Search Publications

Interplanetary type II radio bursts and their association with CMEs and flares
DOI: 10.1007/s10509-018-3345-7 Bibcode: 2018Ap&SS.363..126S

Shanmugaraju, A.; Suresh, K.; Umapathy, S. +2 more

We study the characteristics of the CMEs and their association with the end-frequency of interplanetary (IP)-type-II bursts by analyzing a set of 138 events (IP-type-II bursts–flares–CMEs) observed during the period 1997–2012. The present analysis consider only the type II bursts having starting frequency

2018 Astrophysics and Space Science
SOHO 5
X-ray stars observed in LAMOST spectral survey
DOI: 10.1007/s10509-018-3328-8 Bibcode: 2018Ap&SS.363..104L

Shi, Jianrong; Han, Xianming L.; Lu, Hong-peng +1 more

X-ray stars have been studied since the beginning of X-ray astronomy. Investigating and studying the chromospheric activity from X-ray stellar optical spectra is highly significant in providing insights into stellar magnetic activity. The big data of LAMOST survey provides an opportunity for researching stellar optical spectroscopic properties of …

2018 Astrophysics and Space Science
XMM-Newton 3
History of globulettes in the Milky Way
DOI: 10.1007/s10509-017-3233-6 Bibcode: 2018Ap&SS.363...28G

Grenman, Tiia; Elfgren, Erik; Weber, Hans

Globulettes are small (radii <10 kAU) dark dust clouds, seen against the background of bright nebulae. A majority of the objects have planetary mass. These objects may be a source of brown dwarfs and free floating planetary mass objects in the gala…

2018 Astrophysics and Space Science
eHST 2
GALEX far-ultraviolet observations of metal-poor subdwarfs
DOI: 10.1007/s10509-018-3455-2 Bibcode: 2018Ap&SS.363..235S

Smith, Graeme H.

Far-ultraviolet photometry derived from the GALEX satellite observatory has been compiled for a sample of metal-poor subdwarfs with [Fe/

2018 Astrophysics and Space Science
Gaia 2
The astrometric signal of microlensing events caused by free floating planets
DOI: 10.1007/s10509-018-3374-2 Bibcode: 2018Ap&SS.363..153H

Nucita, Achille A.; De Paolis, Francesco; Hamolli, Lindita +1 more

Astrometric observations of microlensing events can be used to obtain important information about lenses. During these events, the shift of the position of the multiple image centroid with respect to the source star location can be measured. This effect, which is expected to occur on scales from micro-arcseconds to milli-arcseconds, depends on the…

2018 Astrophysics and Space Science
Gaia 1
A review of low-energy transfers
DOI: 10.1007/s10509-018-3461-4 Bibcode: 2018Ap&SS.363..253D

Dutt, Pooja

Low-energy transfers (LET) for lunar and interplanetary missions has received immense attention of the scientific community during the last few decades as its importance was understood by the success of JAXA's Hiten, ESA's SMART-1, NASA's GRAIL and ARTHEMIS missions, and several proposals, like the BepiColombo, Multi-Moon Orbiter and Europa Orbite…

2018 Astrophysics and Space Science
SMART-1 0
Nonlinear model to study filamentation instability of circularly polarized dispersive Alfvén waves in solar wind plasmas
DOI: 10.1007/s10509-018-3382-2 Bibcode: 2018Ap&SS.363..164S

Sharma, R. P.; Sharma, Swati; Mishra, M. K.

This paper examines the small-scale solar wind turbulence driven in view of the Alfvén waves subjected to ponderomotive nonlinearity. Filamentation instability is known to take place for the case of dispersive Alfvén wave (DAW) propagating parallel to the ambient magnetic field. The ponderomotive force associated with DAW is responsible for wave l…

2018 Astrophysics and Space Science
Cluster 0
A two-fluid modeling of kinetic Alfvén wave turbulence
DOI: 10.1007/s10509-018-3427-6 Bibcode: 2018Ap&SS.363..204K

Moon, Y. -J.; Sharma, R. P.; Dwivedi, Navin Kumar +1 more

We present an analytical model to explore the magnetic field turbulent spectrum by coupled high-frequency kinetic Alfvén wave (KAW) and slow mode of Alfvén wave (AW). The spectrum is computed as a realization of energy cascades from larger to smaller scales for a specific case of solar wind plasma at 1 AU. A two-fluid technique is implemented for …

2018 Astrophysics and Space Science
Cluster 0