Search Publications

HCS background magnetic field study HYTARO+
DOI: 10.1051/0004-6361/202245517 Bibcode: 2023A&A...677A.135A

Hidalgo, M. A.; Blanco, J. J.; Arrazola, D.

Context. HYTARO+ is an analytical model developed to evaluate the influence of the solar magnetic dipole in the topology of the local structure of the heliospheric current sheet (HCS).
Aims: Statistical methods such as MVA, which are typically used in the study of the HCS come with two limitations. On one hand, they do not provide any informa…

2023 Astronomy and Astrophysics
Ulysses 0
Temporal Behaviors of Magnetic Helicity Injections by Self and Mutual Sunspot Rotations
DOI: 10.3847/1538-4357/aca800 Bibcode: 2023ApJ...943...96H

Shimizu, Toshifumi; Hasegawa, Takahiro

Magnetic helicity is a physical parameter used to quantify the complexity of magnetic fields, providing an indication of the energy state in the coronal magnetic structure. We investigate the temporal evolution of magnetic helicity and its relationship to the occurrence of a variety of flares in the solar active region NOAA 12297, which was well o…

2023 The Astrophysical Journal
SOHO 0
Statistical analysis of the relationship between Power spectral density of magnetic turbulence and ion velocity in magnetotail bursty bulk Flows
DOI: 10.1016/j.asr.2023.03.024 Bibcode: 2023AdSpR..72..590W

Du, A. M.; Wu, Q.; Wang, G. Q.

Based on the observation of the THEMIS satellites, we utilize the superposed epoch method to statistically analyze how the p (Power Spectral Density) of compressional and transverse components of the magnetic field is affected by the ion inflow velocity V which is the peak velocity of BBFs (Bursty Bulk Flows). The analysis demonstrated…

2023 Advances in Space Research
Cluster 0
A holistic study of the systems V0487 Lac, V0566 Hya, and V0666 Lac
DOI: 10.1515/astro-2022-0228 Bibcode: 2023OAst...32..228A

Alenazi, Moqbil S.; Elkhateeb, Magdy M.

A comprehensive photometric study and evolutionary state for the systems V0487 Lac, V0566 Hya, and V0666 Lac were carried out by means of their first photometric observations. New times of minima were estimated from the observed light curves, and first (O-C) curves were established for all systems. The radiative treatment was carried out using a W…

2023 Open Astronomy
Gaia 0
Impact of Mars GDS 2018 on the Chemistry of Water, Nitrogenated and Deuterated Cluster Ions: NOMAD Observations
DOI: 10.1029/2023JE007993 Bibcode: 2023JGRE..12807993S

Korablev, O.; Haider, S. A.; Shah, Siddhi Y.

The ExoMars Trace Gas Orbiter instruments, Nadir and Occultation for Mars Discovery and Atmospheric Chemistry Suite have provided vertical profiles of H2O and HDO mixing ratios in the presence and absence of Global Dust Storm 2018. These observations are carried out in the lower atmosphere at SZA ∼ 71° of northern mid latitude (∼55°N, 1…

2023 Journal of Geophysical Research (Planets)
ExoMars-16 0
Model-driven engineering for low-code ground support equipment configuration and automatic test procedures definition
DOI: 10.1016/j.actaastro.2023.06.027 Bibcode: 2023AcAau.211..574M

Carrasco, Alberto; Martínez, Agustín; Sánchez, Sebastián +4 more

Space domain systems must go through different types of ground testing. For system-level black-box functional testing, ground support equipment is built ad hoc, customized for each different mission. Building any of this specific equipment involves considerable engineering effort that can be diluted using techniques that allow reusing configuratio…

2023 Acta Astronautica
SolarOrbiter 0
Main Results from the ISSI International Team "Characterization of 67P Cometary Activity"
DOI: 10.3390/universe9100446 Bibcode: 2023Univ....9..446L

Longobardo, Andrea; Della Corte, Vincenzo; Fulle, Marco +8 more

The ESA/Rosetta mission accompanied the Jupiter Family Comet 67P/Churyumov-Gerasimenko and provided a huge amount of data which are providing important results about cometary activity mechanisms. We summarize the results obtained within the ISSI International Team Characterization of 67P cometary activity, which studied dust and gas ejection in di…

2023 Universe
Rosetta 0
Thin jets underlie the solar wind
DOI: 10.1126/science.adj8002 Bibcode: 2023Sci...381..833U

Ugarte-Urra, Ignacio; Wang, Yi-Ming

The Solar Orbiter spacecraft was launched in 2020 by the European Space Agency to study how solar activity drives changes in the inner part of the heliosphere, the region that extends from the Sun to the surrounding interstellar medium. The Solar Orbiter is fitted with a suite of in situ and remote-sensing instruments that allow measurement of the…

2023 Science
SolarOrbiter 0
Performance of the polarization leakage correction in the PILOT data
DOI: 10.1007/s10686-022-09882-5 Bibcode: 2023ExA....56..197B

Griffin, Matt; Savini, Giorgio; Hughes, Annie +34 more

The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment that aims to measure the polarized emission of thermal dust at a wavelength of 240µm (1.2 THz). The PILOT experiment flew from Timmins, Ontario, Canada in 2015 and 2019 and from Alice Springs, Australia in April 2017. T…

2023 Experimental Astronomy
Herschel 0
IRAS 00450+7401 and the Mid-infrared Fade/Burst Cycle of R Coronae Borealis-type Stars
DOI: 10.3847/1538-3881/acda93 Bibcode: 2023AJ....166...40B

Melis, Carl; Wright, E. L.; Della Costa, John +3 more

We present optical and infrared imaging and spectroscopy of the R Coronae Borealis-type (R Cor Bor) star IRAS 00450+7401. Optical spectra further confirm its classification as a cool R Cor Bor system, having a hydrogen-deficient carbon star spectral subclass of HdC5 or later. Mid-infrared spectroscopy reveals the typical ~8 µm "hump" seen in…

2023 The Astronomical Journal
AKARI Gaia 0