Zobrazeno 1 - 10
of 40
pro vyhledávání: '"S. P. Bagare"'
Publikováno v:
Advances in Astronomy, Vol 2015 (2015)
The physical conditions of celestial objects can be analyzed using the spectrum of atoms or molecules present in the object. The present work focuses on the spectroscopic analysis of astrophysically significant molecule AlF. The evaluation of Franck-
Externí odkaz:
https://doaj.org/article/dc1270f744a54a3abb5b9a79a1aef95d
Publikováno v:
The European Physical Journal Plus. 137
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::668c8163c922845c0de4b95755792d89
https://doi.org/10.1140/epjp/s13360-022-03232-2
https://doi.org/10.1140/epjp/s13360-022-03232-2
Publikováno v:
New Astronomy. 78:101366
A high-resolution sunspot umbra spectrum recorded in National Solar Observatory, Kitt Peak in the visible and infrared wave number range 13, 600 – 25, 000cm−1 was taken in the present study for identifying the rotational lines of barium hydride (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b04000676f52ec1ce3be907e9f49b240
https://doi.org/10.1016/j.newast.2020.101366
https://doi.org/10.1016/j.newast.2020.101366
Publikováno v:
Solar Physics. 290:1569-1579
It is essential to know the composition of atoms or molecules present in the astrophysical objects concerned to determine the physical and chemical nature of a solar or stellar region. With the aim to identify them clearly, we therefore analyzed the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::afa1f314e64ef706823996eae1e91ec8
https://doi.org/10.1007/s11207-015-0702-3
https://doi.org/10.1007/s11207-015-0702-3
Autor:
S. P. Bagare
Publikováno v:
Proceedings of the International Astronomical Union. 6:308-314
In our earlier study of a revisit of the classic Wilson Effect, it was found that a large proportion of sunspots do not display the geometric effect which is ascribed to a depression of the umbra. It was shown that the presence or absence of the effe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::78fcd9c7db0540ad969e30bf10ccbb46
https://doi.org/10.1017/s1743921311015432
https://doi.org/10.1017/s1743921311015432
Publikováno v:
Solar Physics. 264:279-285
A search has been carried out for the presence of rotational lines of two bands of the (0, 0) and (1, 1) A 1Π – X 1Σ+ system of the AlH molecule in the high resolution Fourier Transform Spectra of sunspots observed at the National Solar Observato
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d0810d7e070e3d082b12d70eca504c3b
https://doi.org/10.1007/s11207-010-9590-8
https://doi.org/10.1007/s11207-010-9590-8
Publikováno v:
Research Notes of the AAS. 2:21
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::69f4c3efe1e549f1eb6bc3faafc489ec
https://doi.org/10.3847/2515-5172/aaabb9
https://doi.org/10.3847/2515-5172/aaabb9
Publikováno v:
Serbian Astronomical Journal, Vol 179, Pp 95-99 (2009)
Serbian Astronomical Journal, Vol 2009, Iss 179, Pp 95-99 (2009)
Serbian Astronomical Journal, Vol 2009, Iss 179, Pp 95-99 (2009)
A search for fourteen bands of the visible and infrared systems of the beryllium hydride isotopomers, in addition to the previously identified bands A - X(0, 0; 1, 1; 2, 2) for BeH, A - X(0, 0; 1, 1; 2, 2) for BeD and A - X(0, 0; 1, 1; 2, 2) for BeT
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64ffeb58adaa0d522f899949b1b6b496
http://saj.matf.bg.ac.rs/179/pdf/095-099.pdf
http://saj.matf.bg.ac.rs/179/pdf/095-099.pdf
Autor:
K. P. Raju, R. Srinivasan, Dipankar Banerjee, S. Muneer, Girjesh R. Gupta, S. S. Hasan, Jagdev Singh, S. P. Bagare
Publikováno v:
Solar Physics. 260:125-134
We obtained the images of the eastern part of the solar corona in the Fe xiv 530.3 nm (green) and Fe x 637.4 nm (red) coronal emission lines during the total solar eclipse of 29 March 2006 at Manavgat, Antalya, Turkey. The images were obtained using
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fdd28e9fedc7394a35b1a8570fb24e15
https://doi.org/10.1007/s11207-009-9434-6
https://doi.org/10.1007/s11207-009-9434-6
Publikováno v:
Astrophysics and Space Science. 323:41-49
A high resolution spectrum of a sunspot umbra is used for identification of rotational lines due to (0, 0) band of the A 2Π–X 2Σ+ system and (0, 0), (1, 1), and (2, 2) bands of the B 2Σ+–X 2Σ+ system of the molecule SrF. The published sunspot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b05a51af3835bad53386cd498f9e8de7
https://doi.org/10.1007/s10509-009-0043-5
https://doi.org/10.1007/s10509-009-0043-5