Search Publications

Development of a 3-D Plasmapause Model With a Back-Propagation Neural Network
DOI: 10.1029/2019SW002360 Bibcode: 2019SpWea..17.1689Z

He, Fei; Lei, Jiuhou; Zhang, Xiao-Xin +2 more

Several empirical models have been previously developed to study the characteristics of the global plasmasphere. A three-dimensional solar wind-driven global dynamic plasmapause model was developed in this study using a back-propagation neural network based on multisatellite measurements. Our database contains 37,859 plasmapause crossing events fr…

2019 Space Weather
Cluster 3
Link between trees of fragmenting granules and deep downflows in MHD simulation
DOI: 10.1051/0004-6361/201834283 Bibcode: 2019A&A...622A.112R

Malherbe, J. M.; Roudier, T.; Frank, Z. +1 more

Context. Trees of fragmenting granules (TFG) and associated flows are suspected to play a major role in the formation of the network in the quiet Sun. We investigate the counterparts, in terms of dynamics, of surface structures detectable by high resolution observations in deeper layers up to 15 Mm, which are only available from numerical simulati…

2019 Astronomy and Astrophysics
Hinode SOHO 3
Equatorial Magnetosonic Waves Observed by Cluster Satellites: The Chirikov Resonance Overlap Criterion
DOI: 10.1029/2019JA026680 Bibcode: 2019JGRA..124.2864A

Aryan, Homayon; Walker, Simon N.; Balikhin, Michael A. +1 more

Magnetosonic waves play an important role on the overall dynamics of relativistic radiation belt electrons. Numerical codes modeling the evolution of the radiation belts often account for wave-particle interaction with magnetosonic waves. The diffusion coefficients incorporated in these codes are generally estimated based on the results of statist…

2019 Journal of Geophysical Research (Space Physics)
Cluster 3
Analysis of Field-Aligned Currents in the High-Altitude Nightside Auroral Region: Cluster Observation
DOI: 10.5140/JASS.2019.36.1.1 Bibcode: 2019JASS...36....1S

Shin, Youra; Lee, Ensang; Lee, Jae-Jin

In this paper we present analysis of current density when the Cluster spacecraft pass the nightside auroral region at about 4-5 RE from the center of Earth. The analysis is made when the inter-spacecraft separation is within 200 km, which allows all four spacecraft to be situated inside the same current sheet. On 22 February 2002, two field-aligne…

2019 Journal of Astronomy and Space Sciences
Cluster 3
Surveying the Bright Stars by Optical Interferometry. II. A Volume-limited Multiplicity Survey of Main-sequence F Stars
DOI: 10.3847/1538-4365/ab32e1 Bibcode: 2019ApJS..243...32H

Hutter, D. J.; Tycner, C.; Zavala, R. T. +3 more

We present the results of a multiplicity survey for a volume-limited sample of 29 main-sequence F0-G0 stars within 17 pc conducted with the Navy Precision Optical Interferometer (NPOI). Four companions were detected in previously known binary systems. The results for these stars show good agreement with previously published orbits. For one of thes…

2019 The Astrophysical Journal Supplement Series
Gaia 3
A study on radio-loud interacting/non-interacting CMEs-associated SEPs and solar flares
DOI: 10.1016/j.asr.2019.01.019 Bibcode: 2019AdSpR..63.3390P

Feng, Li; Pappa Kalaivani, P.; Prakash, O. +4 more

We have established a data set of 58 major hybrid SEP events associated with meter-to-decahectometer wavelength (m-to-DH) type II bursts, solar flares, and radio-load CMEs during the period of 1997-2014. The main focus of our study is to address the following two questions: Does the interaction of CMEs play a role in the enhancement of SEP intensi…

2019 Advances in Space Research
SOHO 3
V1082-Sgr: A magnetic cataclysmic variable with a lobe-filling companion star
DOI: 10.1093/mnras/stz2388 Bibcode: 2019MNRAS.489.3031X

Xu, Xiaojie; Shao, Yong; Li, Xiang-Dong

V1082 Sgr is a cataclysmic variable with accretion luminosity above 1034 erg s-1, indicating a mass-transfer rate above 10^{-9} M_{⊙ } yr-1. However, its K-type companion was suggested to be underfilling its Roche lobe (RL), making the high mass-transfer rate a mystery. In this work we propose a possible model to e…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 3
Global spectrophotometric properties of Asteroid (21) Lutetia using Rosetta-OSIRIS images
DOI: 10.1016/j.icarus.2019.02.005 Bibcode: 2019Icar..326....1M

Masoumzadeh, N.; Boehnhardt, H.

We present a spectrophotometric analysis of the surface areas of asteroid (21) Lutetia that were imaged during the Rosetta flyby on July 2010 by the OSIRIS camera in the wavelength range 269 to 989 nm. A spectral slope change with respect to phase angle is found and interpreted as being due to areal diversity of Lutetia's surface. We applied Minna…

2019 Icarus
Rosetta 3
South-North Hemispheric Asymmetry of the FAE Distribution Around the Cusp Region: Cluster Observation
DOI: 10.1029/2019JA026582 Bibcode: 2019JGRA..124.5342S

Dunlop, Malcolm; Carr, Chris; Torkar, Klaus +5 more

Cluster data from late July to early October were used to study the distribution of field-aligned electron (FAE) events around the two cusps. An FAE event was defined as electron parallel flux >3 × 108 (cm2 s)-1. The total number of FAE events around the two cusps was basically identical, but downward FAE events…

2019 Journal of Geophysical Research (Space Physics)
Cluster 3
Integrated Spectra of Milky Way Globular Clusters
DOI: 10.3847/1538-4357/ab3eb6 Bibcode: 2019ApJ...885...28M

Trevisan, M.; Barbuy, B.; Moura, T. C. +1 more

Integrated spectra of Milky Way globular clusters (GCs) are reproduced by computing synthetic spectra taking into account individual element abundances. Five clusters were selected from their location in the Galactic bulge, for which integrated spectra were available in the WiFeS Atlas of Galactic Globular Cluster Spectra project. Our aim is to fu…

2019 The Astrophysical Journal
eHST 3