Magnetic field measurements onboard the Interball Tail spacecraft are carried out by the FM-3I instrument which consists of two flux-gate magnetometers covering two different ranges: [-200, +200] nT and [-1000, +1000] nT. Besides scientific goals, the FM-3I experiment data is used to perform the attitude control of the Interball Tail spacecraft. ... August 22, 1995 . ... October 18, 1995 . Top of the page . ... Back to the Interball Home Page . ...

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• List of currently available KP AZ.
• Restored magnetic field
• Space Weather Dials Interpretation Guide

ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Information & tools for observers . ... Australia Telescope Online Archive (ATOA) . ... ATCA | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... The Australia Telescope National Facility Colloquium . ...

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• Southern Cross Astrophysics Conference Series

The main objective of measurements of charged particles and plasma flux characteristics in the INTERBALL project is to study the spatial structure of the terrestrial magnetosphere as a global system in various scales and for varying external conditions. ... The SPS spectrometer is designed for estimating the ion energy and angular distributions and for measurements of the electron energy distributions. ... Particles under measurements . ions/electrons . ions . ... 3 for ions,1 for electrons . ...

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• PhSRM
• The Acceleration of the Aurora
• Events on January 10-11, 1997 - INTERBALL observations

... Deviatov E.V., Khrapai V.S., Shashkin A.A., Dolgopolov V.T., et al. ... Phys. Rev. Lett. ... V.S. Khrapai, A.A. Shashkin, V.T. Dolgopolov . ... V.S. Khrapai . ... V.S. Khrapai, A.A. Shashkin, E.L. Shangina, V. Pellegrini, F. Beltram, G. Biasiol and L. Sorba . ... Khrapai V.S., Shashkin A.A., Trokina M.G., Dolgopolov V.T. et al. ... V.S. Khrapai, A.A. Shashkin, M.G. Trokina, V.T. Dolgopolov, V. Pellegrini, et al. ... V.V. Vanovsky, V.S. Khrapai, A.A. Shashkin, V. Pellegrini, L. Sorba, G. Biasiol . ...

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• LHPP ISSP RAS
• Theoretical department of ISSP RAS
• SPECIALITY 01.04.07 - CONDENSED MATTER PHYSICS SUPPLEMENTARY PROGRAM

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; . ...

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• MISSION WARNING
• SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW
• Additional Parts of Theoretical Astrophysics

CONTENTS : INTRODUCTION INSTRUMENTATION FOR MAGNETIC FIELD MEASUREMENTS Instrumentation for measurement of stellar magnetic fields with the 6-m telescope: Yu. ... 32 The bank of observational data for chemically peculiar stars: V. S. Lebedev .36 RESULTS ON MAGNETIC FIELD MEASUREMENTS A surface magnetic field study of Ap star 78 Virginis: T. A. Ryabchikova, E. S. Davydova, D. Z. Kolev Modern state of magnetic field investigation in M. Yu. ... Magnetic fields of superqiants: E. Gerth .. ...

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• 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
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Home

Magnetic Stars, 2011, pp. ... 2008). ... The origin of magnetic fields of hot massive stars is explained by the fossil field theory, MAGNETISM OF STARS 451 1-5 Be measurements -> 1278 stars 100 N stars 6-10 Be measurements -> 80 stars 50 11-15 Be measurements -> 47 stars 0 20 40 60 80 100 120 140 160 180 The namber of individual measurements The number of individual measurements Figure 1: The number of stars in a single bin versus the number of individual Be determinations for a single star. ...

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• Physics of Magnetic Stars 2007
• Galaxy sector, archive 2015
• HD965

We present the results of an extensive observing campaign on the O7.5 III star xi Persei. The UV observations were obtained with the International Ultraviolet Explorer. xi Per was monitored continuously in October 1994 during 10 days at ultraviolet and visual wavelengths. The ground-based optical observations include magnetic field measurements, HЮБ and He I lambda 6678 spectra, and were partially covered by photometry and polarimetry. ...

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• Superconducting Confined Electron Devices for Possible Application as
• About Magnetic Tape...

... For the first time during space experiments it was shown an opportunity of ballistic transformation of a wave through an ionospheric wave barrier. ... New nonlinear electromagnetic structures like collisionless shock waves ( "jumps" of electric and magnetic fields, plasma density "jumps") are found. ... It has been shown, that the modulated beam of electrons can be used for nonlocal determination of electron density and the magnetic field value. ...

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• APEX/Equipment
• [INTERBALL] pr-7

... Spectral regions highlighted by green bars have been used to detemine the тЯиB z тЯй value from H Balmer lines, and the magenta bars highlight the spectral regions used to estimate the magnetic field from metal lines. ... The FORS1 instrument of the ESO Very Large Telescope was used to obtain low resolution circular polarized spectra of nearly a thousand of different stars, with the aim of measuring their mean longitudinal magnetic fields. ...

