Search Publications

The Response of Saturn's Dawn Field-Aligned Currents to Magnetospheric and Ring Current Conditions During Cassini's Proximal Orbits: Evidence for a Region 2 Response at Saturn
DOI: 10.1029/2021JA029852 Bibcode: 2022JGRA..12729852H

Dougherty, M. K.; Roussos, E.; Cowley, S. W. H. +3 more

Cassini's 2017 proximal orbits provided the opportunity to examine the auroral field-aligned currents in the northern hemisphere dawn sector in relation to wider magnetospheric conditions. We combine three recent studies to examine the response of the dawn region auroral field-aligned currents and the azimuthal ring currents to compressions and ex…

2022 Journal of Geophysical Research (Space Physics)
Cassini 1
Stellar population in the vicinity of the H II region G331.03-00.15
DOI: 10.1051/0004-6361/202244381 Bibcode: 2022A&A...666A..96C

Gamen, R.; Cichowolski, S.; Cárdenas, S. B. +1 more

We present a multi-wavelength study of the H II region G331.03-00.15, with the aim of identifying the population of massive stars associated with it. The distributions of ionised gas and heated dust both exhibit similar spherical forms, while the bordering photo-dissociating region follows a very ring-like distribution, indicating the presence of …

2022 Astronomy and Astrophysics
Gaia 1
Plasma Oscillations and Kinetic Instabilities at Ion Scales in the Expanding Magnetosheath
DOI: 10.3847/1538-4357/ac75c0 Bibcode: 2022ApJ...935..106T

Trávníček, Pavel M.; Chaston, Chris C.

We investigate a relationship between a decaying spectrum of magnetic field perturbations and kinetic instabilities in a slowly expanding magnetosheath plasma using two-dimensional hybrid expanding simulations in (X, Y) space. We impose an initial ambient magnetic field B 0/B 0 = (1, 0, 0), and superimpose a flat spectrum of …

2022 The Astrophysical Journal
Cluster 1
The Stellar Abundances and Galactic Evolution Survey: Photonic Passbands and Extinction Coefficients for the u and v Bands
DOI: 10.1088/1674-4527/ac8b5b Bibcode: 2022RAA....22j5004T

Tan, Ke-Feng; Zhao, Gang; Fan, Zhou +6 more

The Stellar Abundances and Galactic Evolution Survey (SAGES) is a multi-band photometric survey focused on estimation of stellar atmospheric parameters and interstellar extinction. In this paper we have derived photonic passbands for the intermediate-band u and v filters of the SAGES photometric system. The derived photonic passbands have been com…

2022 Research in Astronomy and Astrophysics
Gaia 1
An insight to the cryospheric level in Mars: Case study from the Thaumasia Minor
DOI: 10.1016/j.icarus.2021.114725 Bibcode: 2022Icar..37214725D

Dasgupta, Dipayan; Kundu, Abhik; Dasgupta, Nilanjan

The presence of a subsurface Martian cryosphere has been widely acknowledged. Rampart craters and outflow channels are thought to be the prominent geomorphic signatures in support of the presence of this cryospheric layer. Valley networks, on the other hand, are thought to be the signatures of precipitation, seasonal meltwater flow due to glacial …

2022 Icarus
MEx 1
Extragalactic transient candidates in the second Swift-XRT point source catalogue
DOI: 10.1093/mnras/stac1977 Bibcode: 2022MNRAS.515.4402E

O'Brien, P. T.; Starling, R. L. C.; Evans, P. A. +1 more

The second Swift-XRT Point Source catalogue offers a combination of sky coverage and sensitivity and presents an invaluable opportunity for transient discovery. We search the catalogue at the positions of inactive and active galaxies, and identify transient candidates by comparison with XMM-Newton and ROSAT. We recover 167 previously known transie…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
The impact of photospheric brightness field on exoplanetary transit timings and the TTV excess of HD 189733 b
DOI: 10.1093/mnras/stab3073 Bibcode: 2022MNRAS.509.1048B

Baluev, Roman V.

We consider the issue of excessive TTV noise observed for the exoplanet HD 189733 b. Trying to explain it through the host star photospheric activity, we model the stellar surface brightness as a random field, then characterize statistical properties of the resulting transit signal perturbation and compute individual corrections to transit timings…

2022 Monthly Notices of the Royal Astronomical Society
eHST 1
The role of pre-existing faults and fractures in shaping polygonal impact craters and its tectonic implications in the southern Margaritifer Terra region, Mars
DOI: 10.1007/s12040-022-01857-6 Bibcode: 2022JESS..131...97B

Bhattacharya, Satadru; Dasgupta, Dipayan; Kundu, Abhik +2 more

The presence of polygonal-shaped craters, i.e., craters with complete or incomplete polygonal rims along with circular or elliptical outlines, on the surface of celestial bodies has been known for nearly a century. However, many investigations on their distribution and formation have not been carried out, until recently. Scientists have proposed t…

2022 Journal of Earth System Science
MEx 1
Activity of Selected Solar Twins
DOI: 10.1134/S0016793222070131 Bibcode: 2022Ge&Ae..62..903K

Shlyapnikov, A. A.; Katsova, M. M.; Nizamov, B. A.

We analyze various tracers of magnetic activity for 23 solar twins which are characterized by significant scatter of lithium abundance in their atmospheres. A level of coronal and chromospheric activity has been studied from available X-ray and UV-archival data. It gives us a chance to compare coronae of solar twins of various ages with the solar …

2022 Geomagnetism and Aeronomy
XMM-Newton 1
An Effusive Lunar Dome Near Fracastorius Crater: Spectral and Morphometric Properties
DOI: 10.3390/rs14236135 Bibcode: 2022RemS...14.6135A

Ahrens, Caitlin; Lena, Raffaello

We examine a dome within the boundary between Fracastorius crater and Mare Nectaris. The dome has a noticeable vent structure and appears to be perpendicular to wrinkle ridges in the southern Mare Nectaris basin. The spectral signature of this dome, derived from Clementine UVVIS and Chandrayaan-1 M3 reflectance data, revealed that Fracastorius has…

2022 Remote Sensing
Chandrayaan-1 1