Search Publications

Venus lightning: Comparison with terrestrial lightning
DOI: 10.1016/j.pss.2010.02.010 Bibcode: 2011P&SS...59..965R

Russell, C. T.; Wei, H. Y.; Zhang, T. L. +2 more

Terrestrial lightning is generated by the separation of electric charge residing on water-ice particles in clouds, a few kilometers above the electrically conducting surface of the Earth. It is detected optically, electromagnetically, and aurally. The majority of discharges occur within or between clouds with about one third discharging to the sur…

2011 Planetary and Space Science
VenusExpress 17
The M81 Group Dwarf Irregular Galaxy DDO 165. II. Connecting Recent Star Formation with Interstellar Medium Structures and Kinematics
DOI: 10.1088/0004-637X/735/1/36 Bibcode: 2011ApJ...735...36C

Cannon, John M.; Dolphin, Andrew E.; Skillman, Evan D. +8 more

We compare the stellar populations and complex neutral gas dynamics of the M81 group dIrr galaxy DDO 165 using data from the Hubble Space Telescope and the Very Large Array. Cannon et al. in Paper I of this series identified two kinematically distinct H I components, multiple localized high velocity gas features, and eight H I holes and shells (th…

2011 The Astrophysical Journal
eHST 17
AGN feedback and iron enrichment in the powerful radio galaxy, 4C+55.16
DOI: 10.1111/j.1365-2966.2011.18960.x Bibcode: 2011MNRAS.415.3520H

Fabian, A. C.; Hlavacek-Larrondo, J.; Sanders, J. S. +1 more

We present a detailed X-ray analysis of 4C+55.16, an unusual and interesting radio galaxy, located at the centre of a cool core cluster of galaxies. 4C+55.16 is X-ray bright (LX(cluster)∼ 1045 erg s-1), radio powerful, and shows clear signs of interaction with the surrounding intracluster medium (ICM). By combining…

2011 Monthly Notices of the Royal Astronomical Society
eHST 17
“Crater” flux transfer events: Highroad to the X line?
DOI: 10.1029/2010JA015495 Bibcode: 2011JGRA..116.2204F

Farrugia, C. J.; Lucek, E.; André, M. +12 more

We examine Cluster observations of a so-called magnetosphere “crater FTE,” employing data from five instruments (FGM, CIS, EDI, EFW, and WHISPER), some at the highest resolution. The aim of doing this is to deepen our understanding of the reconnection nature of these events by applying recent advances in the theory of collisionless reconnection an…

2011 Journal of Geophysical Research (Space Physics)
Cluster 17
Hypsometry of Titan
DOI: 10.1016/j.icarus.2010.10.002 Bibcode: 2011Icar..211..699L

Lorenz, Ralph D.; Turtle, Elizabeth P.; Le Gall, Alice +6 more

Cassini RADAR topography data are used to evaluate Titan's hypsometric profile, and to make comparisons with other planetary bodies. Titan's hypsogram is unimodal and strikingly narrow compared with the terrestrial planets. To investigate topographic extremes, a novel variant on the classic hypsogram is introduced, with a logarithmic abscissa to h…

2011 Icarus
Cassini 17
Observation of intensity oscillations above X-ray bright points from the Hinode/XRT: signature of magnetohydrodynamic oscillations in the solar corona
DOI: 10.1111/j.1365-2966.2011.18792.x Bibcode: 2011MNRAS.415.1419K

Srivastava, A. K.; Dwivedi, B. N.; Kumar, Mukul

We analyse the temporal image data of the quiet Sun observed by the X-ray Telescope (XRT) onboard the Hinode spacecraft and Al-poly filter on 2007 March 31. We choose these temporal image data of ∼30 s cadence from 11:34:48 UT to 14:19:35 UT to study intensity oscillations above selected X-ray bright points (XBPs) with an exposure time 8.193 s of …

2011 Monthly Notices of the Royal Astronomical Society
Hinode 17
Solar winds along curved magnetic field lines
DOI: 10.1051/0004-6361/201116668 Bibcode: 2011A&A...529A.148L

Chen, Y.; Li, B.; Xia, L. D.

Context. Both remote-sensing measurements using the interplanetary scintillation (IPS) technique and in-situ measurements by the Ulysses spacecraft show a bimodal structure for the solar wind at solar minimum conditions. At present it still remains to address why the fast wind is fast and the slow wind is slow. While a robust empirical correlation…

2011 Astronomy and Astrophysics
Ulysses 17
Synthetic differential emission measure curves of prominence fine structures. II. The SoHO/SUMER prominence of 8 June 2004
DOI: 10.1051/0004-6361/201117429 Bibcode: 2011A&A...535A.122G

Heinzel, P.; Vial, J. -C.; Anzer, U. +2 more


Aims: This study is the first attempt to combine the prominence observations in Lyman, UV, and EUV lines with the determination of the prominence differential emission measure derived using two different techniques, one based on the inversion of the observed UV and EUV lines and the other employing 2D non-LTE prominence fine-structure modelin…

2011 Astronomy and Astrophysics
SOHO 17
Extended dust shell of the carbon star U Hydrae observed with AKARI
DOI: 10.1051/0004-6361/201015163 Bibcode: 2011A&A...528A..29I

Izumiura, H.; Matsunaga, N.; Tanabé, T. +8 more

Context. Low- to intermediate-mass stars lose a significant fraction of their mass while they are on the asymptotic giant branch (AGB). This mass loss is considered to determine the final stages of their evolution. The material ejected from the stellar photosphere forms a circumstellar envelope in its surroundings. Layers of circumstellar envelope…

2011 Astronomy and Astrophysics
AKARI 17
Nonlinear force-free field extrapolation of the coronal magnetic field using the data obtained by the Hinode satellite
DOI: 10.1029/2010JA015610 Bibcode: 2011JGRA..116.1101H

Yan, Yihua; Wang, Huaning; He, Han

The Hinode satellite can obtain high-quality photospheric vector magnetograms of solar active regions and the simultaneous coronal loop images in soft X-ray and extreme ultraviolet (EUV) bands. In this paper, we continue the work of He and Wang (2008) and apply the newly developed upward boundary integration computational scheme for the nonlinear …

2011 Journal of Geophysical Research (Space Physics)
Hinode SOHO 17