Search Publications

Ultraviolet Hubble Space Telescope Observations of the Jet in M87
DOI: 10.1086/429264 Bibcode: 2005ApJ...624..656W

Zepf, Stephen E.; Waters, Christopher Z.

We present new ultraviolet photometry of the jet in M87 obtained from Hubble Space Telescope (HST) WFPC2 imaging. We combine these ultraviolet data with previously published photometry for the knots of the jet in radio, optical, and X-ray and fit three theoretical synchrotron models to the full data set. The synchrotron models consistently overpre…

2005 The Astrophysical Journal
eHST 20
The disrupted molecular envelope of Frosty Leo
DOI: 10.1051/0004-6361:20041482 Bibcode: 2005A&A...431..979C

Sahai, R.; Sánchez Contreras, C.; Alcolea, J. +2 more

We present maps of CO emission in the protoplanetary nebula Frosty Leo. Observations of the rotational transitions 12CO J=2{-}1 and 1 0 have been obtained with the IRAM interferometer and the OVRO array. The molecular envelope of Frosty Leo is found to be complex and compact; most of the gas extends ⪉6´´ and shows a structure that is ve…

2005 Astronomy and Astrophysics
eHST 20
The Martian atmosphere above great volcanoes: Early planetary Fourier spectrometer observations
DOI: 10.1016/j.pss.2005.02.008 Bibcode: 2005P&SS...53.1053G

Grassi, D.; Ignatiev, N. I.; Zasova, L. V. +4 more

This work reports the first observations of the Martian atmosphere returned by the planetary Fourier spectrometer (PFS) on board of Mars express (MEX) satellite in the vicinity of the greatest volcanic domes of the planet. Two of the early MEX orbits have already covered the region of Olympus Mons and Ascraeus Mons. These measurements are very sim…

2005 Planetary and Space Science
MEx 20
Helium Abundance in High-Temperature Solar Flare Plasmas
DOI: 10.1086/426539 Bibcode: 2005ApJ...619.1142F

Landi, E.; Feldman, U.; Laming, J. M.

In the present work we use emission from dense plasmas late in the decay phase of flares, while the plasmas are still hot [(2-4)×106 K], to determine the absolute helium abundance in flaring solar corona. To achieve this, we make use of intensity ratios of H I and He II lines and of intensity ratios between the He II lines and the brems…

2005 The Astrophysical Journal
SOHO 20
Three Criteria to Discriminate between Elementary and Composite Coronal Loops
DOI: 10.1086/499041 Bibcode: 2005ApJ...634L.193A

Aschwanden, Markus J.

In this Letter, we establish three simple criteria to discriminate between elementary and composite loop structures, based on observations from high-resolution (TRACE) and low-resolution (EIT) imagers. Both data sets contain triple-filter data with a temperature diagnostic in the range of T~0.7-2.8 MK, which we use for forward-fitting of a differe…

2005 The Astrophysical Journal
SOHO 20
Resolving the enigmatic solar wind disappearance event of 11 May 1999
DOI: 10.1029/2004JA010535 Bibcode: 2005JGRA..110.8101J

Janardhan, P.; Tokumaru, M.; Kojima, M. +2 more

On 11 and 12 May 1999, the Earth was engulfed by an unusually low-density (<1 cm-3) and low-velocity (<350 km s-1) solar wind for a period of over 1 day. Extensive studies of this unusual event that occurred during Carrington rotation 1949 (CR1949), using both ground-based and space-based in situ observations, have not …

2005 Journal of Geophysical Research (Space Physics)
SOHO 20
Stability of the inner source pickup ions over the solar cycle
DOI: 10.1029/2004JA010847 Bibcode: 2005JGRA..110.5105A

Geiss, J.; McComas, D. J.; Schwadron, N. A. +2 more

Inner source pickup ions (PUIs) were discovered and are observed by Ulysses. They are thought to be generated by solar wind interaction with dust grains near the Sun. From previous work, four constraints were derived on inner source PUIs from observations near solar minimum: (1) the composition resembles the solar wind; (2) the distribution functi…

2005 Journal of Geophysical Research (Space Physics)
Ulysses 20
Multipoint observations of transient reconnection signatures in the cusp precipitation: A Cluster-IMAGE detailed case study
DOI: 10.1029/2004JA010621 Bibcode: 2005JGRA..110.3219B

Budnik, E.; Berchem, J.; Escoubet, C. P. +10 more

This paper uses 90 min of Cluster multipoint data at ∼5 RE altitude together with global dayside imaging data provided by the IMAGE-SI-12 instrument to analyze the northern cusp crossed on 14 July 2001, during a period of high solar wind pressure Psw and strongly duskward interplanetary magnetic field (IMF). Simultaneous obse…

2005 Journal of Geophysical Research (Space Physics)
Cluster 20
Global structure of the out-of-ecliptic solar wind
DOI: 10.1029/2004JA010875 Bibcode: 2005JGRA..110.3103W

Burlaga, L. F.; Sheeley, N. R.; Wang, Y. -M. +1 more

We use the observed photospheric field maps and the wind speed observed from Ulysses to study the out-of-ecliptic solar wind. The model calculates the wind speed from the rate of magnetic flux tube expansion factors using a conversion function that is determined by least squares fit of all currently available data from Ulysses. Using the best fit …

2005 Journal of Geophysical Research (Space Physics)
Ulysses 20
FUSE Observations of DB White Dwarfs
DOI: 10.1086/428750 Bibcode: 2005ApJ...624..317P

Kruk, J. W.; Chayer, P.; Petitclerc, N. +2 more

We present a comprehensive analysis of the far-ultraviolet spectra of three DB white dwarfs secured with the FUSE observatory. Transitions associated with various carbon ions are detected in all three objects. Atmospheric parameters are first redetermined on the basis of an analysis of archival data available, and the abundance of carbon, together…

2005 The Astrophysical Journal
IUE eHST 20