{"id":64,"date":"2019-09-24T15:40:11","date_gmt":"2019-09-24T13:40:11","guid":{"rendered":"https:\/\/sites.lesia.obspm.fr\/sasikumar-raja-kantepalli\/?page_id=64"},"modified":"2019-11-19T02:13:37","modified_gmt":"2019-11-19T01:13:37","slug":"presentations","status":"publish","type":"page","link":"https:\/\/sites.lesia.obspm.fr\/sasikumar-raja-kantepalli\/?page_id=64","title":{"rendered":"Presentations"},"content":{"rendered":"\n<h3 class=\"wp-block-heading\" id=\"h.p_ID_32\">Oral Presentations<\/h3>\n\n\n\n<ol class=\"wp-block-list\"><li>\u201cDensity turbulence in the solar wind using low-frequency angular broadening observations\u201d, Astronomy Seminar, Indian Institute of Astrophysics, Bengaluru, India, 22 August 2019.<\/li><li>\u201cNan\u00e7ay Decameter Array: Calibration\u201d, Internal meeting, Observatoire de Paris, Meudon, France, 2019.<\/li><li>\u201cTurbulent density fluctuations and proton heating rate in the solar wind from 9 \u2212 20 R \u2299 \u201d, Franco- British Alliance meeting, Observatoire de Paris, Paris, France, 9-10 April 2019.<\/li><li>\u201cTurbulent density fluctuations and proton heating rate in the solar wind from 9 \u2212 20 R \u2299 \u201d, Observatoire de Paris, Meudon, France, 15 January 2019.<\/li><li>\u201cSolar wind density turbulence from 2 \u2212 45 R \u2299 \u201d, Udaipur Solar Observatory, Physical Research Laboratory, Udaipur, Rajasthan, India, 28 November 2018.<\/li><li>\u201cTurbulent density fluctuations and proton heating rate in the solar wind from 9 \u2212 20 R \u2299 \u201d, Department Seminar, Astronomy and Astrophysics Division, Thaltej campus, Physical Research Laboratory, Ahmedabad, India, 15 November 2018.<\/li><li>\u201cTurbulent density fluctuations and proton heating rate in the solar wind from 9 \u2212 20 R \u2299 \u201d, 36th meeting of Astronomical Society of India hosted by Osmania University, Hyderabad, India, 5-9 February 2018.<\/li><li>\u201cCALLISTO Spectrometer at IISER-Pune\u201d, IEEE Indian Antenna Week &#8211; 2017, Defence Institute of Advanced Technology, Pune, India during 5-9 June 2017.<\/li><li>\u201cDensity turbulence in the solar wind using low-frequency angular broadening observations\u201d, Solar Physics Journal Club hosted by IISER, Pune, India, 14 December 2017.<\/li><li> \u201cMagnetic field measurements in the inner solar corona using low-frequency radio observations\u201d, Annual Academic Meeting, Key Laboratory of Solar Activities, Chinese Academy of Sciences, Beijing, China, 4-6 January 2016.<\/li><li> \u201cRadio Polarization Studies of Solar corona at Low-frequencies\u201d, Solar Physics Journal Club hosted by IISER, Pune, India, 7 July 2016.<\/li><li>Thesis presentation titled \u201cRadio Polarization Studies of Solar corona at Low-frequencies\u201d at 34th meeting of Astronomical Society of India hosted by Kashmir University, Srinagar, India, 10-13 May 2016.<\/li><li> \u201cDesign and performance study of a meter wavelength narrow band cross-polarized log-periodic dipole antenna to observe the polarized radio emission\u201d, at 33rd meeting of Astronomical Society of India hosted by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research, Pune, India, 17-20 February 2015.<\/li><li>Public talk on \u201cSun and Solar system\u201d during school outreach conducted by Indian Institute of Astrophysics, Bangalore at Model school, Ramasamudram, India, 15 November 2014.<\/li><li> \u201cLow-frequency observations of transient quasi-periodic radio emission from the Solar atmosphere\u201d, Regional Conference on Radio Science hosted by Symbiosis International University, Pune, India, January 2-5, 2014.<\/li><li> \u201cDesign and performance study of meter wavelength cross-polarized log-periodic dipole antenna to observe the polarized radio emissions from the solar atmosphere\u201d, Regional Conference on Radio Science hosted by Symbiosis International University, Pune, India, January 2-5, 2014.<\/li><\/ol>\n\n\n\n<h2 class=\"wp-block-heading\" id=\"h.p_ID_66\"><a href=\"https:\/\/sites.google.com\/view\/sskmrrj\/presentations#h.p_ID_66\"><\/a>Poster Presentations:<\/h2>\n\n\n\n<ol class=\"wp-block-list\"><li>\u201cSpectral distribution of solar radio type III bursts from 20 kHz to 80 MHz\u201d, CESRA2019: The Sun and the inner heliosphere, Potsdam, Germany, 8-12 July 2019.<\/li><li>\u201cSolar cycle dependence of the density fluctuations and proton heating rate in the solar wind\u201d, Long-term Data-sets for the Understanding of Solar and Stellar Magnetic Cycles, IAU Symposium 340, Jaipur, India, 19-24 February 2018.<\/li><li>\u201cAutomatic detection and classification of solar radio bursts using machine learning and deep learning techniques\u201d, 36th meeting of Astronomical Society of India, Osmania University, Hyderabad, India, 5-9 February 2018.<\/li><li>Poster + 1-minute oral presentation on \u201cAmplitude of solar wind density turbulence from 10 \u2212 45 R \u2299 \u201d, Square Kilometer Array Meeting (SKA-2016), Goa, India, 7-11 October 2016.<\/li><li>\u201cPolarization studies of the type I storm bursts at low frequencies,\u201d in Astronomical Society of India meeting, Trivandrum, India, February 20-22, 2013.<\/li><li>\u201cLow-frequency radio observations of picoflare category energy releases in the solar atmosphere,\u201d COSPAR meeting, Mysore, India, July 14-22, 2012.<\/li><li> \u201cLTPDIMM seeing monitor\u201d, the in-house meeting of Indian Institute of Astrophysics\u201d, Bangalore, 2008.<\/li><\/ol>\n","protected":false},"excerpt":{"rendered":"<p>Oral Presentations \u201cDensity turbulence in the solar wind using low-frequency angular broadening observations\u201d, Astronomy Seminar, Indian Institute of Astrophysics, Bengaluru, India, 22 August 2019. \u201cNan\u00e7ay Decameter Array: Calibration\u201d, Internal meeting, Observatoire de Paris, Meudon, France, 2019. \u201cTurbulent density fluctuations and proton heating rate in the solar wind from 9 \u2212 20 R \u2299 \u201d, Franco- <a class=\"more-link\" href=\"https:\/\/sites.lesia.obspm.fr\/sasikumar-raja-kantepalli\/?page_id=64\">Continue reading <i class=\"fa 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