Pregled bibliografske jedinice broj: 757011
Cosmic Ray modulation by Corotating Interaction Regions
Cosmic Ray modulation by Corotating Interaction Regions // IHY-ISWI Regional Meeting - Heliophysical phenomena and Earth’s environment
Šibenik, Hrvatska, 2009. (poster, međunarodna recenzija, sažetak, ostalo)
CROSBI ID: 757011 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Cosmic Ray modulation by Corotating Interaction Regions
Autori
Čalogović, Jaša ; Vršnak, Bojan ; Temmer, Manuela
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, ostalo
Skup
IHY-ISWI Regional Meeting - Heliophysical phenomena and Earth’s environment
Mjesto i datum
Šibenik, Hrvatska, 07.09.2009. - 13.09.2009
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
cosmic rays; corotating interaction regions; CIR; coronal hole; solar wind
Sažetak
We analyzed the relationship between the ground-based modulation of cosmic rays (CR) and corotating interaction regions (CIRs). Daily averaged data from 8 different neutron monitor (NM) stations were used. The NM stations were selected to include all latitudes (3 NM stations in high, 3 in middle and 2 in low latitudes) and longitudes, covering rigidities from 0 to 12.91 GeV. In situ solar wind data (density n, speed v and magnetic field B) were taken from the Advanced Composition Explorer (ACE) database, whereas the coronal hole (CH) areas were extracted from the Solar X-Ray Imager (GOES-12). For the analysis we have chosen a period in the declining phase of solar cycle 23, covering days 25 – 125 of the year 2005 (25 January until 5 May), when the solar CME activity was particularly low. During the CIR periods CR decreased typically from 0.5 to 1%. The cross-correlation analysis showed a distinct anti-correlation between the magnetic field and CR, with correlation coefficient (r) ranging from -0.31 to -0.41 (mean: -0.37) and with the CR time delay of 2 to 3 days depending on NM station. Similar anti- correlations, but with the lower correlation coefficients, were found for the solar wind density and velocity characterized by the CR time lag of 4 and 1 day, respectively. The relationship was also established between the CR modulation and the area of the CIR-related CH. In this case the anti-correlation has r = -0.20 to -0.39 (mean: -0.29) for the CR time lag of 5 days after the central-meridian passage of CH.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Geodetski fakultet, Zagreb