SH022
Radio Solar and Heliospheric Observations, Instruments, and Modelling for Space Weather Research, Applications, and Forecasting
Session ID#: 251977
Session Description:
The use of solar/heliospheric radio observations, and their data as inclusion into models or in constraining models, is ever-expanding across the space-weather (SW) domain. This includes the pure blue-skies research (e.g. Faraday rotation), heliospheric monitoring and research capabilities including their use in forecasting tools (e.g. interplanetary scintillation), and in studying the quiet and active Sun (e.g. solar imaging/solar dynamic spectra). The use of wide-frequency bandwidth or multiple bands across the radio domain allows for different heights from the Sun to be probed, as well as a whole range of heliospheric distances out from the Sun to well beyond Earth’s orbit. In this session we focus primarily on the SW research, applications, and forecasting capabilities that radio is able to offer, showcasing the use of ground-/space-based radio capabilities to the wider solar/heliospheric communities. In addition, we welcome contributions about ground-/space-based radio instrumentation on current/future concepts that will have solar/heliospheric SW capabilities.
Co-Sponsor(s):
Index Terms:
6994 Instruments and techniques [RADIO SCIENCE]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7924 Forecasting [SPACE WEATHER]
7959 Models [SPACE WEATHER]
Primary Convener: Bernard V Jackson, University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States
Convener: Mario Mark Bisi, United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
Estimating Solar Wind Speeds Using Doppler Broadening: Results from MOM and Akatsuki (1856320)
Keshav Aggarwal, IIT Indore, Department of Astronomy, Astrophysics and Space Engineering, Indore, India, R. K. Choudhary, Space Physics Laboratory, Trivandrum, India and Abhirup Datta, Indian Institute of Technology Indore, Discipline of Astronomy, Astrophysics and Space Engineering, Indore, India
An Interplanetary Scintillation Kp Forecast Five Days in Advance Derived from 3-D Velocity, Density, and Solar Surface Extrapolated GSM Component Fields (1937652)
Bernard V Jackson1, Andrew Buffington1, Kazumasa Iwai2 and Mario Mark Bisi3, (1)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (2)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (3)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
Real-time Solar and Heliospheric Diagnostics with the Owens Valley Radio Observatory Long Wavelength Array (1963733)
Dr. Peijin Zhang1, Bin Chen2, Surajit Mondal2, Dale E Gary2 and OVRO-LWA team, (1)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Edison, NJ, United States, (2)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States
A Time-of-Arrival Technique to Estimate the Source of a Solar Radio Burst (1979751)
Julia Kirkey1, Jamie Hendrickson2, Saul Roman-Ramirez2, Mojtaba Akhavan-Tafti3, Jason Earl Kooi4, Brian Hicks5 and Tracy Clarke5, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan Ann Arbor, Ann Arbor, United States, (3)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)US Naval Research Laboratory, Washington, United States, (5)US Naval Research Laboratory, Washington DC, United States
Radio Investigations for Space Environment Research (RISER): Progress and Plans Two Year In... (1981239)
Mario Mark Bisi1, Biagio Forte2, Steve E. Milan3, David Jackson4, Richard Fallows1, Bernard V Jackson5, Dusan Odstrcil6, Edmund Henley4, Oyuki Chang1, David Barnes1, Matthew Bracamontes7, Siegfried Gonzi4 and Paul Kinsler2, (1)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (2)University of Bath, Department of Electronic and Electrical Engineering, Bath, United Kingdom, (3)University of Leicester, Leicester, United Kingdom, (4)Met Office, Exeter, United Kingdom, (5)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (6)George Mason University, Fairfax, United States, (7)University of California, San Diego, La Jolla, CA, United States
Kilometric Type II Radio Bursts and Interplanetary Shocks: A Complete Survey (1981721)
Franco Manini1, Hebe Cremades1, Fernando López1 and Teresa Nieves-Chinchilla2, (1)Grupo de Estudios en Heliofísica de Mendoza, CONICET, Universidad de Mendoza, Mendoza, Argentina, (2)NASA Goddard Space Flight Center, Heliophysics Science Division, MD, United States
Predicting Full-Disk Solar F10.7 Images with a Deep Learning Method (1999391)
Meiqi Wang1, Haodi Jiang2, Sijie Yu3, Bin Chen3, Peijin Zhang3 and Jason T. L. Wang4, (1)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Edison, NJ, United States, (2)Sam Houston State University, Huntsville, United States, (3)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (4)Institute for Space Weather Sciences, New Jersey Institute of Technology, Newark, United States
Validating MHD Simulations of CMEs Using IPS Observations (2001242)
Nariaki Nitta1, Meng Jin1, Kazumasa Iwai2 and Daikou Shiota3, (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (2)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (3)NICT National Institute of Information and Communications Technology, Tokyo, Japan
