Search Publications

The nearby astrometric-spectroscopic binary star Hip 68682
DOI: 10.3389/fspas.2023.1153912 Bibcode: 2023FrASS..1053912X

Wang, Xiaoli; Fu, Yanning; Chen, Yue +1 more

The nearby astrometric-spectroscopic binary star Hip 68682 has an orbital period of ∼ 9.88 yr. The dynamical state (component masses and kinematic parameters) of this system is redetermined by fitting all the observational data available to us, including the radial velocity data (RVD), the relative position data (RPD), and the Hipparcos Intermedia…

2023 Frontiers in Astronomy and Space Sciences
Hipparcos 1
Ion kinetic effects linked to magnetic field discontinuities in the slow Alfvénic wind observed by Solar Orbiter in the inner heliosphere
DOI: 10.3389/fspas.2023.1250219 Bibcode: 2023FrASS..1050219P

D'Amicis, Raffaella; Perrone, Denise; Perri, Silvia +2 more

Slow solar wind, sharing magnetic and plasma properties typical of fast wind, the so-called slow Alfvénic wind, has been widely observed in the heliosphere. Here, we report an analysis of the turbulent properties of a slow Alfvénic stream observed by Solar Orbiter at 0.64 AU. This solar wind stream is characterized by well distinguishable regions,…

2023 Frontiers in Astronomy and Space Sciences
SolarOrbiter 1
Miras as a distance indicator in the CSST, JWST, and Gaia era
DOI: 10.3389/fspas.2023.1232151 Bibcode: 2023FrASS..1032151S

Sun, Yan; Zhang, Bo; Chen, Wen +5 more

Mira variables are important distance indicators owing to the clear period–luminosity relation at infrared wavelengths. We have compiled a sample of 343 Galactic Miras selected from the American Association of Variable Star Observers database and Gaia Data Release 3. We used V-band observations from the American Association of Variable Star Observ…

2023 Frontiers in Astronomy and Space Sciences
Gaia 1
Exploring the impact of imaging cadence on inferring CME kinematics
DOI: 10.3389/fspas.2023.1232197 Bibcode: 2023FrASS..1032197V

Pant, Vaibhav; Banerjee, Dipankar; Patel, Ritesh +2 more

The kinematics of coronal mass ejections (CMEs) are crucial for understanding their initiation mechanism and predicting their impact on Earth and other planets. With most of the acceleration and deceleration occurring below 4 R⊙, capturing this phase is vital to better understand their initiation mechanism. Furthermore, the kinematics of CMEs in t…

2023 Frontiers in Astronomy and Space Sciences
SOHO 1
The energetic storm particle events of 3 November 2021
DOI: 10.3389/fspas.2023.1209479 Bibcode: 2023FrASS..1009479C

Marcucci, Maria Federica; Consolini, Giuseppe; Chiappetta, Federica +3 more

Observations of energetic particles at interplanetary shocks are important to study acceleration mechanisms and their connection with magnetohydrodynamic turbulence. Energetic storm particle (ESP) events are increases in proton fluxes that occur locally at the passage time of interplanetary shocks. These events are more dangerous when they are sup…

2023 Frontiers in Astronomy and Space Sciences
SolarOrbiter 0
The ability of CSST to determine the orbital solutions of SB1s
DOI: 10.3389/fspas.2023.1152894 Bibcode: 2023FrASS..1052894W

Wang, Xiaoli; Fu, Yanning; Chen, Yue +1 more

The single-lined spectroscopic binaries (SB1s) are composed of two components with large difference in masses and in physical properties. The orbital and physical parameters of a large number of such binary systems are unknown due to lack of necessary observations. Compared with SB2s, SB1s can provide much more stringent constraint to stellar evol…

2023 Frontiers in Astronomy and Space Sciences
Gaia 0
Turbulent dipolarization regions in the Earth's magnetotail: ion fluxes and magnetic field changes
DOI: 10.3389/fspas.2023.1226200 Bibcode: 2023FrASS..1026200K

Kronberg, Elena A.; Blöcker, Aljona; Fedun, Viktor +4 more

In this work, we consider the dynamics of ion fluxes and magnetic field changes in turbulent regions of magnetotail dipolarizations. The data from the Cluster-II mission (magnetic field measurements from fluxgate magnetometers and energetic charged particle observations from RAPID spectrometers) were used for the analysis. We study individual even…

2023 Frontiers in Astronomy and Space Sciences
Cluster 0
RCM modeling of bubble injections into the inner magnetosphere: geosynchronous orbit and the ionospheric responses
DOI: 10.3389/fspas.2023.1189298 Bibcode: 2023FrASS..1089298S

Wang, Chih-Ping; Yang, Jian; Mousavi, Ameneh +3 more

Introduction: Accurate characterization of the plasma sheet source population in the ring current region and its outer boundary at geosynchronous orbit is crucial for understanding the dynamics of the Earth's magnetosphere. The interaction between the ring current and plasma populations from the ionosphere is a focus of extensive research.Methods:…

2023 Frontiers in Astronomy and Space Sciences
Cluster 0
On orbit performance of the solar flare trigger for the Hinode EUV imaging spectrometer
DOI: 10.3389/fspas.2023.1149831 Bibcode: 2023FrASS..1049831B

Warren, Harry P.; Ugarte-Urra, Ignacio; Brooks, David H. +1 more

We assess the on-orbit performance of the flare event trigger for the Hinode EUV Imaging Spectrometer. Our goal is to understand the time-delay between the occurrence of a flare, as defined by a prompt rise in soft X-ray emission, and the initiation of the response observing study. Wide (266″) slit patrol images in the He II 256.32 Å spectral line…

2023 Frontiers in Astronomy and Space Sciences
Hinode 0
The impact of dimensionality reduction of ion counts distributions on preserving moments, with applications to data compression
DOI: 10.3389/fspas.2022.1056508 Bibcode: 2023FrASS...956508D

Thompson, B.; da Silva, D.; Bard, C. +3 more

The field of space physics has a long history of utilizing dimensionality reduction methods to distill data, including but not limited to spherical harmonics, the Fourier Transform, and the wavelet transform. Here, we present a technique for performing dimensionality reduction on ion counts distributions from the MMS/FPI instrument using a data-ad…

2023 Frontiers in Astronomy and Space Sciences
Cluster 0