scholarly journals The research on small-scale structures of ice particle density and electron density in the mesopause region

2019 ◽  
Author(s):  
Anonymous
2019 ◽  
Author(s):  
Ruihuan Tian ◽  
Jian Wu ◽  
Jinxiu Ma ◽  
Yonggan Liang ◽  
Hui Li ◽  
...  

Abstract. In this paper, a growth and motion model is developed to investigate the evolution of radius, velocity, and number density of ice particles in mesopause region. In the growth model, meteoric dust from outer atmosphere and grains moving with the upward neutral wind from the mesosphere bottom serve as nuclei upon which water vapor can condense in the cold and moist condition. And the motion of the ice particles is mainly controlled by the gravity and the neutral drag force. It is shown that the radius of ice particles increases linearly with time. But the particle velocity has a complicated relationship with the radius due to the different mass densities of condensation nuclei and absorbed ice. For certain condensation core radius, the velocity of particles can be reversed at particular height, which leads to local gathering of particles near the boundary layer and small-scale structures of ice particle density on the order of a few meters. Based on the obtained small-scale ice particle distribution, the mean particle charge number and corresponding distributions of electrons are calculated by combining the dust charging processes and quasi-neutrality condition. It shows that the absorption of electrons by ice particles results in the formation of small-scale electron density structures, which can be important to the research on the cause of polar mesosphere summer echoes (PMSE).


2019 ◽  
Vol 37 (6) ◽  
pp. 1079-1094
Author(s):  
Ruihuan Tian ◽  
Jian Wu ◽  
Jinxiu Ma ◽  
Yonggan Liang ◽  
Hui Li ◽  
...  

Abstract. The formation of ice particle density irregularities with a meter scale in the mesopause region is explored in this paper by developing a growth and motion model of ice particles based on the motion equation of a variable mass object. The growth of particles by water vapor adsorption and the action of gravity and the neutral drag force on particles are considered in the model. The evolution of the radius, velocity, and number density of ice particles is then investigated by solving the growth and motion model numerically. For certain nucleus radii, it is found that the velocity of particles can be reversed at a particular height, leading to a local gathering of particles near the boundary layer, which then forms small-scale ice particle density structures. The spatial scale of the density structures can be affected by vertical wind speed, water vapor density, and altitude, and it remains stable as long as these environmental parameters do not change. The influence of the stable small-scale structures on electron and ion density is further calculated by a charging model, which considers the production, loss, and transport of electrons and ions, along with dynamic particle charging processes. Results show that the electron density is anti-correlated to the charged ice particle density and ion density for particles with radii of 11 nm or less due to plasma attachment by particles and plasma diffusion. This finding is in accordance with most rocket observations. The small-scale electron density structures created by small-scale ice particle density irregularities can produce the polar mesosphere summer echo (PMSE) phenomenon.


2000 ◽  
Vol 179 ◽  
pp. 403-406
Author(s):  
M. Karovska ◽  
B. Wood ◽  
J. Chen ◽  
J. Cook ◽  
R. Howard

AbstractWe applied advanced image enhancement techniques to explore in detail the characteristics of the small-scale structures and/or the low contrast structures in several Coronal Mass Ejections (CMEs) observed by SOHO. We highlight here the results from our studies of the morphology and dynamical evolution of CME structures in the solar corona using two instruments on board SOHO: LASCO and EIT.


2007 ◽  
Vol 3 (S247) ◽  
pp. 152-157 ◽  
Author(s):  
Oddbjørn Engvold

AbstractSeismology has become a powerful tool in studies of the magnetic structure of solar prominences and filaments. Reversely, analytical and numerical models are guided by available information about the spatial and thermodynamical structure of these enigmatic structures. The present invited paper reviews recent observational results on oscillations and waves as well as details about small-scale structures and dynamics of prominences and filaments.


2009 ◽  
Vol 399 (1) ◽  
pp. 195-208 ◽  
Author(s):  
Jacco Th. van Loon ◽  
Keith T. Smith ◽  
Iain McDonald ◽  
Peter J. Sarre ◽  
Stephen J. Fossey ◽  
...  

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