The space probes Pioneer 3 and 4 detected a wide belt of trapped particles beyond the inner belt. ... We now know that outer-belt ions and electrons probably come from the long "magnetic tail" of stretched field lines on the night side of the magnetosphere. Two radiation belts . ... When the outburst ends and the electric field dies away, the particles find themselves locked in trapped orbits of the ring current and the outer radiation belt. ... Exploration" home page (index) Glossary . ...

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• Magnetospheric electric fields (Oulu)
• Magnetic Field Lines
• Drift mechanisms [Oulu]

... Listed below are questions submitted by users of "The Exploration of the Earth's Magnetosphere" and the answers given to them. ... The ones included below are either of the sort that keeps coming up again and again--the danger of solar eruptions, the reversal of the Earth's magnetic field, etc.-- or else the answers make a special point, going into extra details which might interest other users. ... Radiation Belts and Manned Space Flight . ... Capturing the Energy of the Solar Wind . ...

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• A Brief History of Magnetospheric Physics Before the Spaceflight Era
• Magnetic Fields
• Magnetic Field Lines

... HST . ... Data . ... HST Overview . Overview . ... Cycle 24 Announcement . ... Retrieving HST Data . ... Instruments . ... Grism Spectroscopy . ... UVIS Flats . ... Instrument Handbook . Data Handbook . ... The Wide Field Camera 3 (WFC3) is a fourth-generation UVIS/IR imager aboard the Hubble Space Telescope (HST). WFC3 was installed in May 2009 during HST servicing mission 4, and replaces the Wide Field Planetary Camera 2 (WFPC2). ... ISR 2016-09: WFC3 Cycle 22 Proposal 14007: UVIS Gain . ...

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• HDF-S Data Products
• The Hubble Deep Field
• HST/ACS Ultra-Deep Field

... Magnetic fields, subatomic particles, etc., traveling in different directions fill the universe. Do they deflect or otherwise affect one another? If so, isnт??t the information we get from them distorted? ... Neutrino astronomy, which is still in its infancy, is attractive because neutrinos interact so weakly with matter that few of these distorting effects occur. Get instant access to subscriber content on Astronomy.com! ...

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• How do neutron stars generate steady magnetic fields? | Astronomy.com
• Do the magnetic fields of the planets affect spacecraft during flybys? |
• Previously understood that magnetic fields were directly related to rotation,

... Nizhnij Arkhyz, 2007 . ... Romanyuk I.I. Speech at the opening ceremony of the conference "Physics of magnetic stars" . ... Gnedin Yu.N. Magnetic fields of stars and fundamental particle physics . ... Landstreet J.D., Andretta V., Bagnulo S., Mason E., Silaj J., Wade G.A. The magnetic fields of peculiar A and B stars in open clusters . ... Wade G.A., Catala C., Alecian E., Folsom C., Bagnulo S., Bohm T., Bouret J.-C., Donati J.-F., Drouin D. , Landstreet J.D. Magnetic fields in Herbig Ae/Be stars . ...

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• Suppression of cooling by strong magnetic fields in white dwarf stars
• New data on the cpmplex field structure of chemically peculiar stars
• Solar activity

... Classes . ... Definition at line 87 of file SDSourceHandler.h . ... Definition at line 114 of file SDSourceHandler.h . ... Definition at line 137 of file SDSourceHandler.h . ... Definition at line 116 of file SDSourceHandler.h . ... Definition at line 139 of file SDSourceHandler.h . ... Definition at line 134 of file SDSourceHandler.h . ... Definition at line 117 of file SDSourceHandler.h . ... Definition at line 138 of file SDSourceHandler.h . ... Definition at line 131 of file SDSourceHandler.h . ...

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• The magnetic fields of neutron stars
• Southern Cross Astrophysics Conference Series
• Propagation through Turbulent Magnetic Fields

Next: The Corotation Radius Up: ``Ecology'' of Magnetic Rotators Previous: The Stopping Radius in . Apparently, the magnetic field of a star becomes significant only when the stopping radius exceeds the radius of the star, . ... Most presently observed NS have magnetic fields  G and dipole moments  G cm , so the magnetic field must necessarily be taken into account when considering interaction of matter with these stars. ... Sat Feb 22 18:38:13 MSK 1997 ...

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• fields
• ADS Abstract Service Results
• The Stopping Radius

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

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• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM
• Researches of Astronomy and Space Physics Department
• Near-Earth Space

... Alexey Zaytsev (Kaliningrad) . ... Let $\Tau=(T_n)_{n \ge 1}$ be a tower of function fields over a finite field. Then there exits a sequence of zeta functions (or L-polynomials) (Z_n(t))_{n\ge 1} (or (L_n(t))_{n\ge 1} ) attached to it. ... At the end of the talk we rephrase Beelen's result in term of asymptotic zeta functions in order to find asymptotic zeta functions of known examples of good tower and suggest a new definition of asymptotic zeta function of a tower of function fields. ...

