Quasi-periodicities in cosmic rays and time lag with the solar activity at a middle latitude neutron monitor: 1982-2017

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F18%3A00497094" target="_blank" >RIV/61389005:_____/18:00497094 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1007/s10509-018-3467-y" target="_blank" >http://dx.doi.org/10.1007/s10509-018-3467-y</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1007/s10509-018-3467-y" target="_blank" >10.1007/s10509-018-3467-y</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Quasi-periodicities in cosmic rays and time lag with the solar activity at a middle latitude neutron monitor: 1982-2017

Popis výsledku v původním jazyce

Galactic cosmic rays (GCRs) after entering the heliosphere are continuously modulated by the change in solar wind and the associated heliosphericmagnetic field. GCRs also follow about 11 year sunspot cycle in an inverse way with some time lag of few months to years, which usually varies from cycle to cycle Badruddin etal. 2007, Kane 2014, Aslam and Badruddin 2015 (e.g. Badruddin et al. in Astron. Astrophys. 466(2):697-704, 2007, Kane in Sol. Phys. 289:2669-2675, 2014, Aslam and Badruddin in Sol. Phys. 290:2333, 2015). In this work, we have investigated solar modulation of GCRs measured at three mid cut-off rigidity neutron monitor stations for the period of 1982 to 2017, covering two complete solar cycles and a major part of the recent cycle24. We study the time lag between GCRs intensity and various solar, geomagnetic and interplanetary parameters separately during the solar cycles under investigation. Further, we have investigated the presence and temporal evolution of mid term quasi-periodicities of GCRs time series during the above mentioned phases utilizing both Morlet wavelet transform and Scargle periodogram technique. Power spectral analysis indicates the presence of several mid term quasi-periodicities including Rieger type and Quasi-biennial oscillations. We discuss the findings and compare them with results of other authors.

Název v anglickém jazyce

Quasi-periodicities in cosmic rays and time lag with the solar activity at a middle latitude neutron monitor: 1982-2017

Popis výsledku anglicky

Galactic cosmic rays (GCRs) after entering the heliosphere are continuously modulated by the change in solar wind and the associated heliosphericmagnetic field. GCRs also follow about 11 year sunspot cycle in an inverse way with some time lag of few months to years, which usually varies from cycle to cycle Badruddin etal. 2007, Kane 2014, Aslam and Badruddin 2015 (e.g. Badruddin et al. in Astron. Astrophys. 466(2):697-704, 2007, Kane in Sol. Phys. 289:2669-2675, 2014, Aslam and Badruddin in Sol. Phys. 290:2333, 2015). In this work, we have investigated solar modulation of GCRs measured at three mid cut-off rigidity neutron monitor stations for the period of 1982 to 2017, covering two complete solar cycles and a major part of the recent cycle24. We study the time lag between GCRs intensity and various solar, geomagnetic and interplanetary parameters separately during the solar cycles under investigation. Further, we have investigated the presence and temporal evolution of mid term quasi-periodicities of GCRs time series during the above mentioned phases utilizing both Morlet wavelet transform and Scargle periodogram technique. Power spectral analysis indicates the presence of several mid term quasi-periodicities including Rieger type and Quasi-biennial oscillations. We discuss the findings and compare them with results of other authors.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/EF15_003%2F0000481" target="_blank" >EF15_003/0000481: Centrum výzkumu kosmického záření a radiačních jevů v atmosféře</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2018

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Astrophysics and Space Science

ISSN

0004-640X

e-ISSN

—

Svazek periodika

363

Číslo periodika v rámci svazku

12

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

17

Strana od-do

—

Kód UT WoS článku

000450075200001

EID výsledku v databázi Scopus

2-s2.0-85056430479