What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes?

Keppler, E.

doi:https://doi.org/10.1007/s00585-998-1552-1

Articles | Volume 16, issue 12

https://doi.org/10.1007/s00585-998-1552-1

Articles | Volume 16, issue 12

31 Dec 1998

What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes?

E. Keppler

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Total article views: 1,258 (including HTML, PDF, and XML)

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PDF: 526
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BibTeX: 68
EndNote: 62

Views and downloads (calculated since 01 Feb 2013)

Month	HTML	PDF	XML	Total
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Mar 2013	5	0	5
Apr 2013	1	7	0	8
May 2013	1	6	0	7
Jun 2013	2	7	0	9
Jul 2013	2	7	0	9
Aug 2013	9	7	0	16
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Oct 2013	3	7	0	10
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Dec 2013	2	5	0	7
Jan 2014	5	0	5
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Oct 2015	8	1	0	9
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Dec 2015	2	1	0	3
Jan 2016	12	5	1	18
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Feb 2018	0
Mar 2018	4	1	0	5
Apr 2018	2	3	0	5
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Aug 2018	3	2	0	5
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Nov 2018	5	2	0	7
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Jan 2019	3	6	0	9
Feb 2019	3	1	0	4
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Apr 2019	3	3	0	6
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Apr 2023	0
May 2023	8	3	3	14
Jun 2023	3	3	0	6
Jul 2023	8	4	1	13
Aug 2023	4	3	1	8
Sep 2023	8	2	10
Oct 2023	7	5	0	12
Nov 2023	4	1	0	5
Dec 2023	5	4	0	9
Jan 2024	5	0	5
Feb 2024	2	2	1	5
Mar 2024	4	4	1	9
Apr 2024	7	2	6	15
May 2024	4	7	1	12
Jun 2024	4	1	1	6
Jul 2024	9	2	1	12
Aug 2024	4	4	1	9
Sep 2024	4	5	1	10
Oct 2024	5	2	0	7
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Dec 2024	4	0	4
Jan 2025	3	5	0	8
Feb 2025	6	4	0	10
Mar 2025	4	3	0	7
Apr 2025	5	9	0	14
May 2025	12	2	4	18
Jun 2025	23	12	0	35

Cumulative views and downloads (calculated since 01 Feb 2013)

Month	HTML	PDF	XML	Total
Feb 2013	6	0	6
Mar 2013	5	0	5
Apr 2013	1	7	0	8
May 2013	1	6	0	7
Jun 2013	2	7	0	9
Jul 2013	2	7	0	9
Aug 2013	9	7	0	16
Sep 2013	5	0	5
Oct 2013	3	7	0	10
Nov 2013	1	4	0	5
Dec 2013	2	5	0	7
Jan 2014	5	0	5
Feb 2014	1	8	0	9
Mar 2014	10	8	0	18
Apr 2014	4	0	4
May 2014	1	5	0	6
Jun 2014	5	0	5
Jul 2014	8	0	8
Aug 2014	1	7	0	8
Sep 2014	1	5	0	6
Oct 2014	1	4	0	5
Nov 2014	2	5	0	7
Dec 2014	6	0	6
Jan 2015	2	0	2
Feb 2015	1	2	1	4
Mar 2015	1	2	0	3
Apr 2015	5	1	0	6
May 2015	8	1	0	9
Jun 2015	24	2	0	26
Jul 2015	14	2	0	16
Aug 2015	5	4	0	9
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Mar 2016	7	2	0	9
Apr 2016	6	5	0	11
May 2016	5	1	0	6
Jun 2016	4	1	0	5
Jul 2016	3	0	3
Aug 2016	3	3	0	6
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Oct 2016	4	1	0	5
Nov 2016	2	0	2
Dec 2016	5	2	0	7
Jan 2017	2	2	0	4
Feb 2017	5	2	0	7
Mar 2017	5	0	5
Apr 2017	5	3	0	8
May 2017	10	1	0	11
Jun 2017	8	0	8
Jul 2017	9	1	0	10
Aug 2017	1	1	0	2
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Jan 2018	3	3	0	6
Feb 2018	0
Mar 2018	4	1	0	5
Apr 2018	2	3	0	5
May 2018	5	4	0	9
Jun 2018	2	2	0	4
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Jun 2019	4	8	0	12
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Jan 2020	8	1	1	10
Feb 2020	3	1	0	4
Mar 2020	4	7	0	11
Apr 2020	2	2	0	4
May 2020	3	4	0	7
Jun 2020	8	0	8
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Aug 2020	7	8	2	17
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Oct 2020	4	5	0	9
Nov 2020	1	7	0	8
Dec 2020	8	7	0	15
Jan 2021	10	4	0	14
Feb 2021	7	3	0	10
Mar 2021	6	1	0	7
Apr 2021	6	6	0	12
May 2021	4	4	0	8
Jun 2021	6	5	0	11
Jul 2021	7	8	0	15
Aug 2021	8	5	0	13
Sep 2021	11	7	0	18
Oct 2021	6	24	0	30
Nov 2021	2	21	0	23
Dec 2021	8	2	0	10
Jan 2022	8	5	0	13
Feb 2022	5	2	1	8
Mar 2022	9	4	0	13
Apr 2022	5	1	6
May 2022	2	4	1	7
Jun 2022	4	1	1	6
Jul 2022	3	1	0	4
Aug 2022	5	2	0	7
Sep 2022	5	2	0	7
Oct 2022	6	1	7
Nov 2022	4	4	0	8
Dec 2022	5	2	0	7
Jan 2023	5	4	0	9
Feb 2023	8	1	0	9
Mar 2023	10	0	10
Apr 2023	0
May 2023	8	3	3	14
Jun 2023	3	3	0	6
Jul 2023	8	4	1	13
Aug 2023	4	3	1	8
Sep 2023	8	2	10
Oct 2023	7	5	0	12
Nov 2023	4	1	0	5
Dec 2023	5	4	0	9
Jan 2024	5	0	5
Feb 2024	2	2	1	5
Mar 2024	4	4	1	9
Apr 2024	7	2	6	15
May 2024	4	7	1	12
Jun 2024	4	1	1	6
Jul 2024	9	2	1	12
Aug 2024	4	4	1	9
Sep 2024	4	5	1	10
Oct 2024	5	2	0	7
Nov 2024	3	2	1	6
Dec 2024	4	0	4
Jan 2025	3	5	0	8
Feb 2025	6	4	0	10
Mar 2025	4	3	0	7
Apr 2025	5	9	0	14
May 2025	12	2	4	18
Jun 2025	23	12	0	35

Cited

Latest update: 30 Jun 2025

What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes?

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