In this section
@inproceedings{Rodriguez:2005,
author = {Rodriguez, L and Woch, J and Krapp, N and Fränz, M and Von, Steiger R and Cid, C and Forsyth, R and Glaßmeier, KH},
pages = {759--762},
title = {Freezing-in temperatures of oxygen, carbon and iron in magnetic clouds},
year = {2005}
}
TY - CPAPER
AB - Magnetic clouds (MCs) represent nearly one third of all the interplanetary coronal mass ejections (ICMEs) seen by Ulysses. The ionization level of the solar wind plasma serves as a robust tool to characterize different types of solar wind. Charge states of heavy ions have been used in this work to infer the temperatures in the source region of ICMEs. MCs show increased temperatures with respect to non-cloud ICMEs and surrounding solar wind. Oxygen ions are found to provide a very good signature of magnetic clouds in the solar wind. The profiles of oxygen, carbon and iron are compared, in order to establish relations between them; inside MCs and in their surrounding solar wind.
AU - Rodriguez,L
AU - Woch,J
AU - Krapp,N
AU - Fränz,M
AU - Von,Steiger R
AU - Cid,C
AU - Forsyth,R
AU - Glaßmeier,KH
EP - 762
PY - 2005///
SN - 0379-6566
SP - 759
TI - Freezing-in temperatures of oxygen, carbon and iron in magnetic clouds
ER -