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19972026
most citedQuantum discord and classical correlation can tighten the uncertainty principle in the presence of quantum memory

165 citations

Showing astro-ph.SRShow all

16 papers · 1 filter

astro-ph.SR2024★ 7 cited

Inter-planetary type-IV solar radio bursts: A comprehensive catalog and statistical results

Atul Mohan, Nat Gopalswamy, Anshu Kumari +2

Decameter hectometric (DH; 1-14 MHz) type-IV radio bursts are produced by flare-accelerated electrons trapped in post-flare loops or the moving magnetic structures associated with…

astro-ph.SR2022★ 4 cited

Supergranular Fractal Dimension and Solar Rotation

Sowmya G. M., Rajani G., U. Paniveni +1

We present findings from an analysis of the fractal dimension of solar supergranulation as a function of latitude, supergranular cell size and solar rotation, employing spectroheli…

astro-ph.SR2022★ 6 cited

Solar supergranular fractal dimension dependence on the Solar cycle phase

G. Rajani, G. M. Sowmya, U. Paniveni +1

We study the complexity of the supergranular network through fractal dimension by using Ca II K digitized data archive obtained from Kodaikanal solar observatory. The data consists…

astro-ph.SR2022★ 3 cited

Magnetic imprints of eruptive and non-eruptive Solar flares as observed by Solar Dynamics Observatory

N. Vasantharaju, P. Vemareddy, B. Ravindra +1

The abrupt and permanent changes of photospheric magnetic field in the localized regions of active regions during solar flares called magnetic imprints (MIs), have been observed fo…

astro-ph.SR2021★ 13 cited

Chemical analysis of two extremely metal-poor stars HE 2148-2039 and HE 2155-2043

Meenakshi Purandardas, Aruna Goswami

We present elemental abundance results for HE 2148-2039 and HE 2155-2043 based on a detailed high-resolution spectroscopic analysis. The high-resolution SUBARU/HDS spectra used for…

astro-ph.SR2020★ 56 cited

Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars

D. Karinkuzhi, S. Van Eck, S. Goriely +5

Among Carbon-Enhanced Metal-Poor (CEMP) stars, some are found to be enriched in s-process elements (CEMP-s), in r-process elements (CEMP-r) or in both s- and r-process elements (CE…