of favorably placed objects in the sky, including constellations, bright variable stars, nebulae through narrow-band filters, comets, the Moon, and planets. ... Shared Skies telescopes are available for use by students at the University of Louisville and the University of Southern Queensland, and by teachers and students in middle and high schools mentored by faculty at the universities. ...

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... Departments . ... Dept. for Physics of Stars&Galaxies . ... Dept. for Physics of Planetary Systems . ... Solar telescopes . ... 2016,MNRAS, 2016MNRAS.tmp.. ... The Department for Physics of Planetary Systems . ... In May 1967 the department for Physics of the Moon and Planets ; was created, it was led by Dr.Sci. ... In 1984, the department was renamed to the Department for Physics of the solar system bodies . ... In 2013 the department was renamed to the Department for Physics of planetary systems ....

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• Activity - Page 2
• Cooperation - Page 3
• Dept. for Astrometry & Space Geodynamics