Search Publications

Estimation of the Reconnection Electric Field in the 2003 October 29 X10 Flare
DOI: 10.1088/0004-637X/732/1/15 Bibcode: 2011ApJ...732...15Y

Krucker, Säm; Cheng, C. Z.; Yang, Ya-Hui +1 more

The electric field in the reconnecting current sheet of the 2003 October 29 X10 flare is estimated to be a few kV m-1 in this study, based on the rate of change in the photospheric magnetic flux in the newly brightened areas of Transition Region and Coronal Explorer (TRACE) UV ribbons. For comparison, the motion speed of Reuven Ramaty H…

2011 The Astrophysical Journal
SOHO 12
Coronal Transient Events During Two Solar Minima: Their Solar Source Regions and Interplanetary Counterparts
DOI: 10.1007/s11207-011-9769-7 Bibcode: 2011SoPh..274..233C

Mandrini, C. H.; Dasso, S.; Cremades, H.

In the frame of two coordinated observational and research efforts, two full solar rotations were investigated in the times of two distinct solar minima. These two campaigns were dubbed Whole Sun Month (WSM; 10 August - 8 September 1996) and Whole Heliosphere Interval (WHI; 20 March - 16 April 2008). The nearly uninterrupted gathering of solar cor…

2011 Solar Physics
SOHO 12
Quasi-periodic flares in EXO 2030+375 observed with INTEGRAL
DOI: 10.1051/0004-6361/201118185 Bibcode: 2011A&A...536L...8K

Klochkov, D.; Santangelo, A.; Ferrigno, C. +5 more

Context. Episodic flaring activity is a common feature of X-ray pulsars in HMXBs. In some Be/X-ray binaries flares were observed in quiescence or prior to outbursts. EXO 2030+375 is a Be/X-ray binary showing "normal" outbursts almost every ~46 days, near periastron passage of the orbital revolution. Some of these outbursts were occasionally monito…

2011 Astronomy and Astrophysics
INTEGRAL 12
The Disappearing Solar Filament of 2003 June 11: A Three-body Problem
DOI: 10.1088/0004-637X/743/2/202 Bibcode: 2011ApJ...743..202B

Panasenco, O.; Balasubramaniam, K. S.; Pevtsov, A. A. +2 more

The eruption of a large quiescent filament on 2003 June 11 was preceded by the birth of a nearby active region—a common scenario. In this case, however, the filament lay near a pre-existing active region and the new active region did not destabilize the filament by direct magnetic connection. Instead it appears to have done so indirectly via magne…

2011 The Astrophysical Journal
SOHO 12
SAID/SAPS-related VLF waves and the outer radiation belt boundary
DOI: 10.1029/2011GL049613 Bibcode: 2011GeoRL..3821101M

Mishin, Evgeny; Santolik, Ondrej; Albert, Jay

We explore Cluster and CRRES observations of plasmaspheric broadband hiss-like VLF emissions related with subauroral ion drifts/polarization streams (SAID/SAPS) to numerically simulate losses of energetic outer zone electrons due to wave-particle interactions. These emissions represent a distinctive subset of substorm/storm-related VLF activity in…

2011 Geophysical Research Letters
Cluster 12
Study of inertial kinetic Alfven waves around cusp region
DOI: 10.1016/j.pss.2010.11.006 Bibcode: 2011P&SS...59..306A

Agarwal, P.; Varma, P.; Tiwari, M. S.

The effect of electron inertia on kinetic Alfven wave has been studied. The expressions for the dispersion relation, growth/damping rate and growth/damping length of the inertial kinetic Alfven wave (IKAW) are derived using the kinetic approach in cusp region. The Vlasov-kinetic theory has been adopted to evaluate the dispersion relation, growth/d…

2011 Planetary and Space Science
Cluster 12
XMM-Newton first X-ray detection of the low-ionization broad absorption line quasar PG 1700+518
DOI: 10.1111/j.1365-2966.2011.18883.x Bibcode: 2011MNRAS.415.2600B

Vignali, C.; Schartel, N.; Ballo, L. +1 more

We report the first high-energy detection of PG 1700+518, a well-known low-ionization broad absorption line quasar (quasi-stellar object, QSO). Due to previous X-ray non-detection, it was classified as soft X-ray weak QSO. We observed PG 1700+518 with XMM-Newton for about 60 ks divided in three exposures. The spectrum below 2 keV is very steep, Γ∼…

2011 Monthly Notices of the Royal Astronomical Society
IUE XMM-Newton eHST 12
The nearby eclipsing stellar system δ Velorum. III. Self-consistent fundamental parameters and distance
DOI: 10.1051/0004-6361/201116896 Bibcode: 2011A&A...532A..50M

Schertl, D.; Kervella, P.; Natta, A. +6 more

Context. The triple stellar system δ Vel (composed of two A-type and one F-type main-sequence stars) is particularly interesting because it contains one of the nearest and brightest eclipsing binaries. It therefore presents a unique opportunity to determine independently the physical properties of the three components of the system, as well as its…

2011 Astronomy and Astrophysics
Hipparcos 12
The Suzaku Discovery of A Hard Power-Law Component in the Spectra of Short Bursts from SGR 0501+4516
DOI: 10.1093/pasj/63.sp3.S813 Bibcode: 2011PASJ...63S.813N

Enoto, Teruaki; Makishima, Kazuo; Nakagawa, Yujin E.

Using data with the Suzaku XIS and HXD, spectral studies of short bursts from the soft gamma repeater SGR 0501 $+$ 4516 were performed. In total, 32 bursts were detected during the $\sim\ $

2011 Publications of the Astronomical Society of Japan
Suzaku 12
High-speed flowing plasmas in the Earth's plasma sheet
DOI: 10.1007/s11434-011-4361-y Bibcode: 2011ChSBu..56.1182F

Parks, George; Fu, SuiYan; Sun, WeiJie +4 more

A research topic of great interest to the space physics community is the observation of plasmas flowing at hundreds of kilometers per second in the Earth's plasma sheet. Although considerable effort has been made to understand the source of fast-flowing plasmas, many questions remain unanswered about the mechanisms that produce high-speed flows an…

2011 Chinese Science Bulletin
Cluster DoubleStar 12