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Kinematics of a compression front associated with a Coronal Mass Ejection
DOI: 10.1393/ncc/i2019-19035-8 Bibcode: 2019NCimC..42...35F

Bemporad, A.; Frassati, F.; Susino, R. +1 more

On 2014 November 1st a solar prominence eruption associated with a C2.7 class flare and a type II radio burst resulted in a fast partial halo Coronal Mass Ejection (CME). Images acquired in the extreme UV (EUV) by SDO/AIA and PROBA-2/SWAP, and in white light (WL) by SOHO/LASCO show a bright compression front expanding ahead of the CME. The main go…

2019 Nuovo Cimento C Geophysics Space Physics C
PROBA-2 1
A multiwavelength view of a classical T Tauri star CV Cha
DOI: 10.1088/1674-4527/19/1/7 Bibcode: 2019RAA....19....7P

Karmakar, Subhajeet; Sharma, Saurabh; Joshi, Arti +3 more

Using long-term optical, ultraviolet (UV) and X-ray data, we present a study of a classical T Tauri star CV Cha. The V -band light curve obtained from the All Sky Automated Survey (ASAS) shows short as well as long-term variability. The short-term variability could be due to rotational modulation of CV Cha. We derive the rotational period of 3.714…

2019 Research in Astronomy and Astrophysics
XMM-Newton 1
Anomaly Detection Performance Comparison on Anomaly-Detection Based Change Detection on Martian Image Pairs
DOI: 10.5194/isprs-archives-XLII-2-W13-1437-2019 Bibcode: 2019ISPAr4213.1437P

Muller, J. -P.; Sidiropoulos, P.; Putri, A. R. D.

The surface of Mars has been imaged in visible wavelengths for more than 40 years since the first flyby image taken by Mariner 4 in 1964. With higher resolution from orbit from MOC-NA, HRSC, CTX, THEMIS, and HiRISE, changes can now be observed on high-resolution images from different instruments, including spiders (Piqueux et al., 2003) near the s…

2019 ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
MEx 1
Probabilities of Physical Link Between the Components of the Selected Multiple Systems from WDS Catalog
DOI: 10.18524/1810-4215.2019.32.181603 Bibcode: 2019OAP....32..192M

Protsyuk, Yu. I.; Maigurova, N. V.

Astrometric CCD observations of visual components of double and multiple stars were performed using the RI MAO Axial Meridian Circle (AMC) with new Apogee Alta AI-F8300 CCD camera mounted at the telescope in 2018. Observations were carried out automatically in driftscan mode using a standard R filter. Objects for observational program were selecte…

2019 Odessa Astronomical Publications
Hipparcos 1
Investigating the Coronal Mass Ejections associated with DH type-II radio bursts and solar flares during the ascending phase of the solar cycle 24
DOI: 10.1016/j.asr.2018.11.001 Bibcode: 2019AdSpR..63.1824N

Nedal, Mohamed; Mahrous, Ayman; Youssef, M. +1 more

We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric - hectometric (DH) type-II radio bursts (1-16 MHz) and solar flares during the period 2008-2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.

We found th…

2019 Advances in Space Research
SOHO 1
Development and qualification of the Feed-Select Mechanism for the Polarimetric and Helioseismic Imager on-board Solar Orbiter
DOI: 10.1007/s12567-019-00246-y Bibcode: 2019CEAS...11..497S

Hirzberger, Johann; Woch, Joachim; Staub, Jan +5 more

The Solar Orbiter Polarimetric and Helioseismic Imager (SO/PHI) will provide maps of the magnetic vector and of the line-of-sight velocities in the solar photosphere. For reaching its science goals, SO/PHI is equipped with two telescopes: the high resolution channel (HRT) and the full disk channel (FDT). Since both optical channels are fed into a …

2019 CEAS Space Journal
SolarOrbiter 1
η Carinae: Particle acceleration and multimessenger aspects
DOI: 10.1002/asna.201913609 Bibcode: 2019AN....340..273W

Walter, R.; Balbo, M.

η Carinae is composed of two very massive stars orbiting each other in 5.5 years. The primary star features the densest known stellar wind, colliding with that expelled by its companion. The wind collision region dissipates energy and accelerates particles up to relativistic energies, producing nonthermal X‑ray and γ‑ray emission detected by Beppo…

2019 Astronomische Nachrichten
INTEGRAL 1
Signatures of red-shifted foot points in the quiescent coronal loop system
DOI: 10.5194/angeo-37-765-2019 Bibcode: 2019AnGeo..37..765R

Rao, Yamini K.; Srivastava, Abhishek K.; Kayshap, Pradeep +1 more

We observed quiescent coronal loops using multi-wavelength observations from the Atmospheric Imaging Assembly (AIA) aboard the Solar Dynamics Observatory (SDO) on 13 April 2016. The flows at the foot points of such loop systems are studied using spectral data from the Interface Region Imaging Spectrograph (IRIS). The Doppler velocity distributions…

2019 Annales Geophysicae
IRIS 1
Image Estimation in the Presence of Irregular Sampling, Noise, and Pointing Jitter
DOI: 10.1109/TIP.2018.2869725 Bibcode: 2019ITIP...28..713P

Piazzo, Lorenzo

2019 IEEE Transactions on Image Processing
Herschel 1
Subpixel real-time jitter detection algorithm and implementation for polarimetric and helioseismic imager
DOI: 10.1117/1.JATIS.5.3.039003 Bibcode: 2019JATIS...5c9003R

Volkmer, Reiner; Roma, David; Carmona, Manuel +12 more

The polarimetric and helioseismic imager instrument for the Solar Orbiter mission from the European Space Agency requires a high stability while capturing images, specially for the polarimetric ones. For this reason, an image stabilization system has been included in the instrument. It uses global motion estimation techniques to estimate the jitte…

2019 Journal of Astronomical Telescopes, Instruments, and Systems
SolarOrbiter 1