Thank you for opening the third edition of this monograph. The first edition [202] was
published in 1996 in the Lecture Notes in Control and Information Sciences series (vol. 220) …

" The study of planet formation has a long history. The idea that the Solar System formed
from a rotating disk of gas and dust-the Nebula Hypothesis-dates back to the writings of …

Water ice is one of the most abundant materials in dense molecular clouds and in the outer
reaches of protoplanetary disks. In contrast to other materials (eg, silicates), water ice is …

Water ice is abundant in protoplanetary disks. Its sticking properties are therefore important
during phases of collisional growth. In this work, we study the sticking and rolling of 1.1 mm …

This review paper examines the dynamics of snow accumulation on vehicle surfaces and its
impacts on vehicle performance and safety. It focuses on the use of computational fluid …

The blowing of sand by wind, known as saltation, ejects dust aerosols into the atmosphere,
creates sand dunes, and erodes geological features. We present a comprehensive …

The present work deals with ice particle fragmentation resulting from impact on a solid wall.
First, a semi-empirical model to predict the size of the largest reemited fragment is …

Snow and ice accumulation on surfaces presents significant safety and efficiency challenges
across various industries, necessitating the development of effective mitigation strategies. In …

The outcome of collisions between small icy bodies, such as Kuiper belt objects, is poorly
understood and yet a critical component of the evolution of the trans-neptunian region. The …

In the framework of HAIC European project, a capability for modeling glaciated and mixed-
phase ice accretion has been added to IGLOO2D, the new ONERA 2D icing suite. A first set …