“The original publication is available at www.springerlink.com” Copyright Springer [Full text of this paper is not available in the UHRA]Optical polarimetry observations on La Palma, Canary Islands, during a Saharan dust episode showed dichroic extinction, indicating the presence of vertically aligned particles in the atmosphere. It is postulated that the alignment was due to an electric field of the order of 1 kV/m or greater. Two alternative mechanisms for the origin of the field are examined, including the effect of reduced atmospheric conductivity and the presence of charged dust
It is well known that aligned, aspherical dust grains emit polarized radiation and that the degree o...
polarization at 800 and 1100 mu m has been observed in the star-forming regions Mon R2, DR21 and W3-...
Context. The sub-millimetre polarisation of dust emission from star-forming clouds carries informati...
Abstract. Optical polarimetry observations on La Palma, Canary Islands, during a Saharan dust episod...
© Author(s) 2007. This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAl...
We carry out an investigation of the influence of particle alignment on the scattering properties of...
© 2021 COMECAP CONFERENCE. All rights reserved. No part of this book may be reproduced or transmitte...
Electrification of atmospheric dust influences the coagulation, wet removal and fall speeds of dust ...
Preferential particle orientation has been previously reported for desert dust and attributed on atm...
Dust particles in lofted atmospheric layers may present a preferential orientation, which could be d...
Atmospheric Electric Potential Gradient (PG) measurements were carried out in three sites forming a ...
We report on the electric field variations during Saharan dust advection over two atmospheric remote...
Gravitational sedimentation of charged dust and its subsequent discharging by ionospheric electrons ...
We report on the electric field variations during Saharan dust advection over two atmospheric remote...
Context. Polarized extinction and emission from dust in the interstellar medium (ISM) are hard to in...
It is well known that aligned, aspherical dust grains emit polarized radiation and that the degree o...
polarization at 800 and 1100 mu m has been observed in the star-forming regions Mon R2, DR21 and W3-...
Context. The sub-millimetre polarisation of dust emission from star-forming clouds carries informati...
Abstract. Optical polarimetry observations on La Palma, Canary Islands, during a Saharan dust episod...
© Author(s) 2007. This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAl...
We carry out an investigation of the influence of particle alignment on the scattering properties of...
© 2021 COMECAP CONFERENCE. All rights reserved. No part of this book may be reproduced or transmitte...
Electrification of atmospheric dust influences the coagulation, wet removal and fall speeds of dust ...
Preferential particle orientation has been previously reported for desert dust and attributed on atm...
Dust particles in lofted atmospheric layers may present a preferential orientation, which could be d...
Atmospheric Electric Potential Gradient (PG) measurements were carried out in three sites forming a ...
We report on the electric field variations during Saharan dust advection over two atmospheric remote...
Gravitational sedimentation of charged dust and its subsequent discharging by ionospheric electrons ...
We report on the electric field variations during Saharan dust advection over two atmospheric remote...
Context. Polarized extinction and emission from dust in the interstellar medium (ISM) are hard to in...
It is well known that aligned, aspherical dust grains emit polarized radiation and that the degree o...
polarization at 800 and 1100 mu m has been observed in the star-forming regions Mon R2, DR21 and W3-...
Context. The sub-millimetre polarisation of dust emission from star-forming clouds carries informati...