Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Sundar, M. N."'
Publikováno v:
2020Ap&SS.365..139R
An isolated, isothermal, and wide magnetic flux tube embedded either in the solar chromosphere or in the lower solar corona is considered, and the propagation of linear torsional Alfv'en waves is investigated. It is shown that the wideness of the tub
Externí odkaz:
http://arxiv.org/abs/2008.03653
Autor:
Thomas, Adam D., Dopita, Michael A., Shastri, Prajval, Davies, Rebecca, Hampton, Elise, Kewley, Lisa, Banfield, Julie, Groves, Brent, James, Bethan L., Jin, Chichuan, Juneau, Stéphanie, Kharb, Preeti, Sairam, Lalitha, Scharwächter, Julia, Shalima, P., Sundar, M. N., Sutherland, Ralph, Zaw, Ingyin
We present the second and final data release of the Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7). Data are presented for 63 new galaxies not included in the first data release, and we provide 2D emission-line fitting products for
Externí odkaz:
http://arxiv.org/abs/1708.02683
Publikováno v:
Adv. Space Res., 61-2 (2018), 715-719
Solar prominences are magnetic structures incarcerating cool and dense gas in an otherwise hot solar corona. Prominences can be categorized as quiescent and active. Their origin and the presence of cool gas (~$10^4$K) within the hot (~$10^6$K) solar
Externí odkaz:
http://arxiv.org/abs/1608.07674
Autor:
Shastri, Prajval, Dopita, Mike, Banfield, Julie, Thomas, Adam, Longbottom, Fergus, Sundar, M. N., Duggal, Chetna, Groves, Brent, Kharb, Preeti, Davies, Rebecca, Kewley, Lisa, Sairam, Lalitha, Hampton, Elise, Puthiyaveettil, Shalima, James, Bethan
Publikováno v:
AIP Conference Proceedings; 2019, Vol. 2109 Issue 1, p090003-1-090003-4, 4p, 2 Charts
Akademický článek
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Autor:
Shastri, P., Dopita, M., Scharwächter, J., Kewley, L., Davies, R., Sutherland, R., Kharb, P., Banfield, J., Jose, J., Ramya, S., Srivastava, S., Bhatt, H. C., Hampton, E., Jin, J., Basurah, H., Fischer, S., Gupta, M., Panda, S., Sundar, M. N., Radhakrishnan, V.
Publikováno v:
AIP Conference Proceedings; 2015, Vol. 1697 Issue 1, p1-3, 3p, 1 Graph