Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements

We analyzed 25 solar energetic particle events, with energies ∼ 1 − 100 MeV, observed with ERNE instrument onboard Solar and Heliospheric Observatory (SOHO) and found that all of the solar energetic particlse were associated with coronal mass ejections, observed with LASCO/SOHO. The observational da...

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Published in:Advances in Astronomy and Space Physics
Date:2011
Main Authors: Allawi, H., Al-Ramdhan, W., Al-Sawad, A.
Format: Article
Language:English
Published: Advances in astronomy and space physics 2011
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/118972
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements / H. Allawi, W. Al-Ramdhan, A. Al-Sawad // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 61-64. — Бібліогр.: 29 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-118972
record_format dspace
spelling Allawi, H.
Al-Ramdhan, W.
Al-Sawad, A.
2017-06-02T18:10:59Z
2017-06-02T18:10:59Z
2011
Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements / H. Allawi, W. Al-Ramdhan, A. Al-Sawad // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 61-64. — Бібліогр.: 29 назв. — англ.
987-966-439-367-3
https://nasplib.isofts.kiev.ua/handle/123456789/118972
We analyzed 25 solar energetic particle events, with energies ∼ 1 − 100 MeV, observed with ERNE instrument onboard Solar and Heliospheric Observatory (SOHO) and found that all of the solar energetic particlse were associated with coronal mass ejections, observed with LASCO/SOHO. The observational data suggests that the associated coronal mass ejections were located at lower heliocentric altitudes during the time of maximum intensity of the high energy protons than those during the time of maximum intensity of lower energy protons. This might indicate that the upper limit of maximum acceleration by the shock waves decreases earlier as we go higher in the proton energy level.
en
Advances in astronomy and space physics
Advances in Astronomy and Space Physics
Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
spellingShingle Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
Allawi, H.
Al-Ramdhan, W.
Al-Sawad, A.
title_short Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
title_full Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
title_fullStr Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
title_full_unstemmed Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements
title_sort observation of maximum injection upper limit for energetic proton events according to soho/erne measurements
author Allawi, H.
Al-Ramdhan, W.
Al-Sawad, A.
author_facet Allawi, H.
Al-Ramdhan, W.
Al-Sawad, A.
publishDate 2011
language English
container_title Advances in Astronomy and Space Physics
publisher Advances in astronomy and space physics
format Article
description We analyzed 25 solar energetic particle events, with energies ∼ 1 − 100 MeV, observed with ERNE instrument onboard Solar and Heliospheric Observatory (SOHO) and found that all of the solar energetic particlse were associated with coronal mass ejections, observed with LASCO/SOHO. The observational data suggests that the associated coronal mass ejections were located at lower heliocentric altitudes during the time of maximum intensity of the high energy protons than those during the time of maximum intensity of lower energy protons. This might indicate that the upper limit of maximum acceleration by the shock waves decreases earlier as we go higher in the proton energy level.
isbn 987-966-439-367-3
url https://nasplib.isofts.kiev.ua/handle/123456789/118972
citation_txt Observation of maximum injection upper limit for energetic proton events according to SOHO/ERNE measurements / H. Allawi, W. Al-Ramdhan, A. Al-Sawad // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 61-64. — Бібліогр.: 29 назв. — англ.
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AT alsawada observationofmaximuminjectionupperlimitforenergeticprotoneventsaccordingtosohoernemeasurements
first_indexed 2025-12-07T15:49:27Z
last_indexed 2025-12-07T15:49:27Z
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