Latitudinal Variation of High Fe Charge State Events

Details Latitudinal Variation of High Fe Charge State Events Latitudinal Variation of High Fe Charge State Events

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsh32a..05l&link_type=abstract

American Geophysical Union, Spring Meeting 2002, abstract #SH32A-05

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7513 Coronal Mass Ejections, 7536 Solar Activity Cycle (2162), 7537 Solar And Stellar Variability

Scientific paper

We present a comparative study of the frequency of high Fe charge state events as a function of latitude. It has been shown that high Fe charge states are observed to occur in the presence of Interplanetary Coronal Mass Ejections (ICMEs) at 1 AU. We compare Fe charge state data from the ACE spacecraft in the ecliptic plane with that from the Ulysses spacecraft spanning a range of latitudes. This study encompasses the ascending phase of Solar Cycle 23, extending from 1998 - 2001. We find that the frequencies of high Fe charge state events at high and ecliptic latitudes become similar as solar maximum approaches.

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