april 21, 2002 00:04:00

1
Relating Solar Source Magnetic Connectivity to SEP properties seen at 1 AU A.J. Coyner, D, Alexander, and M.I. Desai April 21, 2002 00:04:00 August 24, 2002 00:04:00 January 20, 2005 06:04:00 October 28, 2003 06:04:00 •We investigate the effects of solar magnetic configuration (determined with PFSS extrapolations) on observed (Fe/O) ratios for 42 events including January 20, 2005. •Comparisons with Fe/O made at ULEIS energies (0.32-0.45 MeV/Nuc) •January 20, 2005 specifically shows significant open field with the extrapolation. •Less open field magnetic flux than the other campaign events with open field. •We see correlations in the open field event data between Fe/O and open magnetic flux influenced by the high Fe/O ratio events •Future plans include magnetic flux

Upload: bishop

Post on 06-Jan-2016

25 views

Category:

Documents


2 download

DESCRIPTION

April 21, 2002 00:04:00. August 24, 2002 00:04:00. October 28, 2003 06:04:00. January 20, 2005 06:04:00. Relating Solar Source Magnetic Connectivity to SEP properties seen at 1 AU A.J. Coyner, D, Alexander, and M.I. Desai. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: April 21, 2002 00:04:00

Relating Solar Source Magnetic Connectivity to SEP properties seen at 1 AUA.J. Coyner, D, Alexander, and M.I. Desai

April 21, 2002 00:04:00

August 24, 2002 00:04:00

January 20, 2005 06:04:00

October 28, 2003 06:04:00

•We investigate the effects of solar magnetic configuration (determined with PFSS extrapolations) on observed (Fe/O) ratios for 42 events including January 20, 2005.

•Comparisons with Fe/O made at ULEIS energies (0.32-0.45 MeV/Nuc)

•January 20, 2005 specifically shows significant open field with the extrapolation.

•Less open field magnetic flux than the other campaign events with open field.

•We see correlations in the open field event data between Fe/O and open magnetic flux influenced by the high Fe/O ratio events

•Future plans include magnetic flux comparisons with ratios at SIS energies as well