... A. M. Neminsky, P. N. Nikolaev, and D. V. Shovkun . ... The temperature dependence of the magnetic field penetration depth lambda ( T ) is determined down to 0.2 T c by the ac-susceptibility measurements on the Rb 3 C 60 fine powder with small, about 1 K, variation in the grains' superconducting transition temperatures. The lambda ( T ) temperature dependence is exponential at low temperatures, which allows us to determine the energy gap Delta 0 =1.7 k B T c . ...

Еще в разделе: (Показать все результаты (>314) - www.issp.ac.ru/ )

• LEK - Info
• LEK - Equipment
• Shevchun A.F. - Publications

This page provides explanatory text for the dials shown on the Rice Current Solar Wind Conditions and Current Solar Wind Conditions (Dials Only) webpage. These dials use the last good received set of measurements from the Real Time Solar Wind package on the Advanced Composition Explorer (ACE) spacecraft. ... Measured) This quantity is the number of solar wind protons per unit volume as measured by the ACE Solar Wind Electron Proton Alpha Monitor (SWEPAM) . ... It is measured by ACE/SWEPAM. ...

Еще в разделе: (Показать все результаты (>663) - www.iki.rssi.ru/ )

• The Sun's Corona
• Medium
• Sun [Oulu]

... Evolution of the magnetic field (solid lines) , temperature (colour) , and velocity (arrows) at four times for case A1 (a), A2 (b), B1 (c), and B2 (d). The characteristic parameters of magnetic field strength and electron number density are given above each case plot. ... Aims We aim at investigating the formation of jet-like features in the lower solar atmosphere, e.g. chromosphere and transition region, as a result of magnetic reconnection. ...

Еще в разделе: (Показать все результаты (>1291) - star.arm.ac.uk/ )

• A Blinker Model
• Magnetic Reconnection

Cherechukin A.A., Koledov V.V., Shavrov V.G., Tulaikova A.A., Vasil'ev A.N. Magnetic and structural phase transitions in Ni2+УMn1-УGa (0<У<1) alloys are investigated experimentally. The martensite domains formation under the action of external magnetic field on the surface of polycrystalline Ni2,19Mn0,81Ga specimen was investigated by optical method. ... It is found that the martensite phase formation temperature is enhanced by the order of 0,3 K in magnetic field of 1 kOe. ...

Еще в разделе: (Показать все результаты (>516) - www.cplire.ru/ )

• Thin Film Oxide Electronics Laboratory. Equipment
• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order
• Kotel'nikov IRE RAS, LASLDS

SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM . ... 3 components measurements of both magnetic and electric fields; . ... wide frequency range (0 - 10000) Hz; . ... ECHO-EM is intended for measurement of a complete vector and three components of both electric and magnetic fields, and transfers the received data to the block of the processing of the information and also in telemetry. ... digital 0.1-20 Hz; . ... frequency band (0.01- 10000) Hz; . ... digital (500 - 1000) Hz; . ...

Еще в разделе: (Показать все результаты (>63) - space.univ.kiev.ua/ )

• Solar Physics

... Astronomers of the SAO together with an international group of scientists have proposed an explanation to the long-standing mystery of why magnetic fields are more common amongst cool white dwarf stars than amongst young and hotter ones. ... As the result magnetic white dwarfs demonstrate excess in their frequencies in the temperature range below 14000K. The authors also show that the strongly magnetic white dwarfs are of the oldest stars of the Galaxy originated from intermediate-mass relic stars. ...

Еще в разделе: (Показать все результаты (>160) - mavr.sao.ru/ )

• Galaxy sector, archive 2008
• Galaxy sector, archive 2014
• Physics of Magnetic Stars 2007

... Key words: stars: magnetic fields ґ stars: chemically p eculiar 1 Intro duction On the basis of all the available published magnetic measurements for Ap stars we have found a few relations describing the frequency of o ccurrence of the sp ecific magnetic field intensity for all typ es of chemical p eculiarities (Bychkov et al. 2003a). ... Magnetization of stars in the `strongly'-magnetic group exceeds that in the `weak'-magnetic group typically by a factor of 5ґ10, on the average. ...

