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Kantepalli Sasikumar Raja
Kantepalli Sasikumar Raja
Assistant Professor, Indian Institute of Astrophysics, Bangalore, India
Email verificata su iiap.res.in - Home page
Titolo
Citata da
Citata da
Anno
An estimate of the magnetic field strength associated with a solar coronal mass ejection from low frequency radio observations
KS Raja, R Ramesh, K Hariharan, C Kathiravan, TJ Wang
The Astrophysical Journal 796 (1), 56, 2014
582014
Low-frequency radio observations of picoflare category energy releases in the solar atmosphere
R Ramesh, KS Raja, C Kathiravan, AS Narayanan
The Astrophysical Journal 762 (2), 89, 2012
542012
Low-frequency observations of transient quasi-periodic radio emission from the solar atmosphere
KS Raja, R Ramesh
The Astrophysical Journal 775 (1), 38, 2013
452013
Amplitude of solar wind density turbulence from 10 to 45 R⊙
K Sasikumar Raja, M Ingale, R Ramesh, P Subramanian, PK Manoharan, ...
Journal of Geophysical Research: Space Physics 121 (12), 11, 2016
242016
Design and performance of a low-frequency cross-polarized log-periodic dipole antenna
KS Raja, C Kathiravan, R Ramesh, M Rajalingam, IV Barve
The Astrophysical Journal Supplement Series 207 (1), 2, 2013
242013
Automated Detection of Solar Radio Bursts using a Statistical Method
D Singh, KS Raja, P Subramanian, R Ramesh, C Monstein
Solar Physics, 2019
232019
Global solar magnetic field and interplanetary scintillations during the past four solar cycles
KS Raja, P Janardhan, SK Bisoi, M Ingale, P Subramanian, K Fujiki, ...
Solar Physics 294 (9), 1-14, 2019
182019
A statistical study of solar radio Type III bursts and space weather implication
T Ndacyayisenga, J Uwamahoro, KS Raja, C Monstein
Advances in Space Research 67 (4), 1425-1435, 2021
152021
Observations of shock propagation through turbulent plasma in the solar corona
EP Carley, B Cecconi, HA Reid, C Briand, KS Raja, S Masson, ...
The Astrophysical Journal 921 (1), 3, 2021
142021
A statistical study of low-frequency solar radio type III bursts
A Mahender, K Sasikumar Raja, R Ramesh, V Panditi, C Monstein, ...
Solar Physics 295 (11), 153, 2020
132020
Turbulent Density Fluctuations and Proton Heating Rate in the Solar Wind from 9-20 R
K Sasikumar Raja, P Subramanian, R Ramesh, A Vourlidas, M Ingale
IOP Publishing, 2017
132017
Spectral analysis of solar radio type iii bursts from 20 khz to 410 mhz
KS Raja, M Maksimovic, EP Kontar, X Bonnin, P Zarka, L Lamy, H Reid, ...
The Astrophysical Journal 924 (2), 58, 2022
122022
Turbulent proton heating rate in the solar wind from 5–45 r⊙
KS Raja, P Subramanian, M Ingale, R Ramesh, M Maksimovic
The Astrophysical Journal 914 (2), 137, 2021
112021
Solar coronal magnetic fields and sensitivity requirements for spectropolarimetry channel of VELC onboard Aditya-L1
KS Raja, S Venkata, J Singh, BR Prasad
Advances in Space Research 69 (1), 814-822, 2022
92022
Eruption of the EUV Hot Channel from the Solar Limb and Associated Moving Type IV Radio Burst
P Vemareddy, P Démoulin, KS Raja, J Zhang, N Gopalswamy, ...
The Astrophysical Journal 927 (1), 108, 2022
82022
Dissipation scale lengths of solar wind turbulence
KS Raja, P Subramanian, M Ingale, R Ramesh
The Astrophysical Journal 872 (1), 77, 2019
82019
Trends and Characteristics of High-Frequency Type II Bursts Detected by CALLISTO Spectrometers
AC Umuhire, J Uwamahoro, KS Raja, A Kumar, C Monstein, II Block, ...
10.1016/j.asr.2021.06.029, 2021
52021
Two-stage evolution of an extended C-class eruptive flaring activity from sigmoid active region NOAA 12734: SDO and Udaipur-CALLISTO observations
B Joshi, PK Mitra, R Bhattacharyya, K Upadhyay, D Oberoi, KS Raja, ...
Solar Physics 296 (6), 85, 2021
52021
Turbulent density fluctuations and proton heating rate in the solar wind from 9-20~ R_ {\odot}
KS Raja, P Subramanian, R Ramesh, A Vourlidas, M Ingale
arXiv preprint arXiv:1710.06295, 2017
52017
Clearing certain misconception in the common explanations of the aerodynamic lift
N Singh, K Sasikumar Raja, P Janardhan
ARXIV, 9, 2018
32018
Il sistema al momento non può eseguire l'operazione. Riprova più tardi.
Articoli 1–20