Search Publications

Solar Ultraviolet Bursts in the Joint Footpoints of Multiple Transition Region Loops
DOI: 10.3390/sym13081390 Bibcode: 2021Symm...13.1390H

Fu, Hui; Xia, Lidong; Huang, Zhenghua +4 more

2021 Symmetry
IRIS 2
Cassini-Plasma Interaction Simulations Revealing the Cassini Ion Wake Characteristics: Implications for In-Situ Data Analyses and Ion Temperature Estimates
DOI: 10.1029/2020JA029026 Bibcode: 2021JGRA..12629026H

Wilson, R. J.; Morooka, M. W.; Hadid, L. Z. +7 more

We have used Spacecraft Plasma Interaction Software (SPIS) simulations to study the characteristics (i.e., dimensions, ion depletion, and evolution with the changing spacecraft attitude) of the Cassini ion wake. We focus on two regions, the plasma disk at 4.5-4.7 RS, where the most prominent wake structure will be formed, and at 7.6 R

2021 Journal of Geophysical Research (Space Physics)
Cassini 2
Minimally Modified Gravity Fitting Planck Data Better Than ΛCDM
DOI: 10.1134/S1063772921100279 Bibcode: 2021ARep...65.1021P

Pookkillath, M. C.

Here we present cosmology of a class of Minimally Modified Gravity theory dubbed as $f(H)$ theory. After introducing a concrete model for the free function, we find that this cosmological model fits Planck data better than $Λ $CDM.

2021 Astronomy Reports
eHST 2
Fundamental properties of stars from Kepler and Gaia data: parallax offset and revised scaling relations
DOI: 10.1093/mnras/stab996 Bibcode: 2021MNRAS.504.2273Y

Örtel, S.; Yıldız, M.

Data from the space missions Gaia, Kepler, CoRoT and TESS, make it possible to compare parallax and asteroseismic distances. From the ratio of two densities ρscaπ, we obtain an empirical relation fΔν between the asteroseismic large frequency separation and mean density, which is important for more accurate stella…

2021 Monthly Notices of the Royal Astronomical Society
CoRoT Gaia 2
Nonsequential neural network for simultaneous, consistent classification, and photometric redshifts of OTELO galaxies
DOI: 10.1051/0004-6361/202141360 Bibcode: 2021A&A...655A..56D

Cepa, J.; Pérez García, A. M.; Alfaro, E. J. +17 more

Context. Computational techniques are essential for mining large databases produced in modern surveys with value-added products.
Aims: This paper presents a machine learning procedure to carry out a galaxy morphological classification and photometric redshift estimates simultaneously. Currently, only a spectral energy distribution (SED) fitti…

2021 Astronomy and Astrophysics
eHST 2
Comprehensive list of semi-detached double-lined eclipsing binaries with Gaia DR2 data
Bibcode: 2021A&AT...32..111M

Malkov, O. Yu.

Semi-detached eclipsing systems play an important role in our understanding of stellar properties. In the present study, we have cross-matched a previously compiled comprehensive list of SD double-lined eclipsing binaries, containing 119 systems, with Gaia DR2, and analyze the result. A special analysis is conducted for systems with controversial …

2021 Astronomical and Astrophysical Transactions
Gaia 2
Selected phenomena that affect the structure of the cometary landscape
DOI: 10.1007/s12036-021-09772-w Bibcode: 2021JApA...42...91W

Wesołowski, M.

The paper discusses four processes that may be responsible for shaping the relief of the comet landscape. The considerations take into account the following phenomena: intense sublimation of cometary ice, emission of dust from the surface comet and through jets, migration of dust on the cometary surface, and destruction of fragment the nucleus sur…

2021 Journal of Astrophysics and Astronomy
Rosetta 2
Absolute parameters of the W UMa binaries CSS J223614+311343, V523 Aur and V783 And
DOI: 10.1016/j.newast.2020.101401 Bibcode: 2021NewA...8401401K

Michel, Raul; Kjurkchieva, Diana; Popov, Velimir A. +3 more

Photometric BVRc observations of the stars CSS J223614+311343, V523 Aur and V783 And were carried out and their absolute parameters (masses, radii and luminosities) were determined based on light curve modeling and Gaia distances. The main results are: (i) The components of CSS J223614+311343 and V783 And are of K spectral type while th…

2021 New Astronomy
Gaia 2
Evidence for local particle acceleration in the first recurrent galactic cosmic ray depression observed by Solar Orbiter. The ion event on 19 June 2020
DOI: 10.1051/0004-6361/202140966 Bibcode: 2021A&A...656L..10A

Fedorov, A.; Kulkarni, S. R.; Lario, D. +61 more

Context. In mid-June 2020, the Solar Orbiter (SolO) mission reached its first perihelion at 0.51 au and started its cruise phase, with most of the in situ instruments operating continuously.
Aims: We present the in situ particle measurements of the first proton event observed after the first perihelion obtained by the Energetic Particle Detec…

2021 Astronomy and Astrophysics
SolarOrbiter 2
Using Observations of Solar Vector Magnetic Field from Dual View Points to Remove the 180 Ambiguity
DOI: 10.1016/j.chinastron.2021.11.004 Bibcode: 2021ChA&A..45..494Z

Liu, Rui; Zhou, Ru-yun; Wang, Yu-ming +3 more

With Solar Orbiter (SO) being put into successful operational observation, solar magnetic observation has entered the era of remote sensing from dual view points. In this paper, we carried out a simulation of correcting the 180 ambiguity of transverse magnetic field with magnetograms from dual view points using an analytical formula as…

2021 Chinese Astronomy and Astrophysics
SolarOrbiter 2