Еще в разделе: (Показать все результаты (>420) - jet.sao.ru/ )

• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and

... About ATNF overview . ... Parkes radio telescope . ... Saxton & Wu (1999) presented calculations of the stability of the accretion shock which forms on the surface of an accreting magnetic white dwarf in AM Herculis type systems in an attempt to explain the observed properties of the quasi periodic oscillations sometimes seen in these systems. He showed that radiative cooling may cause thermal instability in the post-shock structure of the accretion flow settling onto a magnetic white dwarf. ...

Еще в разделе: (Показать все результаты (>2749) - www.atnf.csiro.au/ )

• Radio pulse characteristics
• Atmospheric opacity and system temperature
• Accretion onto Magnetic White Dwarfs

... The Chinese would certainly not have invented the magnetic compass. ... Chemically and mineralogically, the lodestone is magnetite, a massive type of iron ore, an oxide of iron, a mineral related the the brown stuff coating the magnetic disks and tapes used by computers. ... But even then, just resting a few million years in the Earth's magnetic field would produce no magnetization. ... Still, as Gilbert observed, in a long iron rod that magnetism was channeled to the ends, where it could be noted. ...

Еще в разделе: (Показать все результаты (>1181) - www.cosmos.ru/ )

• Magnetic Fields
• The Sun's Corona
• Plasma Physics -- History

... To determine a lower limit to the sensitivity of current observations to measurements of NS surface temperatures, we have used data from the Einstein Slew Survey (Elvis et al. 1990) to establish temperature limits for 275 pulsars which received nonzero exposure during the survey. ... Filled squares correspond to pulsars actually detected in the survey data; the smaller symbols correspond to upper limits to the count rates. ... Click here for plot of x-ray data vs. cooling curves. ...

Еще в разделе: (Показать все результаты (>748) - hea-www.harvard.edu/ )

• The Interstellar Medium
• Two-Temperature Raymond Model
• The AstroStat Slog temperature

Astronomy Picture of the Day . ... 11.08.1998 . ... Credit: A. Title ( Stanford Lockheed Institute ), TRACE , NASA Explanation: Hot gas dances across the surface of the Sun in this picture from the orbiting TRACE satellite . ... Hot gas is channeled into lanes ordered by the Sun's chaotic magnetic field . ... August . ... August 1998 . ... 1997 1998 . ... NASA Official: Jay Norris. ... U. Based on Astronomy Picture Of the Day . Publications with keywords: Sun . Publications with words: Sun . ...

Еще в разделе: (Показать все результаты (>33626) - www.astronet.ru/ )

• Journal "Peremennye Zvezdy"
• Z Machine Sets Unexpected Earth Temperature Record
• Астронет > Z Machine Sets Unexpected Earth Temperature Record

... Solar Mystery Nears Solution with Data from SOHO Spacecraft . Magnetic Carpet Space Science Update Page . The SOHO Spacecraft . ... The relationship between the structure of the magnetic carpet and the heating of the solar corona was discovered by comparing images of the Sun taken simultaneously by the MDI and EIT instruments on SOHO. Magnetic vs. ... These concentrations make up the solar "magnetic carpet" that is believed to be responsible for the extreme heating of the corona. ...

Еще в разделе: (Показать все результаты (>6788) - www.arcetri.astro.it/ )

• A collection of images
• APOD: 2000 July 20 - AR9077: Solar Magnetic Arcade
• West Gardian temperature controller tech schedule

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 ( ). ...

