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Evidences of early aqueous Mars: Implications on the origin of branched valleys in the Ius Chasma, Mars
DOI: 10.1016/j.pss.2017.10.011 Bibcode: 2017P&SS..148...56M

Martha, Tapas R.; Jain, Nirmala; Vamshi, Gasiganti T. +1 more

This study shows results of morphological and spectroscopic analyses of Ius Chasma and its southern branched valleys using Orbiter datasets such as Mars Reconnaissance Orbiter (MRO)-Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), High Resolution Imaging Science Experiment (MRO-HiRISE) and digital terrain model (HRSC-DTM). Result of t…

2017 Planetary and Space Science
MEx 5
Nitrogen condensation in Titan's atmosphere under contemporary atmospheric composition
DOI: 10.1016/j.icarus.2017.02.005 Bibcode: 2017Icar..289..120T

Tokano, Tetsuya

Temperature profiles of Titan's atmosphere obtained by Cassini radio occultations approach the nitrogen condensation temperature curve at some places. This raises the question as to whether nitrogen, Titan's main atmospheric constituent, might condense in some seasons and areas contrary to previous perception. To address this question, possible ar…

2017 Icarus
Cassini 5
XMM-Newton and NuSTAR joint observations of Mrk 915: a deep look into the X-ray properties
DOI: 10.1093/mnras/stx1360 Bibcode: 2017MNRAS.470.3924B

Campana, S.; Moretti, A.; Vignali, C. +5 more

We report on the X-ray monitoring programme (covering slightly more than 11 d) carried out jointly by XMM-Newton and NuSTAR on the intermediate Seyfert galaxy Mrk 915. The light curves extracted in different energy ranges show a variation in intensity but not a significant change in the spectral shape. The X-ray spectra reveal the presence of a tw…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Intermittency of the Solar Magnetic Field and Solar Magnetic Activity Cycle
DOI: 10.1007/s11207-017-1069-4 Bibcode: 2017SoPh..292...44S

Obridko, V. N.; Sokoloff, D. D.; Shibalova, A. S.

Small-scale solar magnetic fields demonstrate features of fractal intermittent behavior, which requires quantification. For this purpose we investigate how the observational estimate of the solar magnetic flux density B depends on resolution D in order to obtain the scaling lnBD=−k lnD +a in a reasonably wide range. The quantity k demon…

2017 Solar Physics
SOHO 4
On IMF By -Induced Dawn-Dusk Asymmetries in Earthward Convective Fast Flows
DOI: 10.1002/9781119216346.ch8 Bibcode: 2017GMS...230...95P

Nilsson, H.; Hamrin, M.; Karlsson, T. +2 more

2017 Dawn-Dusk Asymmetries in Planetary Plasma Environments
Cluster 4
Recent Climate Variations
DOI: 10.1017/9781139060172.016 Bibcode: 2017acm..book..464F

Head, James W.; Byrne, Shane; Mischna, Michael A. +2 more

2017 Asteroids, Comets, Meteors - ACM2017
MEx 4
Photoionization Modeling of Titan’s Dayside Ionosphere
DOI: 10.3847/2041-8213/aa998d Bibcode: 2017ApJ...850L..26S

Wahlund, J. -E.; Edberg, N. J. T.; Vigren, E. +4 more

Previous modeling studies of Titan’s dayside ionosphere predict electron number densities that are roughly a factor of 2 higher than those observed by the RPWS/Langmuir probe. The issue can equivalently be described as the ratio between the calculated electron production rates and the square of the observed electron number densities resulting in r…

2017 The Astrophysical Journal
Cassini 4
Dynamical Study of the Exoplanet Host Binary System HD 106515
DOI: 10.1017/pasa.2016.59 Bibcode: 2017PASA...34....4R

Rica, F. M.; Barrena, R.; Henríquez, J. A. +2 more

HD 106515 AB (STF1619 AB) is a high common proper motion and common radial velocity binary star system composed of two G-type bright stars located at 35 pc and separated by about 7 arcsec. This system was observed by the Hipparcos satellite with a precision in distance and proper motion of 3 and 2%, respectively. The system includes a circumprimar…

2017 Publications of the Astronomical Society of Australia
Hipparcos 4
Modern Geometric Methods of Distance Determination
DOI: 10.1007/s11214-017-0418-9 Bibcode: 2017SSRv..212.1787T

Pietrzyński, Grzegorz; Thévenin, Frédéric; Falanga, Maurizio +2 more

Building a 3D picture of the Universe at any distance is one of the major challenges in astronomy, from the nearby Solar System to distant Quasars and galaxies. This goal has forced astronomers to develop techniques to estimate or to measure the distance of point sources on the sky. While most distance estimates used since the beginning of the 20t…

2017 Space Science Reviews
Gaia 4
The Acheron Dorsum on Mars: A novel interpretation of its linear depressions and a model for its evolution
DOI: 10.1016/j.epsl.2017.02.019 Bibcode: 2017E&PSL.465...92D

Martino, Salvatore; De Blasio, Fabio Vittorio

The Acheron Dorsum north of Olympus Mons on Mars is a unique 800 km-long arcuate ridge apparently unrelated to other adjacent morphologies. Acheron Dorsum is crossed by deep and wide fractures ("fossae", here referred to also as Linear Depressions or "LDs"), commonly interpreted as grabens formed by local lithosphere stress in response to endogeno…

2017 Earth and Planetary Science Letters
MEx 4