Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Bendict Lawrance"'
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 1, p 14 (2024)
For the first time, we generate solar coronal parameters (density, magnetic field, radial velocity, and temperature) on a near-real-time basis by deep learning. For this, we apply the Pix2PixCC deep-learning model to three-dimensional (3D) distributi
Externí odkaz:
https://doaj.org/article/ea1c8d8da6794d71b8d85d8d11a7f65c
Publikováno v:
In Advances in Space Research 1 January 2015 55(1):407-415
Publikováno v:
Solar Physics. 298
Autor:
P. Vijayalakshmi, A. Shanmugaraju, M. Bendict Lawrance, Y.-J. Moon, Daye Lim, C. K. Balaji, P. Hemalatha
Publikováno v:
Astrophysics and Space Science. 367
Autor:
Vijayalakshmi, P., Shanmugaraju, A., Bendict Lawrance, M., Moon, Y.-J., Na, Hyeonock, Ebenezer, E.
Publikováno v:
Solar Physics; Feb2023, Vol. 298 Issue 2, p1-19, 19p
Autor:
Bendict Lawrance, Harim Lee, Eunsu Park, Il-Hyun Cho, Yong-Jae Moon, Jin-Yi Lee, Shanmugaraju A, Sumiaya Rahman
Publikováno v:
The Astrophysical Journal. 937:111
Low coronal white-light observations are very important to understand low coronal features of the Sun, but they are rarely made. We generate Mauna Loa Solar Observatory (MLSO) K-coronagraph like white-light images from the Solar Dynamics Observatory/
Publikováno v:
Solar Physics. 295
Active region and flare ribbon properties associated with X-class flares and CMEs of solar cycle 24.
Autor:
Vijayalakshmi, P., Shanmugaraju, A., Bendict Lawrance, M., Moon, Y.-J., Lim, Daye, Balaji, C. K., Hemalatha, P.
Publikováno v:
Astrophysics & Space Science; Mar2022, Vol. 367 Issue 3, p1-17, 17p
Publikováno v:
Indian Journal of Physics. 91:711-720
We report our results on comparison of two halo Coronal Mass Ejections (CME) associated with X-class flares of similar strength (X1.4) but quite different in CME speed and acceleration, similar geo-effectiveness but quite different in Solar Energetic
Publikováno v:
Solar Physics. 291:1547-1560
The characteristics and geoeffectiveness of interplanetary coronal mass ejections (ICMEs) are derived and their relationships are investigated. The results are compared for a set of events in the rising phase of Solar Cycles 23 and 24. These events a