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• Conference "Global Fields"
• Conference Global Fields
• Conference "Global fields"

... The polarimetry group at the Arcetri Observatory has been working for several years, mainly from the theoretical-interpretative side, on the polarization of the radiation emitted by objects of astrophysical interest. ... E. Landi Degl'Innocenti "The physics of polarization" in "Astrophysical Spectropolarimetry", J. Trujillo Bueno, F. Moreno Insertis, F. Sanchez (eds.), Cambridge University Press, 1. ... E. Landi Degl'Innocenti "The Zeeman effect: applications to solar physics" Astron. ...

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• Arcetri Solar Physics Group: High Resolution Studies
• Galileo Finds Giant Iron Core in Jupiter's Moon Io
• Hubble Observations Shed New Light on Jupiter Collision

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: The role of magnetic fields in the intermediate-mass star formation process . ... Spectropolarimetric observations of Herbig Ae/Be stars indicate that magnetic fields are important ingredients of intermediate mass star formation. To properly understand the physics involved in the intermediate mass star formation process, it is particularly important to know the origin of the magnetic fields in these stars. ...

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• ESO - Thesis Topic: Magnetic fields in massive stars
• ESO - Thesis Topic: Star formation: probing magnetic fields and their spheres
• ESO - Thesis Topic: Magnetic fields and interaction in binary systems

. Русская версия (Win-1251) . English version

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• Combined database of sunspot magnetic fields
• Magnetic fields database
• Enslish version of database

The space between the planets is far from empty. It contains: electromagnetic radiation (photons); hot plasma (electrons, protons and other ions) a.k.a. the solar wind ; cosmic rays; microscopic dust particles; and magnetic fields (primarily the Sun's). While the Sun 's radiation is obvious, the other components of the interplanetary medium were not discovered until very recently. ... Except near some of the planets, interplanetary space is filled with the Sun's magnetic field. ... Sun .. ...

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• APOD: November 7, 1996 - Fields of Minerals on Ganymede
• APOD: 2002 November 25 - The Earth's Magnetic Field
• APOD: 2015 January 27 - Our Galaxy's Magnetic Field from Planck

Bigbang Forum Message . Forums: . ... The Sun Energy Source Is Not Nuclear Fusion But Magnetic Fields. ... The sun is not heated by fusion reaction but by magnetic fields coming from the galactic center. The nuclear fusion is a by product of the magnetic fields heating. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• A Field Does Not Contain Energy? - an Astronomy Net Blackholes2 Forum Message
• Apparently You Do Not Accept Conventional Physics - an Astronomy Net
• If Gravity Is Conveyed By A Wave Field? - an Astronomy Net Blackholes2 Forum

... 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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• http://www.mso.anu.edu.au/seminars/abstracts/20150326-1100.html
• http://www.mso.anu.edu.au/~geoff/AGD/MHD_Eqns.pdf
• COALA - Computational Astrophysics Laboratory

Origin & Evolution of Magnetic Fields Ellen Zweibel zweibel@astro.wisc.edu Depar tments of Astronomy & Physics University of Wisconsin, Madison and Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas Origin & EvolutionofMagnetic Fields ­ p.1/17 Importance of the Problem A cosmological problem. ... Interplay with ISM studies Structure of galactic fields on large & small scales? How do fields affect turbulence? ... Origin & EvolutionofMagnetic Fields ­ p.7/17 We Also Know.. ...

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• I-GALFA Survey Fields
• Heiles Symposium Presentations
• Slide 25

... The evolution of magnetic fields in OB-type stars from the study of open clusters of different ages . ... Wade G. A. The MiMeS Project: Magnetism in Massive Stars . ... Polosukhina N., Shavrina T., Drake N., Kudryavtsev D. Smirnova M. New results of the spectral observations of CPstars in the Li I 6708? spectral region with BTA telescope of SAO RAS . ... Magnetic Stars-2010 . ... List of participants . List of reports . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

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• Low Level Operators and Bit Fields
• Line-of-sight velocity field of NGC 157.
• Main Researches Activities

The radiation belts around the planets are the interrnal regions of planets' magnetospheres where the own magnetic field of a planet keeps the charged particles (protons and electrons) having the great kinetic energy. ... They usually distinguish the Earth's internal and external radiation belts. the internal radiation belt of the Earth has the maximum particles density (mainly protones) over the equator in the height of 22 thousand km. ... Jupiter and Saturn have the powerful radiation belts. ...

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• sunstroene

... The normalised fluxes of 18 stars of Table 1 for which new field determinations are presented in this paper. ... Detection of magnetic fields has been reported in several sdO and sdB stars. ... We revisit data previously published in the literature, and we present new observations to clarify the question of how common magnetic fields are in subdwarf stars. ... Here we present new FORS1 field measurements for 17 stars, 14 of which have never been observed for magnetic fields before. ...

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• Abstract 205
• James Aumonier: Cattle in the fields
• An Overview of the Coupled Earth-Sun System PPARC Introductory Solar System

... A second method to account for illumination problems in the flat fields is to remove the large scale pattern from the flat field itself. This is useful if there are no reasonable blank sky calibration frames and the astronomical exposures are evenly illuminated but the flat fields are not. ... Obviously, after having obtained the illumination corrected flat field it is reasonable to replace the original flat fields by the corrected flat fields in the reduction table. ...

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• The SNRs radio magnetic fields
• Combining Flat Fields
• Construction of Flat Fields