Search Publications

An Integrated Nonlinear Analysis (INA) Software for Space Plasma Turbulence
DOI: 10.1029/2022EA002692 Bibcode: 2023E&SS...1002692M

Echim, Marius; Munteanu, Costel; Kovács, Péter

We built an integrated nonlinear analysis software (INA)-designed to study space plasma turbulence and intermittency. The MATLAB programming environment was used for the algorithmic development and implementation of methods for spectral analysis, multiscale fluctuations and multifractal analysis. The performance of INA is demonstrated using magnet…

2023 Earth and Space Science
Cluster Ulysses 1
Jupiter's equatorial X-ray emissions over two solar cycles
DOI: 10.1093/mnras/stad905 Bibcode: 2023MNRAS.521.5596W

Coates, A. J.; Branduardi-Raymont, G.; Dunn, W. R. +2 more

Jupiter's disc is bright in X-rays as H2 molecules in the atmosphere are very effective at scattering solar X-rays. K-shell fluorescence from carbon atoms in atmospheric methane is thought to also provide a minor contribution. XMM-Newton has now observed Jupiter over a span of nearly two solar cycles from 2003 to 2021, offering the oppo…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
Flapping motion configurations of geomagnetotail current sheet
DOI: 10.1016/j.jastp.2023.106019 Bibcode: 2023JASTP.24306019S

Dunlop, M.; Rong, Zhaojin; Shen, Chao +5 more

We explore the geometry of the flapping motion of geomagnetotail current sheet with the magnetic measurements of the Cluster (constellation) using a newly developed technique. The principal curvatures and directions of the surfaces of the flapping current sheet are successfully deduced by the normal field analysis (NFA). Results show that the dire…

2023 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 1
Analysis of photospheric magnetic fields in AR 12546: a case study
DOI: 10.1007/s10509-023-04220-3 Bibcode: 2023Ap&SS.368...65A

Abdelkawy, Ali G. A.; Shaltout, Abdelrazek M. K.

We investigate high-resolution observations with the spectropolarimeter (SP) aboard the Hinode satellite of the Solar Optical Telescope (SOT) of a positive polarity sunspot of an active region (AR) (NOAA 12546). We present a case study for the properties of the thermal, magnetic field, and plasma flows as a function of the optical depth from the i…

2023 Astrophysics and Space Science
Hinode 1
Solar Physics in the 2020s: DKIST, Parker Solar Probe, and Solar Orbiter as a Multi-Messenger Constellation
DOI: 10.1017/S1743921323001266 Bibcode: 2023IAUS..372....3M

Müller, D.; Parenti, S.; Andretta, V. +21 more

The National Science Foundation (NSF) Daniel K. Inouye Solar Telescope (DKIST) has started operations at the summit of Haleakalā (Hawai'i). DKIST joins the nominal science phases of the NASA and ESA Parker Solar Probe and Solar Orbiter encounter missions. By combining in-situ measurements of the near-Sun plasma environment and detailed remote obse…

2023 The Era of Multi-Messenger Solar Physics
SolarOrbiter 1
Identifying the population of T-Tauri stars in Taurus: UV–optical synergy
DOI: 10.1007/s12036-023-09972-6 Bibcode: 2023JApA...44...83N

Arun, R.; Mathew, Blesson; Ujjwal, K. +9 more

With the third data release of the Gaia mission, Gaia DR3 with its precise photometry and astrometry, it is now possible to study the behavior of stars at a scale never seen before. In this paper, we developed new criteria to identify T-Tauri stars (TTS) candidates using UV and optical color-magnitude diagrams (CMDs) by combining the GALEX and Gai…

2023 Journal of Astrophysics and Astronomy
Gaia 1
Iron Kα echoes from the circumnuclear disk orbiting Sgr A
DOI: 10.1051/0004-6361/202347184 Bibcode: 2023A&A...679A..44S

Haardt, Francesco; Ponti, Gabriele; Stel, Giovanni

Context. Molecular clouds in the Galactic center (GC) reprocess radiation from past outbursts of nearby high-energy sources, generating a bright Fe Kα fluorescence at 6.4 keV. The closest clouds to the GC are only ≃1.5 pc from Sgr A, forming a torus-like structure known as the circumnuclear disk (CND). The study of fluorescence emissio…

2023 Astronomy and Astrophysics
XMM-Newton 1
Linear and nonlinear kinetic Alfvén waves at Venus
DOI: 10.1051/0004-6361/202245632 Bibcode: 2023A&A...675A.192F

Fichtner, H.; Lazar, M.; Moslem, W. M. +1 more

Space observations show that Venus suffers significant atmospheric erosion caused by the solar wind forcing. Plasma acceleration is found to be one of the main mechanisms contributing to the global atmospheric loss at Venus through its magnetotail. Motivated by these observations, we propose that kinetic Alfvén waves (KAW) may be a possible candid…

2023 Astronomy and Astrophysics
VenusExpress 1
New constraints on decaying dark matter from INTEGRAL/SPI
DOI: 10.1093/mnras/stad304 Bibcode: 2023MNRAS.520.6322F

Santangelo, A.; Ducci, L.; Malyshev, D. +1 more

Based on almost 20 yr of data collected by the high-resolution spectrometer SPI on board the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), we present constraints on a decaying dark matter particle undergoing a decay into two bodies, at least one of which is a photon, manifesting itself via a narrow line-like spectral feature. Our ON-…

2023 Monthly Notices of the Royal Astronomical Society
INTEGRAL 1
Kinetic study of ion acoustic waves in Venusian ionosphere
DOI: 10.1063/5.0145486 Bibcode: 2023PhPl...30g2901K

Lakhina, G. S.; Kamalam, T.; Singh, S. V. +1 more

Kinetic dispersion of the ion acoustic waves has been explored for an unmagnetized five component plasma system comprising of Venusian protons, Venusian oxygen ions, Venusian electrons, solar wind protons, and kappa electrons. The solar wind protons and electrons are assumed to be streaming along the ambient magnetic field. The plasma parameters f…

2023 Physics of Plasmas
Ulysses VenusExpress 1