Search Publications

Observations of the Magnetic Reconnection Signature of an M2 Flare on 2000 March 23
DOI: 10.1088/0004-637X/703/1/877 Bibcode: 2009ApJ...703..877L

Zhang, Jun; Li, Leping

Multiwavelength observations of an M 2.0 flare event on 2000 March 23 in the NOAA active region 8910 provide us a good chance to study the detailed structure and dynamics of the magnetic reconnection region. In the process of the flare, extreme-ultraviolet (EUV) loops displayed two types of sideward motions upon a loop-top hard X-ray source with a…

2009 The Astrophysical Journal
SOHO 27
High energy variability of 3C 273 during the AGILE multiwavelength campaign of December 2007-January 2008
DOI: 10.1051/0004-6361:200810813 Bibcode: 2009A&A...494...49P

Caraveo, P. A.; Antonelli, L. A.; Costa, E. +52 more

Context: We report the results of a 3-week multi-wavelength campaign targeting the flat spectrum radio quasar 3C 273 carried out with the AGILE gamma-ray mission, covering the 30 MeV-50 GeV and 18-60 keV, the REM observatory (covering the near-IR and optical), Swift (near-UV/Optical, 0.2-10 keV and 15-50 keV), INTEGRAL (3-200 keV) and Rossi XTE (2…

2009 Astronomy and Astrophysics
INTEGRAL 27
Hard X-Ray Spectrum from West Lobe of Radio Galaxy Fornax A Observed with Suzaku
DOI: 10.1093/pasj/61.sp1.S327 Bibcode: 2009PASJ...61S.327T

Tashiro, M. S.; Seta, H.; Isobe, N. +2 more

An observation of the West lobe of radio galaxy Fornax A (NGC 1316) with Suzaku is reported. Since Feigelson et al. (1995) and Kaneda et al. (1995) discovered the cosmic microwave background boosted inverse-Comptonized (IC) X-rays from the radio lobe, the magnetic field and electron energy density in the lobes have been estimated under the assumpt…

2009 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 27
VLT/NACO coronagraphic observations of fine structures in the disk of β Pictoris
DOI: 10.1051/0004-6361:200811067 Bibcode: 2009A&A...495..523B

Augereau, J. -C.; Pantin, E.; Boccaletti, A. +2 more

Aims: We present ground-based observations of the disk around the A-type star β Pictoris to obtain scattered light images at the highest angular resolution (60 mas, equivalent to about 1 AU at the distance of the star) and the highest contrast in the very close environment of the star. The purpose of this program is to perform a close inspection o…

2009 Astronomy and Astrophysics
eHST 27
Low-Power Radio Galaxies in the Distant Universe: A Search for FR I at 1 < z < 2 in the Cosmos Field
DOI: 10.1088/0004-637X/696/2/1103 Bibcode: 2009ApJ...696.1103C

Sparks, W. B.; Chiaberge, Marco; Tremblay, Grant +3 more

We present a search for FR I radio galaxies between 1 < z < 2 in the COSMOS field. In absence of spectroscopic redshift measurements, the selection method is based on multiple steps which make use of both radio and optical constraints. The basic assumptions are that (1) the break in radio power between low-power FR Is and the more powerful F…

2009 The Astrophysical Journal
eHST 27
Is the Martian water table hidden from radar view?
DOI: 10.1029/2009GL038945 Bibcode: 2009GeoRL..3615206F

Gurnett, D. A.; Farrell, W. M.; Plaut, J. J. +4 more

Mars may possess a global sub-surface groundwater table as an integral part of its current hydrological system. However, the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) onboard the Mars Express (MEx) spacecraft has yet to make a definitive detection of such a body of liquid water. In this work, we quantify the conditions t…

2009 Geophysical Research Letters
MEx 27
Mesoscale dynamics on the Sun's surface from HINODE observations
DOI: 10.1051/0004-6361:200811101 Bibcode: 2009A&A...495..945R

Roudier, Th.; Malherbe, J. M.; Meunier, N. +5 more

Context:
Aims: The interactions of velocity scales on the Sun's surface, from granulation to supergranulation are still not understood, nor are their interaction with magnetic fields. We thus aim at giving a better description of dynamics in the mesoscale range which lies between the two scales mentioned above.
Methods: We analyse a 48 h h…

2009 Astronomy and Astrophysics
Hinode 26
Stochastic and direct acceleration mechanisms in the Earth's magnetotail
DOI: 10.1029/2008GL036619 Bibcode: 2009GeoRL..36.4103P

Perri, S.; Zimbardo, G.; Greco, A.

Ion beams with energies of the order of several tens of keV are frequently observed in the Earth's magnetotail. Here we consider two possible acceleration mechanisms, the cross tail electric field E y and the stochastic acceleration due to the electromagnetic fluctuations present in the magnetotail. Electromagnetic perturbations are g…

2009 Geophysical Research Letters
Cluster 26
Structures of Local Galaxies Compared to High-Redshift Star-Forming Galaxies
DOI: 10.1088/0004-6256/138/2/362 Bibcode: 2009AJ....138..362P

Gardner, Jonathan P.; Smith, Linda J.; Lotz, Jennifer M. +4 more

The rest-frame far-ultraviolet morphologies of eight nearby interacting and starburst galaxies (Arp 269, M 82, Mrk 8, NGC 520, NGC 1068, NGC 3079, NGC 3310, and NGC 7673) are compared with 54 galaxies at z ~ 1.5 and 46 galaxies at z ~ 4 observed in the Great Observatories Origins Deep Survey (GOODS) taken with the Advanced Camera for Surveys onboa…

2009 The Astronomical Journal
eHST 26
On the triggering of auroral substorms by northward turnings of the interplanetary magnetic field
DOI: 10.5194/angeo-27-3559-2009 Bibcode: 2009AnGeo..27.3559W

Wild, J. A.; Woodfield, E. E.; Morley, S. K.

Some studies over the last decade have indicated that the instability responsible for substorm expansion phase onset may require an external trigger such as a northward turning of the interplanetary magnetic field (IMF). Statistical investigations have lead to contrasting interpretations regarding the relationship between proposed solar wind trigg…

2009 Annales Geophysicae
Cluster 26