High-rigidity Forbush decreases: due to CMEs or shocks?
KP Arunbabu, HM Antia, SR Dugad, SK Gupta… - Astronomy & …, 2013 - aanda.org
Aims. We seek to identify the primary agents causing Forbush decreases (FDs) in high-
rigidity cosmic rays observed from the Earth. In particular, we ask if these FDs are caused …
rigidity cosmic rays observed from the Earth. In particular, we ask if these FDs are caused …
Can solar wind viscous drag account for coronal mass ejection deceleration?
P Subramanian, A Lara… - Geophysical research …, 2012 - Wiley Online Library
The forces acting on solar Coronal Mass Ejections (CMEs) in the interplanetary medium
have been evaluated so far in terms of an empirical drag coefficient CD∼ 1 that quantifies …
have been evaluated so far in terms of an empirical drag coefficient CD∼ 1 that quantifies …
Kinematic properties of slow ICMEs and an interpretation of a modified drag equation for fast and moderate ICMEs
T Iju, M Tokumaru, K Fujiki - Solar Physics, 2014 - Springer
We report kinematic properties of slow interplanetary coronal mass ejections (ICMEs)
identified by SOHO/LASCO, interplanetary scintillation, and in situ observations and propose …
identified by SOHO/LASCO, interplanetary scintillation, and in situ observations and propose …
An analytical model of interplanetary coronal mass ejection interactions
We present an analytical model that describes the evolution of two consecutive
interplanetary coronal mass ejections (ICMEs), their interaction, and the evolution of the …
interplanetary coronal mass ejections (ICMEs), their interaction, and the evolution of the …
CMEs' speed, travel time, and temperature: A thermodynamic approach
HJ Durand‐Manterola, A Flandes… - Journal of …, 2017 - Wiley Online Library
Due to their important role in space weather, coronal mass ejections or CMEs have been
thoroughly studied in order to forecast their speed and transit time from the Sun to the Earth …
thoroughly studied in order to forecast their speed and transit time from the Sun to the Earth …
Generalized additive modeling combined with multiple collinear for ICME velocity forecasting
One of the main issues of space weather is the timely prediction of disturbed solar wind
parameters at L1, especially caused by Coronal Mass Ejection (CME). Using the data from …
parameters at L1, especially caused by Coronal Mass Ejection (CME). Using the data from …
[PDF][PDF] Identificación y caracterización de tubos de flujo magnético en el medio interplanetario a pequeña escala
LFV Ramirez, AL Sanchez - ru.dgb.unam.mx
El estudio de los tubos de flujo magnético es de gran importancia para comprender la
dinámica del viento solar y sus efectos en el entorno espacial cercano a la Tierra. La …
dinámica del viento solar y sus efectos en el entorno espacial cercano a la Tierra. La …
Coronal Mass Ejections from the Sun-Propagation and Near Earth Effects
A Babu - arXiv preprint arXiv:1407.4258, 2014 - arxiv.org
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 …
near-Earth space environment is proving to be increasingly crucial. Earth-directed Coronal …