Computer Science
Scientific paper
Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..347p&link_type=abstract
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 347-350 (2010).
Computer Science
Solar Wind, Solar Magnetism, Spacecraft, Solar Corona, Particle Emission, Solar Wind, Electric And Magnetic Fields, Solar Magnetism, Spacecraft/Atmosphere Interactions, Coronal Mass Ejection
Scientific paper
Fluctuations in the solar wind parameters and in the heliospheric magnetic field have been studied extensively. The nature of fluctuations has been shown to depend on the origin of the solar wind. However, the regions of transition between the high-speed and the slow speed streams have not been investigated with high resolution. In this work we use high resolution magnetic field measurements on the Ulysses spacecraft to calculate the variances of the fluctuations in the magnetic field components and its magnitude over several timescales, concentrating on intervals of rapid change in the solar wind parameters. At the same time, we computed the cross helicity to assess the Alfvénicity of the fluctuations and changes in it during transitions. The strong variability of all those parameters seems to indicate a filamentary nature of the heliospheric medium.
Balogh André
Perri Simona
No associations
LandOfFree
High resolution measurements of magnetic field fluctuations associated with transitions in solar wind parameters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with High resolution measurements of magnetic field fluctuations associated with transitions in solar wind parameters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High resolution measurements of magnetic field fluctuations associated with transitions in solar wind parameters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1423734