Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Susanta Kumar Bisoi"'
We have examined polar magnetic fields for the last three solar cycles, {$\it{viz.}$}, cycles 21, 22 and 23 using NSO Kitt Peak synoptic magnetograms. In addition, we have used SoHO/MDI magnetograms to derive the polar fields during cycle 23. Both Ki
Externí odkaz:
http://arxiv.org/abs/1009.4299
Publikováno v:
Advances in Space Research. 68:2257-2271
Modern-Era Retrospective Analysis for Research and Applications, Version-2 (MERRA-2) total column ozone (TCO) data from 1980 to 2018 and ground based TCO data were used to investigate its responses to periodic variations concerning stratospheric dyna
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::29e9197e0a1590858883a99acf9d6258
https://doi.org/10.1016/j.asr.2021.06.021
https://doi.org/10.1016/j.asr.2021.06.021
Autor:
Divya Oberoi, Susanta Kumar Bisoi, K. Sasikumar Raja, Devojyoti Kansabanik, Atul Mohan, Surajit Mondal, Rohit Sharma
The Square Kilometre Array Observatory (SKAO) is perhaps the most ambitious radio telescope envisaged yet. It will enable unprecedented studies of the Sun, the corona and the heliosphere and help to answer many of the outstanding questions in these a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::72a9f5bbe3a6f1b1eefe48568048ea13
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:6363-6383
The present study examines the response of the terrestrial magnetosphere to the long-term steady declining trends observed in solar magnetic fields and solar wind micro-turbulence levels since mid-1990's that has been continuing beyond the mini-solar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2920ed64effe5cf1d3c72c9ac6e9f15
https://doi.org/10.1029/2019ja026616
https://doi.org/10.1029/2019ja026616
Autor:
Chris J. Nelson, M. B. Korsós, Manolis K. Georgoulis, N. Gyenge, Stefaan Poedts, Susanta Kumar Bisoi, Jiajia Liu, Yihua Yan, Sijie Yu, Robert Erdélyi
In this article, we present the application of the weighted horizontal gradient of magnetic field (WG_M) flare prediction method to 3-dimensional (3D) extrapolated magnetic configurations of 13 flaring solar active regions (ARs). The main aim is to i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::305601bdf659a32eea4cb6719facb841
http://arxiv.org/abs/2005.12180
http://arxiv.org/abs/2005.12180
Publikováno v:
Proceedings of the International Astronomical Union. 13:121-124
We re-examined solar polar magnetic fields, using ground based synoptic photospheric magnetograms, during solar cycle 24. IThe signed polar magnetic fields showed an unusual hemispheric asymmetry in the polar field reversal process with a single unam
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9f5f8bce848f86995159392988a8316e
https://doi.org/10.1017/s1743921318001710
https://doi.org/10.1017/s1743921318001710
Publikováno v:
Advances in Space Research. 60:1708-1715
We connect the time sequence of changes in the IMF-Bz to the development of spread-F at an equatorial station Kwajalein on three different nights in November 2004, one during a geomagnetic quiet period and other two during geomagnetic disturbed perio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::407e8f9ab00bd413440e39eda01d0e95
https://doi.org/10.1016/j.asr.2017.06.020
https://doi.org/10.1016/j.asr.2017.06.020
The very low frequency (VLF) regime below 30 MHz in the electromagnetic spectrum has presently drawing global attentions in radio astronomical research due to its potentially significant science outcomes exploring many unknown extragalactic sources,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a8b1cdba736964ea4884c2c70b6d13f
Autor:
P. Janardhan, Susanta Kumar Bisoi
The magnetic flux cancellation on the Sun plays a crucial role in determining the manner in which the net magnetic flux changes in every solar cycle, affecting the large scale evolution of the coronal magnetic fields and heliospheric environment. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b16a04575600f0fc2d145bb09270691b
http://arxiv.org/abs/1911.03865
http://arxiv.org/abs/1911.03865
Autor:
Milan Maksimovic, Prasad Subramanian, K. Sasikumar Raja, Ken'ichi Fujiki, P. Janardhan, Susanta Kumar Bisoi, Madhusudan Ingale
Publikováno v:
Solar Physics
Solar Physics, Springer Verlag, 2019, 294 (9), ⟨10.1007/s11207-019-1514-7⟩
Solar Physics, Springer Verlag, 2019, 294 (9), ⟨10.1007/s11207-019-1514-7⟩
The extended minimum of Solar Cycle 23, the extremely quiet solar-wind conditions prevailing, and the mini-maximum of Solar Cycle 24 drew global attention and many authors have since attempted to predict the amplitude of the upcoming Solar Cycle 25,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1841684df07e1a4ec7a65ec1f6b84c9
https://hal.archives-ouvertes.fr/hal-03131234
https://hal.archives-ouvertes.fr/hal-03131234