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1. SEP 2004 MODEL BY NYMMIK R.A
Home page: http://srd.sinp.msu.ru/nymmik/ . E-mail nymmik@sinp.msu.ru . ISO TS15391 Memorandum, October 2004 . ISO TS15391, version 2004, October . Report on the ISO WG4 meeting 24.05.2004 . Replies to comment from . G. Bazilevskaya - 1 , 2 . B. Quaghebeur - 1 , 2 . A. Hilgers - . MODEL PARAMETERS (PROTONS) . fluence peak flux . From date year-month (later then 1950-1) . - . To date year-month (before 2008-1) . - . Probability (from 0.01 to 0.9) . table . plot .
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Ссылки http://srd.sinp.msu.ru/nymmik/models/sep.php -- 3.8 Кб -- 01.10.2012
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2. Rikho Nymmik
... 1998 1 : Defended the Doctorate Degree Thesis on "Models of Cosmic Ray Particle Fluxes (Development and Applications)". ... Space Weather . ... Nymmik R.A., Radiation Environment Induced by Cosmic Ray Particle Fluxes in International Space Station Orbit According to Recent Solar and Galactic Cosmic Ray Models, Adv. ... Nymmik R.A., Radiation Environment Induced by Cosmic Ray Particle Fluxes in International Space Station Orbit According to Recent Solar and Galactic Cosmic Ray Models, Adv.Space Res. ...
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Ссылки http://srd.sinp.msu.ru/nymmik/ -- 146.8 Кб -- 12.01.2009
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3. http://srd.sinp.msu.ru/nymmik/models/ISOTS04.pdf
________________________________________________ Space Environment (Natural and Artifical) Probabilistic model for fluences and peak fluxes of solar energetic particles Part I Protons Technical Specification ___________________________________________________________ ... Proton energy ґ [MeV]. ... Differential proton fluence energy (E) distribution in a single SEP event (or in a set of SEP events) [proton/(cm2ЇMeV)]. ... Probability for a given peak flux SEP with energy E to be exceeded. ...
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Ссылки http://srd.sinp.msu.ru/nymmik/models/ISOTS04.pdf -- 231.8 Кб -- 26.01.2007
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4. http://srd.sinp.msu.ru/nymmik/models/hilgers.pdf
... GOES corrected results are wrong, because the publication Smart D.F. and M.A. Shea, Comment on the use of GOES solar proton data and spectra in solar dose calculations, Radiation Measurements 30 (1999) 327-335 was erroneous (see "The issues...." above. ... The criticism of the use of the log-normal distribution for the data fit in Feynman et al. is excessive. Indeed, Feynman et al. use only the high intensity part for the fit making the results almost independent of the low energy part. ...
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Ссылки http://srd.sinp.msu.ru/nymmik/models/hilgers.pdf -- 112.6 Кб -- 26.01.2007
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5. http://srd.sinp.msu.ru/nymmik/models/MEMO2004.pdf
INTERNATIONAL STANDARD ISO TS 15391 Technical specification Version 2004 October ______________________________________________________________ Space Environment (Natural and Artificial) Probabilistic model for fluences and peak fluxes of solar energetic particles Part I Protons Memorandum Reference No. ISO 15391 SPACE ENVIRONMENT (NATURAL AND ARTIFICIAL) Probabilistic model for fluences and peak fluxes of solar energetic particles: Part I - protons 1 Memorandum-2004 (October) (Memorandum is compiled by
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Ссылки http://srd.sinp.msu.ru/nymmik/models/MEMO2004.pdf -- 1418.9 Кб -- 26.01.2007
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6. http://srd.sinp.msu.ru/nymmik/models/bazilevskaya_1.pdf
Reply to the Dr. Bazilevskaya refrees report (comments on Memorandum No 1 Comment Implicitly, the Model states that the proton event with the peak flux f30 = 0.12 proton/(cm2s sr) has, in average, the fluence F30 = 105 proton/cm2. ... We have shown, that besides the one GLE event, analyzed by Smart and Shea, rest 12 GLE events in 1989-1991 demonstrated, that uncorrected GOES high-energy data are rather overestimated, than on the contrary. ... Is it a first attempt to estimate the SEP model exactness. ...
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Ссылки http://srd.sinp.msu.ru/nymmik/models/bazilevskaya_1.pdf -- 135.0 Кб -- 26.01.2007
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7. http://srd.sinp.msu.ru/nymmik/models/bazilevskaya_2.pdf
... Annex (e.g. 3.1) (3) Paragraph/ Figure/Table/ Note (e.g. Table 1) 4 Type of comment2 5 Comment (justification for change) by the MB Date: (6) Document: (7) Secretariat observations on each comment submitted Proposed change by the MB RU RU RU RU 2 2 2 2 Row 2 Row 4 Row 4 Row 5 ed ed ed te SEPs are not fluxes , but particles It is desirable to add that Wolf number is also known as the sunspot number. ... CLOSED: Accepted and implemented in modified form CLOSED: Accepted and RU 2 Row 16 . ...
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Ссылки http://srd.sinp.msu.ru/nymmik/models/bazilevskaya_2.pdf -- 142.9 Кб -- 26.01.2007
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8. http://srd.sinp.msu.ru/nymmik/models/quaghebeur_1.pdf
... Also, if events can be split up into distinct but overlapping events, how do you approximate the fluences of the individual events? ... In any cases, You can observe new increasing the E>30 MeV fluxes after first event. ... And for that case, what should be difference in fluences, predicted by different models. ... Fig. ... For different SEP model characteristics were used different events sets. 183 were physical events, what were used for development of the regularities, inherent to the SEP events....
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Ссылки http://srd.sinp.msu.ru/nymmik/models/quaghebeur_1.pdf -- 115.9 Кб -- 26.01.2007
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9. http://srd.sinp.msu.ru/nymmik/models/quaghebeur_2.pdf
... Notation of symbols used; Bold, italic, roman... 3 te 1 MB = Member body (enter the ISO 3166 two-letter country code, e.g. CN for China; comments from the ISO/CS editing unit are identified by **) 2 Type of comment: ge = general te = technical ed = editorial NOTE Columns 1, 2, 4, 5 are compulsory. page 1 of 5 ISO electronic balloting commenting template/version 2001-10 Template for comments and secretariat observations 1 MB1 2 Clause No./ ... CLOSED: Not accepted BE Be 4.2.2 ed Corrected to "events"...
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Ссылки http://srd.sinp.msu.ru/nymmik/models/quaghebeur_2.pdf -- 168.9 Кб -- 26.01.2007
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10. http://srd.sinp.msu.ru/nymmik/sep2001/Makefile
gostsep: GOSTSEP.FOR f77 GOSTSEP.FOR -o gostsep
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Ссылки http://srd.sinp.msu.ru/nymmik/sep2001/Makefile -- 1.0 Кб -- 26.01.2007
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