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Extreme Ultra-Violet Spectroscopy of the Lower Solar Atmosphere During Solar Flares (Invited Review)
DOI: 10.1007/s11207-015-0748-2 Bibcode: 2015SoPh..290.3399M

Milligan, Ryan O.

The extreme ultra-violet (EUV) portion of the solar spectrum contains a wealth of diagnostic tools for probing the lower solar atmosphere in response to an injection of energy, particularly during the impulsive phase of solar flares. These include temperature- and density-sensitive line ratios, Doppler-shifted emission lines, nonthermal broadening…

2015 Solar Physics
Hinode PROBA-2 53
Suprathermal electron environment of comet 67P/Churyumov-Gerasimenko: Observations from the Rosetta Ion and Electron Sensor
DOI: 10.1051/0004-6361/201526351 Bibcode: 2015A&A...583A..24C

Frahm, R. A.; Goldstein, R.; Mokashi, P. +9 more

Context. The Rosetta spacecraft is currently escorting comet 67P/Churyumov-Gerasimenko until its perihelion approach at 1.2 AU. This mission has provided unprecedented views into the interaction of the solar wind and the comet as a function of heliocentric distance.
Aims: We study the interaction of the solar wind and comet at large heliocent…

2015 Astronomy and Astrophysics
Rosetta 53
Control of the topside Martian ionosphere by crustal magnetic fields
DOI: 10.1002/2014JA020703 Bibcode: 2015JGRA..120.3042A

Gurnett, D. A.; Edberg, N. J. T.; Němec, F. +4 more

We present observations from the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) instrument onboard Mars Express of the thermal electron plasma density of the Martian ionosphere and investigate the extent to which it is influenced by the presence of Mars's remnant crustal magnetic fields. We use locally measured electron densi…

2015 Journal of Geophysical Research (Space Physics)
MEx 53
Mixtures of clays and sulfates within deposits in western Melas Chasma, Mars
DOI: 10.1016/j.icarus.2014.04.009 Bibcode: 2015Icar..251..291W

Wray, James J.; Weitz, Catherine M.; Noe Dobrea, Eldar

We have utilized several data sets from multiple spacecraft that have been acquired over a continuous observation campaign across the southwestern Melas Chasma region of Mars. The blocky deposit observed on the chasma floor and on portions of the southern wallrock consists of mixtures of light- and medium-toned materials that exhibit displacement …

2015 Icarus
MEx 53
THOR: The H i, OH, Recombination line survey of the Milky Way. The pilot study: H i observations of the giant molecular cloud W43
DOI: 10.1051/0004-6361/201425370 Bibcode: 2015A&A...580A.112B

Menten, K. M.; Hill, T.; Henning, T. +30 more

To study the atomic, molecular, and ionized emission of giant molecular clouds (GMCs) in the Milky Way, we initiated a large program with the Karl G. Jansky Very Large Array (VLA): "THOR: The H i, OH, Recombination line survey of the Milky Way". We map the 21 cm H i line, 4 OH lines, up to 19 Hα recombination lines and thecontinuum from 1 to 2 GHz…

2015 Astronomy and Astrophysics
Herschel 53
What Are Little Worlds Made Of? Stellar Abundances and the Building Blocks of Planets
DOI: 10.1088/0004-637X/804/1/40 Bibcode: 2015ApJ...804...40G

Gaidos, Eric

If the photospheres of solar-type stars represent the composition of circumstellar disks from which any planets formed, spectroscopic determinations of stellar elemental abundances offer information on the composition of those planets, including smaller, rocky planets. In particular, the C/O ratio is proposed to be a key determinant of the composi…

2015 The Astrophysical Journal
eHST 53
MRK 1216 and NGC 1277 - an orbit-based dynamical analysis of compact, high-velocity dispersion galaxies
DOI: 10.1093/mnras/stv1381 Bibcode: 2015MNRAS.452.1792Y

Gebhardt, Karl; van de Ven, Glenn; Husemann, Bernd +5 more

We present a dynamical analysis to infer the structural parameters and properties of the two nearby, compact, high-velocity dispersion galaxies MRK 1216 and NGC 1277. Combining deep Hubble Space Telescope imaging, wide-field integral field unit stellar kinematics, and complementary long-slit spectroscopic data out to three effective radii, we cons…

2015 Monthly Notices of the Royal Astronomical Society
eHST 53
Excitation of Chirping Whistler Waves in a Laboratory Plasma
DOI: 10.1103/PhysRevLett.114.245002 Bibcode: 2015PhRvL.114x5002V

Bortnik, J.; Thorne, R. M.; Van Compernolle, B. +3 more

Whistler mode chorus emissions with a characteristic frequency chirp are important magnetospheric waves, responsible for the acceleration of outer radiation belt electrons to relativistic energies and also for the scattering loss of these electrons into the atmosphere. Here, we report on the first laboratory experiment where whistler waves exhibit…

2015 Physical Review Letters
Cluster 53
New binaries among UV-selected, hot subdwarf stars and population properties
DOI: 10.1093/mnras/stv821 Bibcode: 2015MNRAS.450.3514K

Buckley, D. A. H.; Vennes, S.; Németh, P. +4 more

We have measured the orbital parameters of seven close binaries, including six new objects, in a radial velocity survey of 38 objects comprising a hot subdwarf star with orbital periods ranging from ∼0.17 to 3 d. One new system, GALEX J2205-3141, shows reflection on an M dwarf companion. Three other objects show significant short-period variations…

2015 Monthly Notices of the Royal Astronomical Society
IUE 53
Modelling the extreme X-ray spectrum of IRAS 13224-3809
DOI: 10.1093/mnras/stu2087 Bibcode: 2015MNRAS.446..759C

Fabian, A. C.; Gallo, L. C.; Wilkins, D. R. +2 more

The extreme narrow-line Seyfert 1 galaxy IRAS 13224-3809 shows significant variability, frequency-dependent time lags, and strong Fe K line and Fe L features in the long 2011 XMM-Newton observation. In this work, we study the spectral properties of IRAS 13224-3809 in detail, and carry out a series of analyses to probe the nature of the source, foc…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 53