Parameterization of galactic cosmic-ray fluxes during opposite polarity solar cycles for future space missions

C. Grimani; M. Fabi; N. Finetti; D. Tombolato

Parameterization of galactic cosmic-ray fluxes during opposite polarity solar cycles for future space missions

C. Grimani, M. Fabi, N. Finetti, D. Tombolato

Research output: Contribution to conference › Paper › peer-review

Abstract

Galactic cosmic-ray (GCR) long-term variations and short-term fluctuations affect observations on board long-lived space missions. We have developed a parameterization of proton and helium fluxes for various levels of solar modulation during opposite polarity periods on the basis of experimental data. In spite of a general agreement among different results on p, p, e⁺ and e^?, some contradictory clues have been found both at solar minimum and maximum during negative polarity periods (A<0). We illustrate the implications of the results of this work for and with missions like LISA (Laser Interferometer Space Antenna).

Original language	English
Pages	485-488
Number of pages	4
Publication status	Published - 1 Jan 2007
Externally published	Yes
Event	30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: 3 Jul 2007 → 11 Jul 2007

Conference

Conference	30th International Cosmic Ray Conference, ICRC 2007
Country/Territory	Mexico
City	Merida, Yucatan
Period	3/07/07 → 11/07/07

Cite this

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title = "Parameterization of galactic cosmic-ray fluxes during opposite polarity solar cycles for future space missions",

abstract = "Galactic cosmic-ray (GCR) long-term variations and short-term fluctuations affect observations on board long-lived space missions. We have developed a parameterization of proton and helium fluxes for various levels of solar modulation during opposite polarity periods on the basis of experimental data. In spite of a general agreement among different results on p, p, e+ and e?, some contradictory clues have been found both at solar minimum and maximum during negative polarity periods (A<0). We illustrate the implications of the results of this work for and with missions like LISA (Laser Interferometer Space Antenna).",

author = "C. Grimani and M. Fabi and N. Finetti and D. Tombolato",

year = "2007",

month = jan,

day = "1",

language = "English",

pages = "485--488",

note = "30th International Cosmic Ray Conference, ICRC 2007 ; Conference date: 03-07-2007 Through 11-07-2007",

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TY - CONF

T1 - Parameterization of galactic cosmic-ray fluxes during opposite polarity solar cycles for future space missions

AU - Grimani, C.

AU - Fabi, M.

AU - Finetti, N.

AU - Tombolato, D.

PY - 2007/1/1

Y1 - 2007/1/1

N2 - Galactic cosmic-ray (GCR) long-term variations and short-term fluctuations affect observations on board long-lived space missions. We have developed a parameterization of proton and helium fluxes for various levels of solar modulation during opposite polarity periods on the basis of experimental data. In spite of a general agreement among different results on p, p, e+ and e?, some contradictory clues have been found both at solar minimum and maximum during negative polarity periods (A<0). We illustrate the implications of the results of this work for and with missions like LISA (Laser Interferometer Space Antenna).

AB - Galactic cosmic-ray (GCR) long-term variations and short-term fluctuations affect observations on board long-lived space missions. We have developed a parameterization of proton and helium fluxes for various levels of solar modulation during opposite polarity periods on the basis of experimental data. In spite of a general agreement among different results on p, p, e+ and e?, some contradictory clues have been found both at solar minimum and maximum during negative polarity periods (A<0). We illustrate the implications of the results of this work for and with missions like LISA (Laser Interferometer Space Antenna).

M3 - Paper

AN - SCOPUS:84899500009

SP - 485

EP - 488

T2 - 30th International Cosmic Ray Conference, ICRC 2007

Y2 - 3 July 2007 through 11 July 2007

ER -

Parameterization of galactic cosmic-ray fluxes during opposite polarity solar cycles for future space missions

Abstract

Conference

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