CaltechAUTHORS
  A Caltech Library Service

Fe Enhancements in SEP Onsets: Flare/CME Mixture or Transport Effect?

Mason, G. M. and Li, G. and Cohen, C. M. S. and Desai, M. I. and Haggerty, D. K. and Leske, R. A. and Mewaldt, R. A. and Zank, G. P. (2014) Fe Enhancements in SEP Onsets: Flare/CME Mixture or Transport Effect? In: Outstanding Problems in Heliophysics: From Coronal Heating to the Edge of the Heliosphere. ASP Conference Series. Vol.484. Astronomical Society of the Pacific , San Francisco, CA, pp. 137-143. https://resolver.caltech.edu/CaltechAUTHORS:20160624-090842763

[img] PDF - Published Version
See Usage Policy.

3446Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20160624-090842763

Abstract

During the onset phases of SEP events, the Fe/O ratio is often observed to be initially enhanced (~1) over typical SEP values, followed by a decline to values close to typical averages over entire events (Fe/O ~0.1). Two mechanisms have been suggested to explain this behavior, namely (1) a two-step process with an initial injection of “flare” particles with high Fe/O followed by shock-accelerated particles with lower Fe/O, and (2) a transport effect wherein the lower charge-to-mass ratio of Fe vs. O results in faster transport of Fe to the observer, leading to enhanced Fe/O in the early stages of the event. Distinguishing between these two scenarios is important to building a basic picture of processes taking place in large SEP events. We have carried out a detailed study of 17 large SEP events where energetic particle data were fitted by a state-of-the-art model whose computed time-intensity profiles were compared to the observed profiles of H, He, O, and Fe over a very broad energy range. We find that the observed decrease in Fe/O during the rise phase can be reasonably fitted by the transport model where the differences in Fe vs. O transport are due to the slope of the turbulence spectrum of the interplanetary magnetic field (IMF).


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/2014ASPC..484..137MADSArticle
http://aspbooks.org/a/volumes/article_details/?paper_id=36307PublisherArticle
ORCID:
AuthorORCID
Mason, G. M.0000-0003-2169-9618
Cohen, C. M. S.0000-0002-0978-8127
Mewaldt, R. A.0000-0003-2178-9111
Additional Information:© 2014 Astronomical Society of the Pacific. This work was supported by NASA under LWS TR&T grant NNX07-AP69G (APL), and other grants including NNX09AP74A (UAH), NNX08AI11-G (Caltech), and NNX08AK87G (SwRI) and NSF grants including AGS-1135432 (UAH) and ATM-0551127 (SwRI). Figure 1 is reproduced by permission of the AAS.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANNX07AP69G
NASANNX09AP74A
UAHNNX08A111G
NASANNX08AK87G
NSFAGS-1135432
NSFATM-0551127
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2014-01
Series Name:ASP Conference Series
Record Number:CaltechAUTHORS:20160624-090842763
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160624-090842763
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:68652
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:27 Jun 2016 22:25
Last Modified:22 Nov 2019 09:58

Repository Staff Only: item control page