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Dipolarization Observed by TC1 and Cluster During Substorm in Sep. 14, 2004
DOI: 10.1002/cjg2.1104 Bibcode: 2007ChJG...50..866C

Dunlop, M. W.; Reme, H.; Korth, A. +12 more

We study the substorm dipolarization occurring from 1730 to 1930 UT on Sep 14, 2004 based on DSP/TC1, Cluster and Polar data, combined with the aurora and geosynchronous energetic particle measurements and ground-based magnetic field observations. During this time period the IMF was continuously southward. Substorm onset started at about 1822 UT. …

2007 Chinese Journal of Geophysics
Cluster DoubleStar 0
Erratum to “An analysis of solar radio burst events on December 1, 2004” [Adv. Space Res. 39 (2007) 1441 1446]
DOI: 10.1016/j.asr.2007.06.019 Bibcode: 2007AdSpR..40.1543H

Liu, Yuying; Yan, Yihua; Huang, Jing

2007 Advances in Space Research
SOHO 0
The evolution of a complex solar radio burst corresponding to special configuration of microwave sources
DOI: 10.1016/j.asr.2007.04.025 Bibcode: 2007AdSpR..39.1474X

Liu, Y. Y.; Xie, R. X.; Ren, D. B.

A complex radio burst associated with periodic (∼1 and 6 min) pulsations and several kinds fine structures, e.g., normal- and reverse-drifting type III bursts, zebra patterns, and slowly drifting structure was observed with the radio spectrometers (1.0-2.0, 2.6-3.8, 5.2-7.6, and 0.65-1.5 GHz) at the National Astronomical Observatories of China (NA…

2007 Advances in Space Research
SOHO 0
Constraints on Simplified Quartessence Cosmology from the Latest Observational Data
DOI: 10.1142/S0218271807011085 Bibcode: 2007IJMPD..16.1783W

Wu, Puxun; Dong, Sumei

The simplified generalized Chaplygin gas (GCG) model as a candidate of UDME is studied in this paper. By using the latest 162 ESSENCE type Ia supernovae (Sne Ia) data, 30 high red shift Sne Ia data and the distance ratio from z = 0.35 to z = 1089 (the red shift of decoupling), we obtain Ω k = 0.076-0.077+0.093 and …

2007 International Journal of Modern Physics D
eHST 0
Multipoint Analysis of the Rapid Convection Event
DOI: 10.1002/cjg2.1128 Bibcode: 2007ChJG...50.1100M

Dandouras, I.; Lucek, E.; Reme, H. +4 more

Basing on the data from three satellites of Cluster (C1, C3 and C4) in the years of 2001 and 2002, we examine the relationship between the rapid convection event (RCE) and substorm. The observation of RCE measured by single satellite can not exactly describe what happens in the magnetotail. Both C1 and C3 observed the event occurring on July 25, 2…

2007 Chinese Journal of Geophysics
Cluster 0
Erratum to “Titan's surface albedo variations over a Titan season from near-infrared CFHT/FTS spectra”. [Planetary and Space Science 54 (2006) 1225 1246]
DOI: 10.1016/j.pss.2007.02.006 Bibcode: 2007P&SS...55.2221N

Lellouch, E.; Rannou, P.; Coustenis, A. +5 more

2007 Planetary and Space Science
Cassini 0
Plasma - a view from space
DOI: 10.1088/2058-7058/20/4/32 Bibcode: 2007PhyW...20d..30N

Nykyri, K.

2007 Physics World
Cluster 0
Continuous tailward flow in the near-Earth magnetotail observed by TC-1 satellite
DOI: 10.1007/s11434-007-0228-7 Bibcode: 2007ChSBu..52.1980Z

Shen, Chao; Zhang, LingQian; Liu, ZhenXing +2 more

On July 11, 2004, a substorm process in the period of continuous tailward flow was observed by the joint exploration of the TC-1, IMAGE and ACE satellites. The substorm observed by the TC-1 in the near-Earth has three stages: the growth phase (from 11:43 to 12:19), the pre-expansion process (from 12:19 to 12:28) and the dipolarization process. The…

2007 Chinese Science Bulletin
DoubleStar 0
The Discovery of the Nearest Star
Bibcode: 2007MNSSA..66..244G

Glass, I. S.

In the 1830s, the double star α Centauri was the subject of the first successful stellar parallax measurement. For almost eighty years it remained the nearest star known. However, in 1915 at the Union Observatory in Johannesburg, R.T.A. Innes found a faint object near α Cen with a similar proper motion. Its parallax was measured over the following…

2007 Monthly Notes of the Astronomical Society of South Africa
Hipparcos 0
Turbulent and directed mass motions in various structures of the low corona
DOI: 10.1029/2006GI000151 Bibcode: 2007IJGA....7.2004D

Delone, A. B.; Yakunina, G. V.; Porfir'eva, G. A. +1 more

[1] A brief review on turbulent and ordered plasma motions in the solar corona is presented. Velocities in quiet coronal regions, coronal loops, coronal holes, and cavities around quiescent prominences are analyzed. Data based on interferometric observations of several total solar eclipses obtained earlier by the authors and in addition the values…

2007 International Journal of Geomagnetism and Aeronomy
SOHO 0