Search Publications

Surface charging of Saturn's plasma-absorbing moons
DOI: 10.1029/2010JA015525 Bibcode: 2010JGRA..115.8225R

Krupp, N.; Jones, G. H.; Roussos, E. +1 more

Recent results from the study of the interaction of Earth's moon with the solar wind have highlighted lunar surface charging as an important physical process not only for the local interaction of the surface and the impinging plasma but also for charged dust ejection and transport. Excluding Earth's moon, however, such studies have been limited to…

2010 Journal of Geophysical Research (Space Physics)
Cassini 16
Heliospheric Energetic Particle Reservoirs: Ulysses and ACE 175-315 keV Electron Observations
DOI: 10.1063/1.3395944 Bibcode: 2010AIPC.1216..625L

Lario, D.

Heliospheric energetic particle reservoirs are usually observed in the decay phase of large solar energetic particle (SEP) events when particle intensities measured by widely separated spacecraft (in longitude, latitude and radial distance) present comparable intensities (within a factor of 2-3) that evolve similarly in time. We use near-relativis…

2010 Twelfth International Solar Wind Conference
Ulysses 16
2MASS J03105986 +1648155 AB - a new binary at the L/T transition
DOI: 10.1051/0004-6361/200913711 Bibcode: 2010A&A...516A..37S

Bouy, H.; Henning, Th.; Brandner, W. +2 more

Context. The transition from the L to the T spectral type of brown dwarfs is marked by a very rapid transition phase, remarkable brightening in the J-band, and higher binary frequency. Despite being an active area of inquiry, this transition region still remains one of the most poorly understood phases of brown dwarf evolution.
Aims: We resol…

2010 Astronomy and Astrophysics
eHST 16
An Optical-infrared Study of the Young Multipolar Planetary Nebula NGC 6644
DOI: 10.1088/0004-637X/725/1/173 Bibcode: 2010ApJ...725..173H

Zhang, Yong; Volk, Kevin; Kwok, Sun +2 more

High-resolution Hubble Space Telescope imaging of the compact planetary nebula NGC 6644 has revealed two pairs of bipolar lobes and a central ring lying close to the plane of the sky. From mid-infrared imaging obtained with the Gemini Telescope, we have found a dust torus which is oriented nearly perpendicular to one pair of the lobes. We suggest …

2010 The Astrophysical Journal
IUE eHST 16
Tiny Pores Observed by Hinode/Solar Optical Telescope
DOI: 10.1088/0004-637X/723/1/440 Bibcode: 2010ApJ...723..440C

Chae, Jongchul; Cho, Kyung-Suk; Kim, Yeon-Han +2 more

The study of pores, small penumbraless sunspots, can give us a chance to understand how strong magnetic fields interact with convective motions in the photosphere. For a better understanding of this interaction, we investigate the temporal variation of several tiny pores smaller than 2''. These pores were observed by the Solar Optical Telescope on…

2010 The Astrophysical Journal
Hinode 16
Sublimation of the Martian CO 2 Seasonal South Polar Cap
DOI: 10.1016/j.pss.2010.03.018 Bibcode: 2010P&SS...58.1129S

Bibring, Jean-Pierre; Langevin, Yves; Martin, Patrick +6 more

The polar condensation/sublimation of CO 2, that involve about one fourth of the atmosphere mass, is the major Martian climatic cycle. Early observations in visible and thermal infrared have shown that the sublimation of the Seasonal South Polar Cap (SSPC) is not symmetric around the geographic South Pole. Here we use observations by OM…

2010 Planetary and Space Science
MEx 16
Source mechanism of Saturn narrowband emission
DOI: 10.5194/angeo-28-1013-2010 Bibcode: 2010AnGeo..28.1013M

Cecconi, B.; Menietti, J. D.; Rymer, A. M. +2 more

Narrowband emission (NB) is observed at Saturn centered near 5 kHz and 20 kHz and harmonics. This emission appears similar in many ways to Jovian kilometric narrowband emission observed at higher frequencies, and therefore may have a similar source mechanism. Source regions of NB near 20 kHz are believed to be located near density gradients in the…

2010 Annales Geophysicae
Cassini 16
Orbit Determination of Double-lined Spectroscopic Binaries by Fitting the Revised Hipparcos Intermediate Astrometric Data
DOI: 10.1088/0004-6256/139/5/1975 Bibcode: 2010AJ....139.1975R

Ren, Shulin; Fu, Yanning

Untill now, the Hipparcos intermediate astrometric data (HIAD) have contributed little to the full orbit determination of double-lined spectroscopic binaries (SB2s). This is because the photocenter of such a binary system is usually not far from the system mass center, and its orbital wobble is generally weak with respect to the accuracy of the HI…

2010 The Astronomical Journal
Hipparcos 16
Comparison of eight years magnetic field data from Cluster with Tsyganenko models in the inner magnetosphere
DOI: 10.5194/angeo-28-309-2010 Bibcode: 2010AnGeo..28..309Z

Woodfield, E. E.; Dunlop, M. W.; Zhang, Q. -H. +1 more

Eight years of magnetic field data, taken while the four Cluster spacecraft pass through, or adjacent to, the equatorial ring current, have been surveyed to investigate the effects on the Earth's magnetic field of the externally driven current systems connecting the ionosphere, cusp and ring current regions. This study extends previous work to cov…

2010 Annales Geophysicae
Cluster 16
A multilayer model for thermal infrared emission of Saturn’s rings II: Albedo, spins, and vertical mixing of ring particles inferred from Cassini CIRS
DOI: 10.1016/j.icarus.2010.06.032 Bibcode: 2010Icar..210..330M

Altobelli, Nicolas; Spilker, Linda; Ohtsuki, Keiji +3 more

Since the Saturn orbit insertion of the Cassini spacecraft in mid-2004, the Cassini composite infrared spectrometer (CIRS) measured temperatures of Saturn's main rings at various observational geometries. In the present study, we apply our new thermal model (Morishima, R., Salo, H., Ohtsuki, K. [2009]. Icarus 201, 634-654) for fitting to the early…

2010 Icarus
Cassini 16