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Theoretical studies of low and high frequency electrostatic solitary waves in the magnetopause associated with asymmetric magnetic reconnection
DOI: 10.1016/j.asr.2022.01.034 Bibcode: 2022AdSpR..69.3008B

Bharuthram, R.; Rufai, O. R.; Maharaj, S. K.

In a comprehensive analysis of Cluster data, Graham et al. (2015) have reported the existence of slow and fast electrostatic solitary waves (ESWs) associated with asymmetric magnetic reconnection arising from the merger of the magnetic fields, and mixing, of the hot tenuous magnetospheric plasma and the cooler dense magnetosheath plasma. Their ana…

2022 Advances in Space Research
Cluster 3
Detection of the third innermost radiation belt on LEO CORONAS-Photon satellite around 2009 solar minimum
DOI: 10.1016/j.asr.2022.06.031 Bibcode: 2022AdSpR..70.1441D

Phillips, Kenneth J. H.; Sylwester, Janusz; Dudnik, Oleksiy V. +2 more

We analyze variations of high energy charged particle populations filling various magnetospheric regions under, inside and outside of the Van Allen inner and outer electron radiation belts in May 2009. The study is based on the experimental data obtained from the STEP-F and the SphinX instruments placed close to each other aboard the low-Earth cir…

2022 Advances in Space Research
SOHO 1
A study of the characteristic properties of SEP events observed by SOHO ERNE during solar cycle 24
DOI: 10.1016/j.asr.2022.01.024 Bibcode: 2022AdSpR..69.2902B

Biji, M. S.; Prince, P. R.

Properties and association of Solar Energetic Particle (SEP) events with their solar sources during the 24th solar cycle were examined. SEPs observed by SOHO ERNE were used. SEP properties include solar release time, peak proton flux and total fluence in different energy channels. Solar release times of SEP events were found out using Velocity Dis…

2022 Advances in Space Research
SOHO 1
Machine learning for effective spacecraft operation: Operating INTEGRAL through dynamic radiation environments
DOI: 10.1016/j.asr.2022.04.004 Bibcode: 2022AdSpR..69.3909S

Finn, Timothy; Southworth, Richard; Donati, Alessandro +8 more

INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory) is an astronomical observatory of the European Space Agency, responsible for many significant scientific discoveries in the last few decades. It orbits Earth since 2002 in a highly elliptical orbit, passing through the Van Allen belts - areas with high-energy ionized particles that can dam…

2022 Advances in Space Research
INTEGRAL 1
The 6.7 keV thermal emission lines in the stellar flare spectra of two chromospherically active Binaries: Algol and GT Mus
DOI: 10.1016/j.asr.2021.09.037 Bibcode: 2022AdSpR..69..499E

Eze, Ambrose Chukwudi; Esaenwi, Sudum; Madu, Fidelis Okey

Chromospherically active binaries' (CABs) are late-type evolved stars with strong chromosphere/coronae and high flare activity levels. Starspot evolution in these CABs and binaries reveals strong stellar and chromospheric activities. In binaries, the tidal interaction via the internal dynamo motion, during rapid rotation of the component stars gen…

2022 Advances in Space Research
Suzaku 1
Episodic and declining fluvial processes in Noctis Fossae, Syria Planum Province, Mars
DOI: 10.1016/j.asr.2022.07.032 Bibcode: 2022AdSpR..70.3205C

Chavan, Anil; Sarkar, Subham; Bhandari, Subhash

The Noachian surfaces across Mars bear abundant evidence for aqueous processes; however, the transformation of the planet from warm and wet to the present-day cold and dry is unclear. A key question is whether these processes continued by the same or different magnitudes in the Hesperian and Amazonian times. The equatorial region of Mars has exten…

2022 Advances in Space Research
MEx 1
Plasma vortices driven by magnetic torsion generated by electric currents in non-magnetic planetary wakes
DOI: 10.1016/j.asr.2022.03.002 Bibcode: 2022AdSpR..69.3902D

Flandes, Alberto; Durand-Manterola, Héctor Javier

In non-collisional magnetised astrophysical plasmas, vortices can form as it is the case of the Venus plasma wake where Lundin et al. (2013) identified a large vortex through the integration of data of many orbits from the Venus Express (VEX) spacecraft. On the one hand, our purpose is to develop a theoretical foundation in order to explain the oc…

2022 Advances in Space Research
VenusExpress 1
A search for thermal X-ray emission from the composite supernova remnant G21.5-0.9 with Suzaku
DOI: 10.1016/j.asr.2021.11.016 Bibcode: 2022AdSpR..69..531R

Raycheva, Nergis C.; Sezer, Aytap

G21.5-0.9 is a young plerionic composite supernova remnant (SNR) hosting a bright pulsar wind nebula. The previous X-ray studies reported that the X-ray spectrum of the entire SNR can be fitted with a non-thermal spectral model, while the recent Chandra studies have pointed out that its X-ray spectrum also shows weak thermal emission. With this mo…

2022 Advances in Space Research
Suzaku 0
Galactic component mapping of galaxy UGC 2885 by machine learning classification
DOI: 10.1016/j.asr.2022.04.032 Bibcode: 2022AdSpR..70..229K

Holwerda, Benne W.; Barmby, Pauline; Kwik, Robin J. +1 more

Automating classification of galaxy components is important for understanding the formation and evolution of galaxies. Traditionally, only the larger galaxy structures such as the spiral arms, bulge, and disc are classified. Here we use machine learning (ML) pixel-by-pixel classification to automatically classify all galaxy components within digit…

2022 Advances in Space Research
Gaia eHST 0
X-ray investigation of the X-ray source 1RXS J121902.7-630910 with Suzaku
DOI: 10.1016/j.asr.2022.07.076 Bibcode: 2022AdSpR..70.3263D

Bakis, Hicran; Raycheva, Nergis C.; Sezer, Aytap +1 more

We present a study of the unidentified X-ray source 1RXS J121902.7-630910 based on Suzaku X-ray Imaging Spectrometer observation. We aim at clarifying the nature of the emission from 1RXS J121902.7-630910. We found that the spectrum is well represented by a thermal plasma model with an electron temperature of kTe ∼ 3.7 keV, the upper li…

2022 Advances in Space Research
Suzaku 0