نتایج جستجو برای: solar cosmic ray particle

تعداد نتایج: 600674  

2007
REKHA AGARWAL MISHRA RAJESH K. MISHRA RAVI KATARE

There are two types of high-speed solar wind streams classified in two categories: coronal hole associated and flare generated streams. These two types of streams are classified in two categories base on magnetic field and solar wind plasma parameters. We studied the dependence of cosmic ray depressions due to high-speed solar wind streams during low amplitude days. Cosmic ray intensity data wa...

2010
J. M. Ryan G. A. de Nolfo P. Evenson J. R. Jokipii C. Lopate D. Ruffolo M. Shea D. Smart C. Steigies

EXECUTIVE SUMMARY The global network of ground based neutron monitors and muon telescopes constitutes a unique “instrument” in an armada of particle detection and measurement facilities now in space and to be deployed in the future. This network has a particle energy detection threshold of order 500 MeV, extending up to 50 GeV, with a full-sky field of view continuously making dozens of pointed...

2003
V. Florinski J. R. Jokipii E. C. Stone A. C. Cummings G. P. Zank

The two Voyager spacecraft provide valuable information about the energetic particle population near the termination shock (TS), such as the anomalous cosmic ray (ACR) spectra, the intensity gradients, and the radial diffusion coefficients obtained from anisotropy measurements. While the spectra and gradients have been modeled successfully using the test-particle approach, the shock modificatio...

Journal: :Physical review letters 2013
O Adriani G C Barbarino G A Bazilevskaya R Bellotti A Bianco M Boezio E A Bogomolov M Bongi V Bonvicini S Bottai A Bruno F Cafagna D Campana R Carbone P Carlson M Casolino G Castellini C De Donato C De Santis N De Simone V Di Felice V Formato A M Galper A V Karelin S V Koldashov S A Koldobskiy S Y Krutkov A N Kvashnin A Leonov V Malakhov L Marcelli M Martucci A G Mayorov W Menn M Mergé V V Mikhailov E Mocchiutti A Monaco N Mori R Munini G Osteria F Palma P Papini M Pearce P Picozza C Pizzolotto M Ricci S B Ricciarini L Rossetto R Sarkar V Scotti M Simon R Sparvoli P Spillantini S J Stochaj J C Stockton Y I Stozhkov A Vacchi E Vannuccini G I Vasilyev S A Voronov Y T Yurkin G Zampa N Zampa V G Zverev

Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray positron flux and fraction that extends previously published measurements up to 300 GeV in kinetic energy. The ...

2003
S. A. Starodubtsev I. G. Usoskin

We study the temporal behavior of the power spectra for Galactic cosmic-ray fluctuations during the last two solar cycles. We use the 5-min data for 1980–2002 corrected for the barometric effect from two widely separated high-latitude cosmic-ray stations, Tixie Bay and Oulu. The cosmicray fluctuation spectrum is shown to be subjected to a regular long-term modulation with a period of about 11 y...

Solar flare events of high importance were utilised to study solar latitudinal frequency distribution of the solar flares in northern and southern hemisphere for the solar cycle 22 to recent solar cycle 23. A statistical analysis was performed to obtain their relationship with sudden storm commencement (SSCs) and Forbush decrease events (Fd) of cosmic ray intensity. An 11-year cyclic variation ...

2003
Paul Evenson

Time variations in the flux of galactic cosmic rays are the result of changing conditions in the solar wind. Maximum cosmic ray fluxes, which occur when solar activity is at a minimum, are well defined. Reductions from this maximum level are typically systematic and predictable but on occasion are rapid and unexpected. Models relating the flux level at lower energy to tha t at neutron monitor e...

1998
Henrik Svensmark

During the last solar cycle Earth’s cloud cover underwent a modulation more closely in phase with the galactic cosmic ray flux than with other solar activity parameters. Further it is found that Earth’s temperature follows more closely decade variations in galactic cosmic ray flux and solar cycle length, than other solar activity parameters. The main conclusion is that the average state of the ...

2004
Diego Casadei

The Alpha Magnetic Spectrometer (AMS) is a cosmic ray (CR) experiment that will operate on the International Space Station for three years, measuring the particle spectra in the rigidity range from 0.2 GV to 2 TV. The AMS-02 detector will provide measurements with unprecedented statistics of the hadronic and leptonic cosmic rays, allowing for a better study of the Earth magnetosphere through th...

Journal: :Radiation protection dosimetry 2002
S Roesler W Heinrich H Schraube

Energy spectra of secondary cosmic rays are calculated for aircraft altitudes and a discrete set of solar modulation parameters and rigidity cut-off values covering all possible conditions. The calculations are based on the Monte Carlo code FLUKA and on the most recent information on the interstellar cosmic ray flux including a detailed model of solar modulation. Results are compared to a large...

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