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Spectral manifestations of extremely strong magnetic fields in the sunspot umbra
Lozitsky, V. G.
Fine peculiarities of the Zeeman effect in two big sunspots of October 29, 2003, and October 25, 2014, are analyzed. In order to search spectral evidences of very strong spatially unresolved magnetic fields, the Stokes I ± V and V profiles of the Fe I 6301.5 and 6302.5 Å lines are studied in detail. Confirmed are two effects discovered earlier by …
Sunward-propagating Solar Energetic Electrons inside Multiple Interplanetary Flux Ropes
Temmer, Manuela; Veronig, Astrid; Dresing, Nina +8 more
On 2013 December 2 and 3, the SEPT and STE instruments on board STEREO-A observed two solar energetic electron events with unusual sunward-directed fluxes. Both events occurred during a time interval showing typical signatures of interplanetary coronal mass ejections (ICMEs). The electron timing and anisotropies, combined with extreme-ultraviolet …
Night side distribution of SO2 content in Venus' upper mesosphere
Montmessin, F.; Bertaux, J. -L.; Fedorova, A. A. +6 more
In this paper we present the first night side distribution of SO2 content in Venus' upper mesosphere (altitudes from 85 to 105 km). The dataset is based on the SPICAV UV stellar occultation experiment which took place onboard ESA's Venus Express (VEX) orbiter in 2006-2014. The UV channel of SPICAV spectrometer detected absorption bands …
Locating dayside magnetopause reconnection with exhaust ion distributions
Fuselier, S. A.; Trattner, K. J.; Broll, J. M.
Magnetic reconnection at Earth's dayside magnetopause is essential to magnetospheric dynamics. Determining where reconnection takes place is important to understanding the processes involved, and many questions about reconnection location remain unanswered. We present a method for locating the magnetic reconnection X line at Earth's dayside magnet…
Thermal Structure and Composition
Encrenaz, Thérèse; Smith, Michael D.; Bougher, Stephen W. +2 more
OMEGA - OSIRIS Mapping of Emission-line Galaxies in A901/2 - III. Galaxy properties across projected phase space in A901/2
Chies-Santos, Ana L.; Wolf, Christian; Aragón-Salamanca, Alfonso +6 more
We conduct a comprehensive projected phase-space analysis of the A901/2 multicluster system at z ∼ 0.165. Aggregating redshifts from spectroscopy, tunable-filter imaging and prism techniques, we assemble a sample of 856 cluster galaxies reaching 108.5 M⊙ in stellar mass. We look for variations in cluster galaxy properties bet…
Stacked Average Far-infrared Spectrum of Dusty Star-forming Galaxies from the Herschel/SPIRE Fourier Transform Spectrometer
Pearson, Chris; Clements, David L.; Valtchanov, Ivan +13 more
We present stacked average far-infrared spectra of a sample of 197 dusty star-forming galaxies (DSFGs) at 0.005< z< 4 using about 90% of the Herschel Space Observatory SPIRE Fourier Transform Spectrometer (FTS) extragalactic data archive based on 3.5 years of science operations. These spectra explore an observed-frame 447-1568 GHz frequency …
Orbiting a binary. SPHERE characterisation of the HD 284149 system
Avenhaus, H.; Fantinel, D.; Messina, S. +53 more
Aims: In this paper we present the results of the SPHERE observation of the
Methods: We observed
A systematic analysis of the XMM-Newton background: I. Dataset and extraction procedures
Tiengo, Andrea; De Luca, Andrea; Marelli, Martino +6 more
XMM-Newton is the direct precursor of the future ESA ATHENA mission. A study of its particle-induced background provides therefore significant insight for the ATHENA mission design. We make use of ∼12 years of data, products from the third XMM-Newton catalog as well as FP7 EXTraS project to avoid celestial sources contamination and to disentangle …
Detection of Extraplanar Diffuse Ionized Gas in M83
Gallagher, J. S., III; Boettcher, Erin; Zweibel, Ellen G.
We present the first kinematic study of extraplanar diffuse ionized gas (eDIG) in the nearby, face-on disk galaxy M83 using optical emission-line spectroscopy from the Robert Stobie Spectrograph on the Southern African Large Telescope. We use a Markov Chain Monte Carlo method to decompose the [N II]λ λ 6548, 6583, Hα, and [S II]λ λ 6717, 6731 emis…