The temporal and spatial development of MeV proton acceleration at interplanetary shocks

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The temporal and spatial development of MeV proton acceleration at interplanetary shocks. / Kallenrode, May Britt.
in: Journal of Geophysical Research A: Space Physics, Jahrgang 102, Nr. A10, 97JA01678, 01.10.1997, S. 22347-22363.

Publikation: Beiträge in ZeitschriftenZeitschriftenaufsätzeForschungbegutachtet

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@article{c258439cf77a46f198874ce19ed2654b,
title = "The temporal and spatial development of MeV proton acceleration at interplanetary shocks",
abstract = "Particle events observed in association with interplanetary shocks exhibit a wide variety of different features. In this paper we will demonstrate how these features can be understood in terms of a spatially and temporally varying shock efficiency and the subsequent interplanetary propagation. The examples presented here will show that while the location of the observer relative to the shock is an important factor in determining the event properties, the radial and temporal evolution of the shock also plays an important role. In particular, there are shocks which in a given energy range predominately accelerate particles close to the Sun, while in others the shock efficiency increases as they propagate outward. Another goal of this paper is to demonstrate that the black box model used here is able to fit the data. Copyright 1997 by the American Geophysical Union.",
keywords = "Engineering",
author = "Kallenrode, {May Britt}",
year = "1997",
month = oct,
day = "1",
doi = "10.1029/97JA01678",
language = "English",
volume = "102",
pages = "22347--22363",
journal = "Journal of Geophysical Research A: Space Physics",
issn = "0148-0227",
publisher = "Wiley-Blackwell Publishing, Inc.",
number = "A10",

}

RIS

TY - JOUR

T1 - The temporal and spatial development of MeV proton acceleration at interplanetary shocks

AU - Kallenrode, May Britt

PY - 1997/10/1

Y1 - 1997/10/1

N2 - Particle events observed in association with interplanetary shocks exhibit a wide variety of different features. In this paper we will demonstrate how these features can be understood in terms of a spatially and temporally varying shock efficiency and the subsequent interplanetary propagation. The examples presented here will show that while the location of the observer relative to the shock is an important factor in determining the event properties, the radial and temporal evolution of the shock also plays an important role. In particular, there are shocks which in a given energy range predominately accelerate particles close to the Sun, while in others the shock efficiency increases as they propagate outward. Another goal of this paper is to demonstrate that the black box model used here is able to fit the data. Copyright 1997 by the American Geophysical Union.

AB - Particle events observed in association with interplanetary shocks exhibit a wide variety of different features. In this paper we will demonstrate how these features can be understood in terms of a spatially and temporally varying shock efficiency and the subsequent interplanetary propagation. The examples presented here will show that while the location of the observer relative to the shock is an important factor in determining the event properties, the radial and temporal evolution of the shock also plays an important role. In particular, there are shocks which in a given energy range predominately accelerate particles close to the Sun, while in others the shock efficiency increases as they propagate outward. Another goal of this paper is to demonstrate that the black box model used here is able to fit the data. Copyright 1997 by the American Geophysical Union.

KW - Engineering

UR - http://www.scopus.com/inward/record.url?scp=37149031351&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/1288364d-3ea6-337e-95ea-31387d712e49/

U2 - 10.1029/97JA01678

DO - 10.1029/97JA01678

M3 - Journal articles

AN - SCOPUS:37149031351

VL - 102

SP - 22347

EP - 22363

JO - Journal of Geophysical Research A: Space Physics

JF - Journal of Geophysical Research A: Space Physics

SN - 0148-0227

IS - A10

M1 - 97JA01678

ER -

DOI