Characterising coronal turbulence using snapshot imaging of radio bursts in 80–200 MHz
A Mohan - Astronomy & Astrophysics, 2021 - aanda.org
Context. Metrewave solar type-III radio bursts offer a unique means to study the properties of
turbulence across coronal heights. Theoretical models have shown that the apparent …
turbulence across coronal heights. Theoretical models have shown that the apparent …
Fine structure of type III solar radio bursts from Langmuir wave motion in turbulent plasma
The Sun frequently accelerates near-relativistic electron beams that travel out through the
solar corona and interplanetary space. Interacting with their plasma environment, these …
solar corona and interplanetary space. Interacting with their plasma environment, these …
Global solar magnetic field and interplanetary scintillations during the past four solar cycles
The extended minimum of Solar Cycle 23, the extremely quiet solar-wind conditions
prevailing and the mini-maximum of Solar Cycle 24 drew global attention and many authors …
prevailing and the mini-maximum of Solar Cycle 24 drew global attention and many authors …
Direct observation of solar wind proton heating from in situ plasma measurements
Aims. We determine the perpendicular and parallel proton heating rate in the solar wind,
which is one of the primary goals of the Parker Solar Probe mission. Methods. To estimate …
which is one of the primary goals of the Parker Solar Probe mission. Methods. To estimate …
The role of plasma heating and expansion in the energetics of solar coronal mass ejections
N THEJASWI S - 2019 - dr.iiserpune.ac.in
Coronal Mass Ejections (CMEs) are bodily expulsions of hot plasma and magnetic fields
from the solar corona. Such ejections, which are often directed towards the Earth cause …
from the solar corona. Such ejections, which are often directed towards the Earth cause …