Coronal Mass Ejections from the Sun - Propagation and Near Earth Effects

TL;DR

This paper investigates the structure, propagation, and near-Earth effects of Coronal Mass Ejections (CMEs), emphasizing cosmic ray diffusion, turbulence, and magnetic forces, to better understand space weather disturbances affecting Earth.

Contribution

It provides new insights into CME structure, turbulence levels, and the forces driving CMEs, using cosmic ray observations and spacecraft data, advancing the understanding of CME propagation and effects.

Findings

Diffusion of galactic cosmic rays into CMEs causes Forbush decreases.

Turbulence in the sheath region influences cosmic ray diffusion and FD lag.

CMEs exhibit non-force-free magnetic fields, supporting Lorentz self-force driving.

Abstract

Owing to our dependance on spaceborne technology, an awareness of disturbances in the near-Earth space environment is proving to be increasingly crucial. Earth-directed Coronal mass ejections (CMEs) emanating from the Sun are the primary drivers of space weather disturbances. Studies of CMEs, their kinematics, and their near-Earth effects are therefore gaining in importance. The effect of CMEs near the Earth is often manifested as transient decreases in galactic cosmic ray intensity, which are called Forbush decreases (FDs). In this thesis we probe the structure of CMEs and their associated shocks using FD observations by the GRAPES-3 muon telescope at Ooty. We have established that the cumulative diffusion of galactic cosmic rays into the CME is the dominant mechanism for causing FDs (Chapter 3). This diffusion takes place through a turbulent sheath region between the CME and the shock. One of our main results concerns the turbulence level in this region. We have quantitatively established that cross-field diffusion aided by magnetic field turbulence accounts for the observed lag between the FD and the magnetic field enhancement of the sheath region (Chapter 4 ). We have also investigated the nature of the driving forces acting on CMEs in this thesis. Using CME data from the SECCHI coronagraphs aboard STEREO sapcecraft, we have found evidence for the non-force-free nature of the magnetic field configuration inside these CMEs, which is the basis for the (often-invoked) Lorentz self-force driving (Chapter 5). Taken together the work presented in this thesis is a comprehensive attempt to characterise CME propagation from typical coronagraph fields of view to the Earth.