Zobrazeno 1 - 10
of 102
pro vyhledávání: '"Suresh Venkata"'
Autor:
Sunderamurthe Satisvar, Subash Chandra Bose Gopinath, Mohd Khairuddin Md Arshad, Dee Vie Ong, Thangavel Lakshmipriya, Chun Hong Voon, Uda Hashim, Abdul Rahim Ruslinda, Suresh Venkata Chinni
Publikováno v:
Songklanakarin Journal of Science and Technology (SJST), Vol 39, Iss 3, Pp 373-381 (2017)
In tandem to the Salmonellosis infection worldwide, a study was conducted to determine the conserved and nonconserved region in Salmonella enterica sub-species so that it can be used to design probes in biosensors for the detection of Salmonella en
Externí odkaz:
https://doaj.org/article/a29c3591c8464cc6ac258df30be10030
Autor:
Nagaraju, K., Prasad, B. Raghavendra, Hegde, Bhavana S., Narra, Suresh Venkata, Utkarsha, D., Kumar, Amit, Singh, Jagdev, Kumar, Varun
One of the major science goals of the Visible Emission Line Coronagraph (VELC) payload aboard the Aditya-L1 mission is to map the coronal magnetic field topology and the quantitative estimation of longitudinal magnetic field on routine basis. The inf
Externí odkaz:
http://arxiv.org/abs/2108.08997
Publikováno v:
In Advances in Space Research 1 October 2019 64(7):1455-1464
Akademický článek
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Akademický článek
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Publikováno v:
Experimental Astronomy. 53:71-82
Autor:
S. Nagabhushana, B. Raghavendra Prasad, Suresh Nagesh, Suresh Venkata Nara, D. S. Sandeep, P. U. Kamath, Shalab Misra, Bhavana Hegde, D. Utkarsha, Mrityunjay Kumar Sinha, S. Kathiravan, V. Natarajan, S. Pawan Kumar, Amit Kumar
Publikováno v:
Journal of Astronomical Instrumentation. 11
One of the major objectives of the optomechanics is to support large optics required for the purpose and also to maintain high dynamic stability in operation. This requirement calls for more number of supports, to support large optics. While addressi
Autor:
Tan, Xinq Yuan, Citartan, Marimuthu, Chinni, Suresh Venkata, Ahmed, Siti Aminah, Tang, Thean-Hock
Publikováno v:
Indian Journal of Microbiology; Mar2023, Vol. 63 Issue 1, p33-41, 9p
Publikováno v:
Advances in Space Research. 64:1455-1464
It is very important to make the spectrographic observations of the outer emission corona in number of emission lines simultaneously in view of the results of the observations made in [Fe x] 6374 A, [Fe xi] 7892 A, [Fe xiv] 5303 A and [Fe xiii] 10,74
Understanding solar coronal magnetic fields is crucial to address the long-standing mysteries of the solar corona and solar wind. Although routine photospheric magnetic fields (MFs) are available for decades, coronal MFs are rarely reported. Visible
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f4c13926983e83feec53aca9bd33df2
http://arxiv.org/abs/2110.14179
http://arxiv.org/abs/2110.14179