HelioWebTIFR, National Centre for Radiophysics, Pune
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I[TIFR, National Centre for Radiophysics, Pune]
PI["Parent Institutions (1)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (34)"]
CA["Linked Collaborating Authors (9)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
click PI "#parent-institutions"
click CI "#child-institutions"
click AW "#affiliated-works"
click CA "#collaborating-authors"
Parent Institutions [?]
Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- Radio Observations of Rapid Acceleration in a Slow Filament Eruption/Fast CME Event
- MEXART Measurements of Radio Sources. Interplanetary Scintillation Array in Mexico
- Search for Radio Emission from Extrasolar Planets with the GMRT: Some Results from the 2004 Data and a Preliminary Look at the 2005 Data
- Search for Radio Emissions From Extrasolar Planets at 150 MHz
- MEXART. Interplanetary Scintillation Array in Mexico in the IHY2007
- First IPS Radio Sources Detected By MEXART
- SMEI Remote Sensing and the 3D Reconstruction of Corotating Heliospheric Structures
- Solar Wind 3D Reconstructions of the Whole Heliospheric Interval
- Solar Science with the Murchison Widefield Array: Commissioning and Beyond
- A New Class of Weak Radio Bursts: Nanoflares and Coronal Heating?
- Automated Discovery of Short Duration Solar Radio Bursts in Murchison-Widefield Array (MWA) Data
- Solar Magnetic Reconnection at Low Altitudes and Associated Type III Solar Radio Bursts and X-Ray Emission
- High Fidelity Solar and Heliospheric Imaging at Low Radio Frequencies: Progress and Future Prospects
- Interplanetary Scintillation Observations with a New Generation of Radio Telescopes: First results from the MWA
- Modeling the Solar Wind throughout Interplanetary Space Using Ground-based and Spacecraft Observational Data
- Potential Use of Observations of Interplanetary Scintillation (IPS) and Faraday Rotation (FR) in Support of the Solar Orbiter and Solar Probe Plus Missions
- Power Law of Micro-Scale Turbulence in the Solar Wind Combining Observations of IPS at Different Wavelengths
- The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network in support of Space-Weather Science and Forecasting
- Wavelet Based Characterization of Low Radio Frequency Solar Emissions
- How Interplanetary Scintillation Data Can Improve Modeling of Coronal Mass Ejection Propagation
- The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network October 2016 Observing Campaign: Initial WIPSS Data Analyses
- New Insights from Spectroscopic Snapshot Imaging of Weak Type III Radio Bursts using MWA
- Routine Estimation of Coronal Mass Ejection Magnetic Fields at Coronal Heights
- The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network: A Ground-Based Heliospheric Observatory for Science and Space Weather
- A detailed look at a type II radio burst using the Murchison Widefield Array
- Constraining the Physical Parameters of Coronal Mass Ejections at Large Coronal Heights using Low Radio Frequency Gyrosynchrotron Emission
- Estimating Coronal Propagation Effects in the Quiet Sun Corona Using Low Radio Frequency Observations
- First radio evidence of ubiquitous magnetic reconnections and impulsive heating in the quiet solar corona
- Applying Unsupervised Machine Learning to Characterize Weak Impulsive Narrowband Quiet Sun Emissions in the Radio Spectrum
- Characterising the Properties of Weak Impulsive Narrowband Quiet Sun Emissions and Their Relationship with EUV Bursts
- Probing coronal magnetic fields using high fidelity low-frequency spectro-polarimetric radio imaging with SKA precursor
- First detailed polarimetric study of a group of type-III solar radio bursts with the Murchison Widefield Array
- First detailed polarimetric study of a type II solar radio burst with the Murchison Widefield Array
- First ever measurement of quiet solar coronal magnetic field using low-frequency radio observation