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Bubbles, Bow-Shocks, and Bullets over Broad-lines: Three Ionized Outflows Resolved with HST
Bibcode: 2002RMxAC..13..170C

Veilleux, S.; Ferruit, P.; Cecil, G.

HST images and spectra of high-velocity outflows from three AGN: (1) Show 5 arcsec -long bow shock/Mach disk complexes at the ends of the active radio jet in NGC 4258. We argue that the jet has precessed to its current orientation seen at VLBI-scales. (2) Fully resolve [O III]5007Å and H beta line profiles in the NLR of NGC 1068, and show compact …

2002 Revista Mexicana de Astronomia y Astrofisica Conference Series
eHST 4
The Spectrum and Term System of S VII
DOI: 10.1238/Physica.Regular.066a00140 Bibcode: 2002PhyS...66..140J

Jupén, Christer; Engström, Lars

The spectrum of six times ionized sulphur, S VII, has been investigated in the wavelength region 200-4000Å by means of the beam-foil and laser-produced plasma techniques. The analysis comprises 219 lines of which 105 are newly identified. The present work establishes 123 2s22p5nl energy levels of which 66 are new. The level energies are determined…

2002 Physica Scripta
SOHO 4
Motion of auroral ion outflow structures observed with CLUSTER and IMAGE FUV
DOI: 10.1029/2001JA005075 Bibcode: 2002JGRA..107.1186K

Lundin, R.; Winningham, J. D.; Dandouras, I. +22 more

During February 2001 the CLUSTER satellites recorded a number of perigee passes through the midnight auroral zone. We concentrate on one pass, on 23 February 2001, when structured outflow was observed. Simultaneous observations of the aurora were available from the FUV instrument on IMAGE. The features in the ion outflow observed by the Cluster Io…

2002 Journal of Geophysical Research (Space Physics)
Cluster 4
Quantitative Stellar Spectral Classification. II. Early Type Stars
DOI: 10.48550/arXiv.astro-ph/0205315 Bibcode: 2002RMxAA..38..127S

García, J.; Stock, J.; Stock, M. J. +1 more

The method developed by Stock & Stock (1999) for stars of spectral types A to K to derive absolute magnitudes and intrinsic colors from the equivalent widths of absorption lines in stellar spectra is extended to B-type stars. Spectra of this type of stars for which the Hipparcos catalogue gives parallaxes with an error of less than 20% were ob…

2002 Revista Mexicana de Astronomia y Astrofisica
Hipparcos 4
The rising phase of solar cycle 23 as seen by Ulysses
DOI: 10.1016/S0273-1177(01)00603-2 Bibcode: 2002AdSpR..29..401M

Marsden, R. G.

Following its highly successful survey of the latitudinal structure of the heliosphere under near-minimum solar activity conditions, the Ulysses space-probe embarked in 1998 on a second out-of-ecliptic orbit of the Sun. This second high-latitude survey will culminate near solar maximum, offering a unique opportunity to study the polar regions of t…

2002 Advances in Space Research
Ulysses 4
A discussion of recent evidence for solar irradiance variability and climate
DOI: 10.1016/S0273-1177(02)00206-5 Bibcode: 2002AdSpR..29.1417P

Kuhn, Jeff; Fröhlich, Claus; Sofia, Sabatino +2 more

One of the over-arching questions, among others, to be addressed by studying Sun-Earth connections is: "Is the climate changing in a way we can understand and predict?" The Earth's climate is the result of a complex and incompletely understood system of external inputs and interacting parts. Climate change can occur over a range of time scales, ma…

2002 Advances in Space Research
SOHO 4
The acceleration and release of solar energetic particles in events from April 20 - May 9, 1998
DOI: 10.1016/S0273-1177(02)00213-2 Bibcode: 2002AdSpR..29.1493S

Simnett, G. M.

The most active period in X-rays of the current solar cycle to date (August 1998) occurred from April 23 - May 9, 1998, when there were four X-class flares and two more which exceeded M6. All were likely to have been from AR 8210 (two were occulted and thus didn't have positive identification, although the coronal Yohkoh images were consistent wit…

2002 Advances in Space Research
SOHO 4
Do red giant stars pulsate in high overtones?
DOI: 10.1046/j.1365-8711.2002.05564.x Bibcode: 2002MNRAS.334..669P

Percy, John R.; Hosick, JoAnne

About 30 photometrically variable red giant stars have periods less than 10d, as determined by the compilers of the Hipparcos Catalogue from Hipparcos photometric measurements. These periods, when combined with estimates of the radii and masses of these stars, and with pulsation theory, imply that these stars are pulsating in very high overtones. …

2002 Monthly Notices of the Royal Astronomical Society
Hipparcos 4
A study of opacity in SOHO-SUMER and SOHO-CDS spectral observations. III. The validity of the escape probability model
DOI: 10.1051/0004-6361:20020581 Bibcode: 2002A&A...389..295F

Fischbacher, G. A.; Loch, S. D.; Summers, H. P.

The assumptions underpinning escape probability and absorption factor methods for describing spectral emission from optically thick plasmas, are addressed to test the range of validity of the associated expressions and to develop them for use within non-stratified atmospheres which include plasma flow and line blending. It is found that for modera…

2002 Astronomy and Astrophysics
SOHO 4
Astrophysics in 2001
DOI: 10.1086/341673 Bibcode: 2002PASP..114..475T

Aschwanden, Markus J.; Trimble, Virginia

During the year, astronomers provided explanations for solar topics ranging from the multiple personality disorder of neutrinos to cannibalism of CMEs (coronal mass ejections) and extra-solar topics including quivering stars, out-of-phase gaseous media, black holes of all sizes (too large, too small, and too medium), and the existence of the unive…

2002 Publications of the Astronomical Society of the Pacific
SOHO 4