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Beyond the Minisolar Maximum of Solar Cycle 24: Declining Solar Magnetic Fields and the Response of the Terrestrial Magnetosphere
DOI: 10.1029/2019JA026616 Bibcode: 2019JGRA..124.6363I

Janardhan, P.; Ingale, M.; Bisoi, S. K.

The present study examines the response of the terrestrial magnetosphere to the long-term steady declining trends observed in solar magnetic fields and solar wind microturbulence levels since mid-1990s that has been continuing beyond the minisolar maximum of cycle 24. A detailed analysis of the response of the terrestrial magnetosphere has been ca…

2019 Journal of Geophysical Research (Space Physics)
Cluster 12
UV to X-Ray Comptonization Delay in Mrk 493
DOI: 10.3847/2041-8213/aaf8ab Bibcode: 2019ApJ...870L..13A

Dewangan, Gulab C.; Pal, Main; Pawar, Pramod +1 more

The broadband X-ray emission from type 1 active galactic nuclei, dominated by a power-law continuum, is thought to arise from repeated inverse Compton scattering of seed optical/UV photons by energetic electrons in a hot corona. The seed optical/UV photons are assumed to arise from an accretion disk, but direct observational evidence has remained …

2019 The Astrophysical Journal
XMM-Newton 12
Measuring the expansion and age of the nova shell IPHASX J210204.7 + 471015
DOI: 10.1093/mnras/sty3364 Bibcode: 2019MNRAS.483.3773S

Guerrero, M. A.; Toalá, J. A.; Santamaría, E. +4 more

The parallax expansion and kinematics of a nova shell can be used to assess its age and distance, and to investigate the interaction of the ejecta with the circumstellar medium. These are key to understand the expansion and dispersal of the nova ejecta in the Galaxy. Multi-epoch images and high-dispersion spectroscopic observations of the recently…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
First Evidence of Enhanced Recombination in Astrophysical Environments and the Implications for Plasma Diagnostics
DOI: 10.3847/2041-8213/ab5954 Bibcode: 2019ApJ...887L...9N

Dupree, A. K.; Raymond, J.; García-Rojas, J. +6 more

We report the first unambiguous observational evidence of Rydberg Enhanced Recombination (RER), a potentially important recombination mechanism that has hitherto been unexplored in low-temperature photoionized plasmas. RER shares similarities with dielectronic recombination, with the difference that the electron is captured into a highly excited s…

2019 The Astrophysical Journal
IUE 12
Migrating Scarps as a Significant Driver for Cometary Surface Evolution
DOI: 10.1029/2019GL083982 Bibcode: 2019GeoRL..4612794B

Soderblom, J. M.; Davidsson, B.; Oklay, N. +10 more

Rosetta observations of 67P/Churyumov-Gerasimenko (67P) reveal that most changes occur in the fallback-generated smooth terrains, vast deposits of granular material blanketing the comet's northern hemisphere. These changes express themselves both morphologically and spectrally across the nucleus, yet we lack a model that describes their formation …

2019 Geophysical Research Letters
Rosetta 12
TOPCAT and Gaia
DOI: 10.48550/arXiv.1811.09480 Bibcode: 2019ASPC..523...43T

Taylor, M. B.

TOPCAT, and its command line counterpart STILTS, are powerful tools for working with large source catalogs. ESA's Gaia mission, most recently with its second data release, is producing source catalogs of unprecedented quality for more than a billion sources. This paper presents some examples of how TOPCAT and STILTS can be used for analysis of Gai…

2019 Astronomical Data Analysis Software and Systems XXVII
Gaia 12
Study of Sunspot Penumbra to Umbra Area Ratio Using Kodaikanal White-light Digitised Data
DOI: 10.1007/s11207-019-1462-2 Bibcode: 2019SoPh..294...72J

Banerjee, Dipankar; Jha, Bibhuti Kumar; Mandal, Sudip

We study the long-term behaviour of the sunspot penumbra to umbra area ratio by analysing recently digitised Kodaikanal white-light data (1923 - 2011). We implement an automatic umbra extraction method and compute the ratio over eight solar cycles (Cycles 16 - 23). Although the average ratio does not show any variation with spot latitudes, cycle p…

2019 Solar Physics
SOHO 12
IMF By Influence on Magnetospheric Convection in Earth's Magnetotail Plasma Sheet
DOI: 10.1029/2019GL084190 Bibcode: 2019GeoRL..4611698P

Hamrin, M.; Tenfjord, P.; Laundal, K. M. +7 more

We use Geotail, Cluster, and Time History of Events and Macroscale Interactions during Substorms data over 15 years (1995-2009) to statistically investigate convective ion flows (V⊥xy<200 km/s) in the magnetotail plasma sheet under the influence of a clearly nonzero dawn-dusk interplanetary magnetic field (IMF By). We find…

2019 Geophysical Research Letters
Cluster 12
A nitrogen-enhanced metal-poor star discovered in the globular cluster ESO280-SC06
DOI: 10.1093/mnras/stz2611 Bibcode: 2019MNRAS.490..741S

Martell, Sarah L.; Simpson, Jeffrey D.

We report the discovery of the only very nitrogen-enhanced metal-poor star known in a Galactic globular cluster. This star, in the very metal-poor cluster ESO280-SC06 , has [N/Fe] > +2.5, while the other stars in the cluster show no obvious enhancement in nitrogen. Around 80 NEMP stars are known in the field, and their abundance patterns are be…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
Recent Advancements and Remaining Challenges Associated With Inner Magnetosphere Cross-Energy/Population Interactions (IMCEPI)
DOI: 10.1029/2018JA026282 Bibcode: 2019JGRA..124..886Y

Jordanova, Vania K.; Yu, Yiqun; Liemohn, Mike W. +2 more

The geospace inner magnetosphere, within about 10 Earth radii, contains various plasma populations with energy from a few electron volts to megaelectron volts and plays important roles in regulating the energy density of the magnetosphere, the magnetic field configuration, and wave dynamics. As an integrated part of the magnetosphere, the inner ma…

2019 Journal of Geophysical Research (Space Physics)
Cluster 12