Search Publications

Reconstructing the cruise-phase trajectory of deep-space probes in a general relativistic framework: An application to the Cassini gravitational wave experiment
DOI: 10.1007/s42064-023-0160-x Bibcode: 2023AsDyn...7..301O

Barriot, Jean-Pierre; O'Leary, Joseph

Einstein's theory of general relativity is playing an increasingly important role in fields such as interplanetary navigation, astrometry, and metrology. Modern spacecraft and interplanetary probe prediction and estimation platforms employ a perturbed Newtonian framework, supplemented with the Einstein-Infeld-Hoffmann n-body equations of motion. W…

2023 Astrodynamics
Cassini 0
New atomic data for C I Rydberg states compared with solar UV spectra
DOI: 10.1093/mnras/stad2736 Bibcode: 2023MNRAS.526.1396S

Del Zanna, G.; Storey, P. J.; Dufresne, R. P.

We use the Breit-Pauli R-matrix method to calculate accurate energies and radiative data for states in C I up to n = 30 and with l ≤ 3. We provide the full data set of decays to the five 2s2 2p2 ground configuration states 3P0,1,2, 1D2, and 1S0. This is the fir…

2023 Monthly Notices of the Royal Astronomical Society
SOHO 0
The Influence of Oxygen Ions on the Formation of a Thin Current Sheet in the Magnetotail
DOI: 10.1134/S0010952523700259 Bibcode: 2023CosRe..61..218D

Malova, H. V.; Popov, V. Yu.; Zelenyi, L. M. +2 more

A thin current sheet in the Earth's magnetotail with characteristic thickness of one to several proton gyroradii is often observed during magnetospheric disturbances named substorms, when a relatively thick current configuration in the magnetotail is narrowed to an extremely small thickness and then can spontaneously be destroyed. The current-shee…

2023 Cosmic Research
Cluster 0
Sub-Auroral Flows and Associated Magnetospheric and Ionospheric Phenomena Developed During 7-8 September 2017
DOI: 10.1029/2022JA030966 Bibcode: 2023JGRA..12830966H

Horvath, Ildiko; Lovell, Brian C.

This study investigates the Sub-Auroral Polarization Streams (SAPS) and Sub-Auroral Ion Drifts (SAID) along with the associated magnetospheric and ionospheric phenomena developed during 7-8 September 2017. Then, a series of substorms occurred before and during the geomagnetic storm (SYM-Hmin = -146 nT). Results are obtained by utilizing…

2023 Journal of Geophysical Research (Space Physics)
Cluster 0
The Pleiades flare stars in the Gaia era
DOI: 10.52526/25792776-23.70.2-242 Bibcode: 2023CoBAO..70..242T

Ghazaryan, S.; Hambaryan, V.; Hambardzumyan, L. +3 more

We study the six-dimensional arrangement of flare stars in the Pleiades cluster region using the third release of the Gaia–mission (Gaia DR3) and we provide preliminary, a new, original view of the spatial configuration of the flare "star-members" of the cluster.

2023 Communications of the Byurakan Astrophysical Observatory
Gaia 0
Generating a unified catalogue of open clusters and their most probable members
Bibcode: 2023BAAA...64..102P

Perren, G. I.; Pera, M. S.; Navone, H. D. +1 more

In this work we present the largest database of open clusters catalogued to date. To obtain it we combine almost a dozen existing databases of open clusters to generate a cross-matched list of more than 5000 unique objects, scattered throughout the Galaxy. In addition, we process around 2000 of these clusters with a new membership algorithm code; …

2023 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 0
Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
DOI: 10.1051/0004-6361/202245606 Bibcode: 2023A&A...672A.166S

Palicio, P. A.; Vazdekis, A.; Sánchez-Blázquez, P. +1 more

Context. The X-shooter Spectral Library (XSL) is a large empirical stellar library used as a benchmark for the development of stellar population models. The inclusion of α-element abundances is crucial to disentangling the chemical evolution of any stellar system.
Aims: The aim of this paper is to provide a catalogue of high-precision, accura…

2023 Astronomy and Astrophysics
Gaia 0
A Surrogate Model for Studying Solar Energetic Particle Transport and the Seed Population
DOI: 10.1029/2023SW003593 Bibcode: 2023SpWea..2103593B

Schwadron, Nathan A.; Baydin, Atilim Guneş; Poduval, Bala

The high energy particles originating from the Sun, known as solar energetic particles (SEPs), contribute significantly to the space radiation environment, posing serious threats to astronauts and scientific instruments on board spacecraft. The mechanism that accelerates the SEPs to the observed energy ranges, their transport in the inner heliosph…

2023 Space Weather
Ulysses 0
Markov Chain Monte Carlo Optimization applied to Dysonís Visual Double Stars
DOI: 10.48550/arXiv.2306.15100 Bibcode: 2023JAVSO..51..180S

Budding, E.; Banks, T.; Si, I. S. X. +1 more

Estimates of orbital parameters were made using a Bayesian optimization technique on astrometric data for 25 visual binary systems catalogued a century ago by the ninth Astronomer Royal, Sir Frank Dyson. An advantage of this method is that it provides reliable, unbiased uncertainty estimates for the optimized parameters. Reasonable agreement is fo…

2023 Journal of the American Association of Variable Star Observers (JAAVSO)
Gaia 0
The second Venus flyby of BepiColombo mission reveals stable atmosphere over decades
DOI: 10.1038/s41467-023-43888-7 Bibcode: 2023NatCo..14.8225H

Haus, Rainer; Arnold, Gabriele; Hiesinger, Harald +4 more

Studies of the Venusian mesosphere provide important information about the current state of the entire Venusian atmosphere. This includes information about the dense cloud structure, its vertical thermal profile, temperature fields, and the resulting dynamical and meteorological processes that contribute to a deeper understanding of the climatolog…

2023 Nature Communications
BepiColombo 0