Coronal mass ejections (CMEs) play an important role in space weather. The propagation
characteristics of CMEs in the Corona and interplanetary space determine whether, when …

Context. Coronal mass ejections (CMEs) are the primary source of strong space weather
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …

Interplanetary (IP) shocks are perturbations observed in the solar wind. IP shocks correlate
well with solar activity, being more numerous during times of high sunspot numbers. Earth …

One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …

In this work, we present results of a time-dependent data-driven numerical simulation
developed to study the dynamics of coronal active region magnetic fields. The evolving …

We report a detailed analysis of interplanetary flux ropes observed at Venus and
subsequently at Earth's Lagrange L1 point between June 15 and 17, 2012. The observation …

Predicting the magnetic field within an Earth‐directed coronal mass ejection (CME) well
before its arrival at Earth is one of the most important issues in space weather research. In …

The Space Weather Investigation Frontier (SWIFT) mission will aim at making major
discoveries on the three-dimensional structure and dynamics of heliospheric structures that …

Abstract We utilize Total Electron Content (TEC) measurements and electron density (Ne)
retrieval profiles from Global Navigation Satellite System (GNSS) receivers onboard multiple …

Abstract Analysis of the variation in galactic cosmic rays and changes in various
characteristics of Forbush effects associated with the influence of interacting solar wind …