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Solar proton events in solar cycle 23: long-term database and applications. / Yakovchouk, Olesya; Lazutin, Leonid; Logachev, Yurii; Vashenyuk, Eduard; Daibog, Elena; Miroshnichenko, Leonty; Nazarova, Margarita; Vitaly, Ishkov; Bazilevskaya, Galina; Petrenko, Inna; Stupishin, Alexey; Surova, Galina.

40th COSPAR Scientific Assembly. Том 40 2014. D2.5-56-14.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции

Harvard

Yakovchouk, O, Lazutin, L, Logachev, Y, Vashenyuk, E, Daibog, E, Miroshnichenko, L, Nazarova, M, Vitaly, I, Bazilevskaya, G, Petrenko, I, Stupishin, A & Surova, G 2014, Solar proton events in solar cycle 23: long-term database and applications. в 40th COSPAR Scientific Assembly. Том. 40, D2.5-56-14, 40th COSPAR Scientific Assembly 2014, Москва, Российская Федерация, 2/08/14. <http://adsabs.harvard.edu/abs/2014cosp...40E3679Y>

APA

Yakovchouk, O., Lazutin, L., Logachev, Y., Vashenyuk, E., Daibog, E., Miroshnichenko, L., Nazarova, M., Vitaly, I., Bazilevskaya, G., Petrenko, I., Stupishin, A., & Surova, G. (2014). Solar proton events in solar cycle 23: long-term database and applications. в 40th COSPAR Scientific Assembly (Том 40). [D2.5-56-14] http://adsabs.harvard.edu/abs/2014cosp...40E3679Y

Vancouver

Yakovchouk O, Lazutin L, Logachev Y, Vashenyuk E, Daibog E, Miroshnichenko L и пр. Solar proton events in solar cycle 23: long-term database and applications. в 40th COSPAR Scientific Assembly. Том 40. 2014. D2.5-56-14

Author

Yakovchouk, Olesya ; Lazutin, Leonid ; Logachev, Yurii ; Vashenyuk, Eduard ; Daibog, Elena ; Miroshnichenko, Leonty ; Nazarova, Margarita ; Vitaly, Ishkov ; Bazilevskaya, Galina ; Petrenko, Inna ; Stupishin, Alexey ; Surova, Galina. / Solar proton events in solar cycle 23: long-term database and applications. 40th COSPAR Scientific Assembly. Том 40 2014.

BibTeX

@inproceedings{50423bc7679c4e779176d8686291cd78,
title = "Solar proton events in solar cycle 23: long-term database and applications",
abstract = "Investigation of solar active phenomena requires systematic data of solar cosmic ray outbursts, the identification of sources and study of their impacts on near-Earth space. The description of these phenomena changed and developed during space age according to instrumentation and understanding. Consequently the goal was to have a uniform catalogue of solar proton events covering various years. Initiated by Z. {\v S}vestka and P. Simon this data base exists for the years 1955-1996. The catalogue includes solar proton events with E ≥ 10 MeV flux exceeding 1 cm (-2) s (-1) sr (-1) near Earth. Enhancing this catalogue by solar cycle 23 we can now present a comparative analysis of solar activity in cycles 20-23 (period 1955-2009), including energy spectra characteristics of proton fluxes, their connection with X-rays and shock waves. For the first time a study of the maximum energy of the accelerated particles in individual solar proton events will be shown. We will describe the proposed method to determine the maximum energy and present a statistical analysis, based on source parameters and propagation conditions in the heliosphere.",
author = "Olesya Yakovchouk and Leonid Lazutin and Yurii Logachev and Eduard Vashenyuk and Elena Daibog and Leonty Miroshnichenko and Margarita Nazarova and Ishkov Vitaly and Galina Bazilevskaya and Inna Petrenko and Alexey Stupishin and Galina Surova",
year = "2014",
language = "English",
volume = "40",
booktitle = "40th COSPAR Scientific Assembly",
note = "40th COSPAR Scientific Assembly 2014 ; Conference date: 02-08-2014 Through 10-08-2014",
url = "https://www.cospar-assembly.org/",

}

RIS

TY - GEN

T1 - Solar proton events in solar cycle 23: long-term database and applications

AU - Yakovchouk, Olesya

AU - Lazutin, Leonid

AU - Logachev, Yurii

AU - Vashenyuk, Eduard

AU - Daibog, Elena

AU - Miroshnichenko, Leonty

AU - Nazarova, Margarita

AU - Vitaly, Ishkov

AU - Bazilevskaya, Galina

AU - Petrenko, Inna

AU - Stupishin, Alexey

AU - Surova, Galina

PY - 2014

Y1 - 2014

N2 - Investigation of solar active phenomena requires systematic data of solar cosmic ray outbursts, the identification of sources and study of their impacts on near-Earth space. The description of these phenomena changed and developed during space age according to instrumentation and understanding. Consequently the goal was to have a uniform catalogue of solar proton events covering various years. Initiated by Z. Švestka and P. Simon this data base exists for the years 1955-1996. The catalogue includes solar proton events with E ≥ 10 MeV flux exceeding 1 cm (-2) s (-1) sr (-1) near Earth. Enhancing this catalogue by solar cycle 23 we can now present a comparative analysis of solar activity in cycles 20-23 (period 1955-2009), including energy spectra characteristics of proton fluxes, their connection with X-rays and shock waves. For the first time a study of the maximum energy of the accelerated particles in individual solar proton events will be shown. We will describe the proposed method to determine the maximum energy and present a statistical analysis, based on source parameters and propagation conditions in the heliosphere.

AB - Investigation of solar active phenomena requires systematic data of solar cosmic ray outbursts, the identification of sources and study of their impacts on near-Earth space. The description of these phenomena changed and developed during space age according to instrumentation and understanding. Consequently the goal was to have a uniform catalogue of solar proton events covering various years. Initiated by Z. Švestka and P. Simon this data base exists for the years 1955-1996. The catalogue includes solar proton events with E ≥ 10 MeV flux exceeding 1 cm (-2) s (-1) sr (-1) near Earth. Enhancing this catalogue by solar cycle 23 we can now present a comparative analysis of solar activity in cycles 20-23 (period 1955-2009), including energy spectra characteristics of proton fluxes, their connection with X-rays and shock waves. For the first time a study of the maximum energy of the accelerated particles in individual solar proton events will be shown. We will describe the proposed method to determine the maximum energy and present a statistical analysis, based on source parameters and propagation conditions in the heliosphere.

M3 - Conference contribution

VL - 40

BT - 40th COSPAR Scientific Assembly

T2 - 40th COSPAR Scientific Assembly 2014

Y2 - 2 August 2014 through 10 August 2014

ER -

ID: 36387108