Еще в разделе: (Показать все результаты (>180) - www.astro.spbu.ru/ )

• Linear polarization: wavelength dependence

. Next: Diameters Up: Stellar parameters from calibrations Previous: Gravities Contents . Temperatures of stars are derived from their spectral type and luminosity class. Calibrations are stored in files spec_par.V, spec_par.IV, spec_par.III, spec_par.II, spec_par.I in oyster/starbase . teff_stars Compute effective temperature for all stars in startable. teff_star ( spectrum _char ) Function. Return effective temperature for star with specified spectrum. Christian Hummel 2015-04-28

Еще в разделе: (Показать все результаты (>2787) - www.eso.org/ )

• ESO - Thesis Topic: Magnetic fields in massive stars
• ESO - Thesis Topic: The role of magnetic fields in the intermediate-mass star
• ESO - Thesis Topic: Star formation: probing magnetic fields and their spheres

TEMPERATURE OF REGOLITH IN COLD TRAPS ON THE MOON A.A. Berezhnoi Sternberg Astronomical Institute Moscow, Russia The hypothesis of the existence of the lunar ice in cold traps was stated in (Watson et al., ... Arnold, 1979) estimated the mean temperature on the surface of lunar cold traps as 40-90 K. We plotted the dependence of regolith mean temperature on depth for these two values of mean temperature on the surface (see figure 1). ... Arnold J.R. Ice in the lunar polar regions, J. Geophys. ...

Еще в разделе: (Показать все результаты (>65) - selena.sai.msu.ru/ )

• http://selena.sai.msu.ru/Symposium/RadioMoonE.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf
• http://selena.sai.msu.ru/Kozl/Publications/ms40/50_Kozlova_Shevchenko.pdf

. Русская версия (Win-1251) . English version

Еще в разделе: (Показать все результаты (>185) - www.gao.spb.ru/ )

• Combined database of sunspot magnetic fields
• Magnetic fields database
• Home Page

. A filament stretches across the lower half of the Sun in this image captured by NASA s Solar Dynamics Observatory on February 10, 2015. Filaments are huge tubes of relatively cool solar material held high up in the corona by magnetic fields. Researchers simulated how the material moves in filament threads to explore how a particular type of motion could contribute to the extremely hot temperatures in the Sun s upper atmosphere, the corona. NASA/SDO

Еще в разделе: (Показать все результаты (>1414) - www.astronomy.com/ )

• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B16CB2439-EABA-45B5-BE6A-2FFA27C553C1%7D
• magnetic field | Astronomy.com
• How do neutron stars generate steady magnetic fields? | Astronomy.com

... Джемпер Bestia. ... Mini Creative NdFeB Magnetic Ball Puzzle 5mm Diameter Educational Toy - 432Pcs . ... Puzzle Style: Magnetic Puzzle . ... Package Contents: 432 x Magnetic Ball . ...

Еще в разделе: (Показать все результаты (>470) - astrokuban.info/ )

• Золотое кольцо 01K613066Z - Ювелирное изделие - Ювелирное изделие Introduction
• Сланцы Nike - Nike - Nike Золотое кольцо 01T415224
• Комплект для кроватки Micuna Juliette 120х60 (6 предметов) - Micuna - Micuna

ARCSAT ID NUMBER: AS05 DESCRIPTIVE TITLE: Time Series photometry of F/G/K + M dwarf eclipsing binaries PI: Leslie Hebb OBSERVER(S): Leslie Hebb UNCERTIFIED/UNTRAINED OBSERVERS: HWS students, Michelle Gomez and Betty Vasquez COLLABORATORS: Yilen Gomez Maqueo Chew CONTACT INFORMATION: Leslie Hebb , hebb @hws.edu, 206-618-9843 TIME REQUESTED: 1 week in April INSTRUMENT: Flarecam FILTERS: griz COMMENTS: no BRIEF SCIENCE JUSTIFICATION ...

Еще в разделе: (Показать все результаты (>222) - www.apo.nmsu.edu/ )

• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS04.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2015/AS08.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS08.html

... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ... The derived temperature maps are quite similar to the ones obtained earlier with a different methods, the main differences occurring in the spot latitudes and relative strength of the spot structures....

Еще в разделе: (Показать все результаты (>114) - vo.astronet.ru/ )