The Sun is our nearest star and the source of energy for life on Earth. ... For centuries astronomers wondered whether they were clouds floating in the Sun's atmosphere, but we now know that they really are huge regions of magnetic field, about as intense as the field at the poles of an iron magnet. ... Such abrupt events were named solar flares , and what made them especially interesting was that occasionally, after a prominent flare, a magnetic storm would erupt on Earth. ...

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• Sun [Oulu]

Next: Radio pulse characteristics Up: An overview Previous: The structure of neutron . Typically Gauss for normal pulsars . Consistent with flux conservation during stellar collapse . ... Gravity dominates stellar structure . B field dominates exterior . Stellar surface is so small that observed emission is dominated by the magnetic field. ... Only field lines inside light cylinder are closed . Particles are constrained move along field lines . ...

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• Stellar wind and stellar disc models of dispersion and rotation measure
• Australia Telescope Compact Array Home Page
• Modeling the Observed Relationship

... Precisely one month ago, on 11 July 2009, the last active area of the new solar cycle disappeared from the surface of the Sun. Over the 30 days following this, neither observers on Earth nor devices in space have been able to detect the emergence of any sunspots. ... Therefore, it seems that our star has once again returned to a state of deep solar "winter", following several sparks of activity in May-June 2009. ... To date, this period has lasted 30 days. ...

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• The Russian TESIS Observatory will observe two solar eclipses from space
• Sunspots and active regions January 13, 2008
• Sunspots and active regions January 11, 2008

... Observatory . ... Science . ... Science Users Information > Science and Technical Meetings > Conferences 2015 > Stellar Halos 2015 . ... Science Users Information . Observing Facilities . La Silla Paranal Observatory . Paranal Facilities . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... Final Announcement & Note to participants . ...

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• ESO - Baryons at Low Densities: the Stellar Halos around Galaxies
• Gaitee Hussain @ ESO
• Rivi: Magnetic Stars

Various types of stars have dust around them. In the well known case of the Pleiades the dust around the stars is unrelated to the stars, and is instead dust from an interstellar cloud that the Pleiades cluster has drifted into on its way through the galactic disk. ... The dust in interstellar space is observed in a variety of ways: due to its passive absorption of starlight ("extinction"), by its production of polarization in starlight, and then at long wavelengths due to its thermal radiation. ...

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• Stellar Photometry
• Stars as Observed in the Infrared
• A search for the cause of cyclical wind variability in O stars. Simultaneous UV

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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• Astrophysics Group COAST Astronomical Results

Magnetic Stars, 2011, pp. ... Key words: stars: pre­main­sequence ­ stars: atmospheres ­ stars: individual: HD 101412 ­ stars: magnetic fields ­ stars: rotation ­ stars: variables: general 1 Intro duction In our previous studies we reported detections at a level higher than 3 for three out of seven Herbig Ae stars observed with the low­resolution spectropolarimeter FORS1 at the VLT (Hubrig et al., ... This is the first time the presence of element spots is detected on the surface of a Herbig Ae star. ...

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• HD965
• Galaxy sector, archive 2012
• Solar system sector, archive 2008

Observed stellar magnetic fields and some associated phenomena JD L 01/03/09 Leverhulme Lectures on Stellar Magnetism Sunspot magnetism Hale's discovery opened study of sunspot fields ­ ­ ­ ­ ­ ­ ­ 01/03/09 Sunspots typically have fields of 1- 3 kG Sunspots tend to come in pairs of opposite polarity In one hemisphere, north polarity usually leads and south trails ... If polar fields are different, chemistry could be too. ... Magnetic OB stars not always chemically peculiar. ...

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• http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-1-intro-to-stellar-magnetism.pdf
• Solar Eclipse Observed Armagh Observatory
• Born-again stars

... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...

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• Emission molecular bands
• About laboratory
• SCORPIO: IFP Gallery

... The Search of a pulsar Once the dedispersed time series is obtained, a Fourier transformation is performed. ... 2 Binary parameters The orbit of a pulsar , as well as any object, in a binary system is determined in its geometrical characteristics, space displacement and syncronised in time by the following parameters : Semimajor axis Eccentricity Longitude of periastron Binary period Time of ascending node a e PB T0 True spin period and observed spin period The ...

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• Searching the Environment around LyAlpha Absorbers
• Heiles Symposium Presentations
• REU Science Area

... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...