Search Publications

Delay in solar energetic particle onsets at high heliographic latitudes
DOI: 10.5194/angeo-21-1367-2003 Bibcode: 2003AnGeo..21.1367D

Balogh, A.; Krucker, S.; Dalla, S. +9 more

Ulysses observations have shown that solar energetic particles (SEPs) can easily reach high heliographic latitudes. To obtain information on the release and propagation of SEPs prior to their arrival at Ulysses, we analyse the onsets of nine large high-latitude particle events. We measure the onset times in several energy channels, and plot them v…

2003 Annales Geophysicae
Ulysses 33
On the origin of inner-source pickup ions
DOI: 10.1029/2002GL015218 Bibcode: 2003GeoRL..30.1077W

Wimmer-Schweingruber, Robert F.; Bochsler, Peter

In situ measurements of pickup ions (PUI) exhibit a component that has nearly thermalized with the solar wind. This implies an origin close to the Sun and is generally ascribed to interaction of the solar wind with interplanetary dust particles (IDPs). We propose a scenario for the origin of inner-source PUIs in which a population of very small ID…

2003 Geophysical Research Letters
SOHO 33
Toroidal-shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000
DOI: 10.1029/2002JA009574 Bibcode: 2003JGRA..108.1220T

Kojima, Masayoshi; Tokumaru, Munetoshi; Fujiki, Ken'ichi +2 more

Interplanetary scintillation (IPS) measurements made with the 327 MHz radio telescopes of the Solar-Terrestrial Environment Laboratory, Nagoya University, have been used to study a three-dimensional structure of the interplanetary (IP) disturbance associated with the halo coronal mass ejection (CME) event on 14 July 2000 (the so-called "Bastille D…

2003 Journal of Geophysical Research (Space Physics)
SOHO 33
A Hubble Space Telescope WFPC2 Snapshot Survey of 2MASS-selected Red QSOs
DOI: 10.1086/375163 Bibcode: 2003ApJ...590..707M

Hines, Dean C.; Armus, Lee; Schmidt, Gary D. +5 more

Using simple infrared color selection, the Two Micron All Sky Survey (2MASS) has found a large number of red, previously unidentified, radio-quiet quasi-stellar objects (QSOs). Although missed by UV/optical surveys, the 2MASS QSOs have Ks-band luminosities that are comparable to ``classical'' QSOs. This suggests the possible discovery o…

2003 The Astrophysical Journal
eHST 33
Evidence of Flaring in a Transequatorial Loop on the Sun
DOI: 10.1086/380558 Bibcode: 2003ApJ...598L..59H

Harra, Louise K.; Matthews, Sarah A.; van Driel-Gesztelyi, Lidia

We present evidence of flaring behavior in a transequatorial loop (TEL) that lights up in soft X-rays on 2000 July 13. The large loop structure connects NOAA Active Regions 9070/9066 in the northern hemisphere and AR 9069/9068 in the southern hemisphere. We follow the loop systems for 2 days and observe several pieces of evidence strongly suggesti…

2003 The Astrophysical Journal
SOHO 33
Hipparcos red stars in the HpVT2 and VIC systems
DOI: 10.1051/0004-6361:20021589 Bibcode: 2003A&A...397..997P

Makarov, V. V.; Berdnikov, L. N.; Lebzelter, T. +6 more

For Hipparcos M, S, and C spectral type stars, we provide calibrated instantaneous (epoch) Cousins V - I color indices using newly derived HpVT2 photometry. Three new sets of ground-based Cousins VI data have been obtained for more than 170 carbon and red M giants. These datasets in combination with the published sources of V…

2003 Astronomy and Astrophysics
Hipparcos 33
Solar maximum low-energy particle observations at heliographic latitudes above 75 degrees
DOI: 10.1016/S0273-1177(03)00339-9 Bibcode: 2003AdSpR..32..579L

Lario, D.; Reisenfeld, D. B.; Roelof, E. C. +1 more

We present a preliminary analysis of low-energy particle observations by the Ulysses and ACE spacecraft during the time intervals that Ulysses spent at heliographic latitudes above 75 degrees during its solar maximum orbit. The most southerly and northerly latitudes (80.2°) were reached by Ulysses in November 2000 and October 2001, respectively. T…

2003 Advances in Space Research
Ulysses 33
H1320+551: a type 1.8/1.9 Seyfert galaxy with an unabsorbed X-ray spectrum
DOI: 10.1046/j.1365-8711.2003.06238.x Bibcode: 2003MNRAS.339..757B

Barcons, X.; Carrera, F. J.; Ceballos, M. T.

We present new optical spectroscopic and XMM-Newton X-ray observations of the active galactic nucleus (AGN) H1320+551. The optical data (consistent with but of better quality than a previously published spectrum) show this source to be a type 1.8/1.9 Seyfert galaxy at z= 0.0653. The narrow-line region is significantly reddened, with a Balmer decre…

2003 Monthly Notices of the Royal Astronomical Society
XMM-Newton 33
Near-IR spectra of ISOGAL sources in the inner Galactic Bulge
DOI: 10.1051/0004-6361:20030459 Bibcode: 2003A&A...405..531S

Omont, A.; Schultheis, M.; Ojha, D. K. +2 more

We present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15;mu m detected during the ISOGAL survey. Making use of the DENIS interstellar extinction map from Schultheis et al. (1999) we derive luminosities and find that the Mbol vs. 12CO and M_bol vs. H2O diagrams are powerful to…

2003 Astronomy and Astrophysics
ISO 33
What Do the Hubble Space Telescope and Chandra Tell Us about the Jet and the Nuclear Region of the Radio Galaxy 3C 270?
DOI: 10.1086/344690 Bibcode: 2003ApJ...582..645C

Sparks, William B.; Chiaberge, Marco; Capetti, Alessandro +2 more

The Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph ultraviolet image of the FR I radio galaxy 3C 270 shows the presence of a jetlike structure emerging from the position of the nucleus. This feature, which represents the first jetlike component ever detected in the UV in a radio galaxy with jets lying almost on the plane of the …

2003 The Astrophysical Journal
eHST 33