Search Publications

Agile Development of Science Operations: The Solar Orbiter Experience
Bibcode: 2020ASPC..522..335G

García-Reinaldos, María; Marcos, José; Sánchez, Luis

Cost and schedule are very rigid external constraints for the development of a Science Operations Centre (SOC), as typically the SOC is not considered a critical item for launch and cost and schedule depend on the overall project. Therefore, the greatest degree of flexibility in SOC development is the scope: while we aim to satisfy all the high le…

2020 Astronomical Data Analysis Software and Systems XXVII
SolarOrbiter 0
On the unexpected geomagnetic storm on june 8, 2019, and the heliospheric current sheet effect
DOI: 10.1016/j.pss.2020.105084 Bibcode: 2020P&SS..19305084D

Augusto, C. R. A.; Navia, C. E.; de Oliveira, M. N. +1 more

A period of minimum magnetic solar activity (such as June 2019) favors the observation of rare solar transient events, which would otherwise be lost in the magnetic vortex during a period of maximum solar activity. In this paper, we show that the most plausible explanation for the origin of an unexpected geomagnetic storm on June 8, 2019, is a sma…

2020 Planetary and Space Science
SOHO 0
Numerical simulation of ion reflection by lunar crustal magnetic fields
DOI: 10.5194/egusphere-egu2020-18137 Bibcode: 2020EGUGA..2218137D

Divin, Andrey; Deca, Jan; Lue, Charles +1 more

We investigate the dynamics of solar wind - Moon interaction by means of large-scale Particle-in-Cell (PIC) simulations in this study. Implicit moment PIC method and open boundaries are implemented in the code (iPIC3D) allowing to use large-scale domains in three dimensions. Even though the Moon has no global dipolar magnetic field, satellite magn…

2020 EGU General Assembly Conference Abstracts
Chandrayaan-1 0
Steerable High-Gain Dual-Reflector Antenna at X-Band for Solar Orbiter
DOI: 10.1109/TAP.2020.2980333 Bibcode: 2020ITAP...68.5784M

Martinez, Victor Sanchez; Jimenez, Fernando Martin; Baladron, Inaki Pinto +7 more

2020 IEEE Transactions on Antennas and Propagation
SolarOrbiter 0
Search for the Relationship between the Velocity of a Coronal Mass Ejection and the Decay Rate of the Magnetic Field in the Region of Mass Emission Generation
DOI: 10.1134/S0016793220080277 Bibcode: 2020Ge&Ae..60.1114Z

Fainshtein, V. G.; Rudenko, G. V.; Zagainova, Yu. S.

In this paper, we search for the relationship between the Vlin linear projection velocity and the Vss velocity in the 3D space of coronal mass ejections (CMEs) recorded by LASCO coronagraphs with an "n" decay rate of the transverse component of the Bt magnetic field above the polarity inversion line (PIL) of the ph…

2020 Geomagnetism and Aeronomy
SOHO 0
Some notes concerning open clusters and GAIA DR2 data
DOI: 10.1002/asna.202013784 Bibcode: 2020AN....341.1031L

Loktin, Alexander Vasilievich; Popova, Maria Erikovna

Issues in applying the Gaia DR2 data to determine the main parameters of open star clusters and the use of a formal, two color diagram for the initial selection of cluster members are discussed. The possibility of using the catalog estimates of interstellar absorption is considered. It has been shown that these estimates correlate with the E(B - V…

2020 Astronomische Nachrichten
Gaia 0
The Emission-Line Dusty Object IRAS 07080+0605, A Less-Evolved Example of the Red Rectangle
DOI: 10.18524/1810-4215.2020.33.216403 Bibcode: 2020OAP....33..141K

Miroshnichenko, A. S.; Manset, N.; Zharikov, S. V. +11 more

The all-sky survey conducted by the InfraRed Astronomical Satellite (IRAS) in the 1980's discovered many objects with infrared excesses whose nature has not been explored until recently. IRAS07080+0605 is one of those identified in the visual spectral range with an early-type star, which shows the B[e] phenomenon. The object is puzzling, because i…

2020 Odessa Astronomical Publications
Gaia 0
High-resolution optical spectroscopy of Nova V392 Per
DOI: 10.48550/arXiv.1906.06055 Bibcode: 2020BlgAJ..32...63S

Stoyanov, K. A.; Georgiev, S.; Stateva, I. +1 more

Here we analyze high-resolution spectra of the Nova V392 Per obtained during the 2018 outburst. The Hα and Hβ emission lines show a triple-peak structure with radial velocities of about -2000 km/s, -250 km/s and 1900 km/s respectively. The near infrared spectrum is dominated by the narrow and single-peaked Paschen lines of hydrogen and the O I λ84…

2020 Bulgarian Astronomical Journal
Gaia 0
Eye of a skull reveals details of cometary materials
DOI: 10.1038/d41586-020-02941-x Bibcode: 2020Natur.586..675A

Asphaug, Erik

The Philae spacecraft was meant to anchor itself to the surface of the comet 67P/Churyumov-Gerasimenko, but instead bounced into a hidden grotto. The telltale markings of its passage reveal details of the comet's fragile boulders.

2020 Nature
Rosetta 0
Some kinematics of halo coronal mass ejections
DOI: 10.1515/astro-2020-0010 Bibcode: 2020OAst...29...81V

Chandra, Ramesh; Verma, Virendra Kumar; Mittal, Nishant

We present an investigation of halo coronal mass ejections (HCMEs) kinematics and other facts about the HCMEs. The study of HCMEs is very important because HCMEs are regarded as the main causes of heliospheric and geomagnetic disturbances. In this study, we have investigated 313 HCMEs observed during 1996-2012 by LASCO, coronal holes, and solar fl…

2020 Open Astronomy
SOHO 0