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• Conference 98
• Preprints

... Russian Academy of Sciences, Department of Physical Sciences , Project number . ... Bicrystal junction and heterostructures made of cuprate oxide material with strong correlated electrons will be investigated. ... DC, microwave and noise properties of the junction will be investigated. ... To investigate noise spectral density in oxide superconducting bicrystal junction. ... To develop new type of bicrystal junction with misorientation of c axes around the basic plane axes. ...

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• IRE RAS. Research Divisions.
• Magnetic Resonance and Spin Relaxation in Solids. IRE RAS.
• MIT images

... Measurements of magnetic fields on scales larger than galaxy clusters are needed to distinguish between fields generated in the primordial Universe and those generated at later epochs, with implications for particle physics, cosmology, and astrophysics. ... In this talk I will review mechanisms for generating magnetic fields across cosmic time, implications for post-recombination physics, and current observational constraints on intergalactic magnetic fields. ...

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Proposal Identi cation No.: ... Instrument Setup 430 G 610 L-wide 430 CH receiver S-band receiver S-low Atmospheric Optical Instruments: Special Equipment or setup: several Mammoth 2 tapes RFI Considerations Frequency Ranges Planned 425-435 (50 MHz if a wider RF lter is available) 690-730 (ie, new receiver at 710 MHz) (*) 1100-1550 2300-2500 (*) observations at this band be scheduled between AST: 0 hr and 6 hr This proposal requires coordination with Punta Salinas radar within the band 1222-1381 MHz.. ...

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• http://www.naic.edu/~astro/chicago2/talks/Bastian-Solar_Radiophysics_of_the_Future.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/RobishawtagA2764tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/BhattagP1926tp.pdf

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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• http://www.gao.spb.ru/russian/psas/ffk2013/talkfiles.html
• http://www.gao.spb.ru/russian/psas/ffk2013/talks.html
• Description of database

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Magnetic fields in massive stars . ... Observing Facilities . ... Data Handling and Products . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... While magnetic fields in the sun and solar-like stars have been studied intensively, very little is yet known about their existence, origin and role in massive stars, like O and Wolf-Rayet stars. ...

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

... Units are separated by spaces, positive numbers denote powers, all units to the right of the slash are in the denominator (negative powers). Planck constant h . ... 6.0221367e23 particles/mol . ... Free electron gyromagnetic ratio gamma e . ... gamma p / (2 pi) = 42.576375 MHz/T . ... Gas constant R . ... The NIST Reference on Constants, Units, and Uncertainty . CODATA Internationally recommended values of the Fundamental Physical Constants . ... Table of Fundamental Physical Constants (MIT) . ...

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• MIT 3.091 Table of Fundamental Physical Constants
• Photon/Particle Counting Image Measurement System : PIAS-TI (Hamamatsu
• X-ray Electron Microscope : C5333 (Hamamatsu Photonics)

... Credit: Jack Connerney, Mario Acuna, Carol Ladd, MGS , NASA Explanation: Mapping Mars from orbit, instruments on the Mars Global Surveyor (MGS) spacecraft have recently revealed banded magnetic field patterns - a startling and unanticipated suggestion that the Red Planet was more Earth-like in its distant past. ... Such patterns are known to be produced on Earth by plate tectonics . ... NASA Official: Jay Norris. ... Publications with keywords: Mars - magnetic field - plate tectonics . ...

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• Астронет > Magnetic Mars
• The Smooth Spheres of Gravity Probe B
• XWare > APOD

... May 4, 1999 . Magnetic Mars . Credit: Jack Connerney, Mario Acuna, Carol Ladd, MGS , NASA . Explanation: Mapping Mars from orbit, instruments on the Mars Global Surveyor (MGS) spacecraft have recently revealed banded magnetic field patterns - a startling and unanticipated suggestion that the Red Planet was more Earth-like in its distant past. ... As the crustal plates spread apart along the mid-ocean ridges , they carry a progressive banded record of Earth's changing magnetic field. ...

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• Medium
• APOD: 2000 December 3 - Earth's North Magnetic Pole
• APOD: 2004 September 19 - Earth's North Magnetic Pole

Main News Phones Research area Brief history Institute Structure Experimental Base Observational data English/Russian . ... 677980 Yakutsk, Russia . ... 7(4112)390400 . Fax: . ... Magnetic Observatory . ... the Yakutsk magnetic observatory is located at a distance of 9-10 km to the south from Yakutsk . ... absolute and variation measurements of the Earth?s magnetic field . ... facilities for absolute measurement of the geomagnetic field i.e. the proton magnetometer, the QHM-magnetometer . ...

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... NASA Lunar Orbiter . ... The Lunar Prospector is designed for a low-polar orbit investigation of the Moon, including mapping of surface composition and possible polar ice deposits, measurements of magnetic and gravity fields, and study of lunar outgassing events. Data from the 1- to 3-year mission will allow construction of a detailed map of the surface composition of the Moon, and will improve our understanding of the origin, evolution, current state, and resources of the Moon. ...

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• Galileo Finds Giant Iron Core in Jupiter's Moon Io
• Arcetri Solar Physics Group: Solar Polarimetry
• APOD: 2000 July 20 - AR9077: Solar Magnetic Arcade