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A recent study has suggested a link between the surface level diurnal temperature range (DTR) and variations in the cosmic ray (CR) flux. As the DTR is an effective proxy for cloud cover, this result supports the notion that widespread…

Atmospheric and Oceanic Physics · Physics 2012-12-14 Benjamin A. Laken , Jasa Čalogović , Tariq Shahbaz , Enric Pallé

Forbush decreases (Fd) are transient, short-term reductions in the intensity of galactic cosmic rays that reach the Earth's surface. When this reduction is observed at multiple locations at the same time, it is referred to as simultaneous…

We present the results of an investigation of the relation between space-weather parameters and cosmic ray (CR) intensity modulation using algorithm-selected Forbush decreases (FDs) from Moscow (MOSC) and Apatity (APTY) neutron monitor (NM)…

Solar and Stellar Astrophysics · Physics 2022-01-05 Jibrin A. Alhassan , Ogbonnaya Okike , Augustine E. Chukwude

The abrupt aperiodic modulation of cosmic ray (CR) flux intensity, often referred to as Forbush decrease (FD), plays a significant role in our understanding of the Sun-Earth electrodynamics. Accurate and precise determination of FD…

Solar and Stellar Astrophysics · Physics 2022-05-11 Jibrin Adejoh Alhassan , Ogbonnaya Okike , Augustine Ejikeme Chukwude

Following on previous work by others, which gave evidence for few-day changes in the European Diurnal Temperature Range (DTR) apparently correlated with Cosmic Ray Forbush Decreases, we have made an independent study. We find no positive…

Atmospheric and Oceanic Physics · Physics 2012-12-13 Anatoly D. Erlykin , Arnold W. Wolfendale

The Forbush Decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections (CMEs) or high-speed streams from coronal holes. It has been mainly explored with ground-based…

High Energy Astrophysical Phenomena · Physics 2021-11-03 Francesca Alemanno , Qi An , Philipp Azzarello , Felicia Carla Tiziana Barbato , Paolo Bernardini , XiaoJun Bi , MingSheng Cai , Elisabetta Casilli , Enrico Catanzani , Jin Chang , DengYi Chen , JunLing Chen , ZhanFang Chen , MingYang Cui , TianShu Cui , YuXing Cui , HaoTing Dai , Antonio De Benedittis , Ivan De Mitri , Francesco de Palma , Maksym Deliyergiyev , Margherita Di Santo , Qi Ding , TieKuang Dong , ZhenXing Dong , Giacinto Donvito , David Droz , JingLai Duan , KaiKai Duan , Domenico D'Urso , RuiRui Fan , YiZhong Fan , Fang Fang , Kun Fang , ChangQing Feng , Lei Feng , Piergiorgio Fusco , Min Gao , Fabio Gargano , Ke Gong , YiZhong Gong , DongYa Guo , JianHua Guo , ShuangXue Han , YiMing Hu , GuangShun Huang , XiaoYuan Huang , YongYi Huang , Maria Ionica , Wei Jiang , Jie Kong , Andrii Kotenko , Dimitrios Kyratzis , . Li , ShiJun Lei , WenHao Li , WeiLiang Li , Xiang Li , XianQiang Li , YaoMing Liang , ChengMing Liu , Hao Liu , Jie Liu , ShuBin Liu , Yang Liu , Francesco Loparco , ChuanNing Luo , Miao Ma , PengXiong Ma , Tao Ma , XiaoYong Ma , Giovanni Marsella , Mario Nicola Mazziotta , Dan Mo , XiaoYang Niu , Xu Pan , Andrea Parenti , WenXi Peng , XiaoYan Peng , Chiara Perrina , Rui Qiao , JiaNing Rao , Arshia Ruina , MariaMunoz Salinas , Zhi Shangguan , WeiHua Shen , ZhaoQiang Shen , ZhongTao Shen , Leandro Silveri , JingXing Song , Mikhail Stolpovskiy , Hong Su , Meng Su , HaoRan Sun , ZhiYu Sun , Antonio Surdo , XueJian Teng , Andrii Tykhonov , JinZhou Wang , LianGuo Wang , Shen Wang , ShuXin Wang , XiaoLian Wang , Ying Wang , YanFang Wang , YuanZhu Wang , DaMing Wei , JiaJu Wei , YiFeng Wei , Di Wu , Jian Wu , LiBo Wu , Sha Sha Wu , Xin Wu , ZiQing Xia , EnHeng Xu , HaiTao Xu , ZhiHui Xu , ZunLei Xu , GuoFeng Xue , ZiZong Xu , HaiBo Yang , Peng Yang , YaQing Yang , Hui Jun Yao , YuHong Yu , GuanWen Yuan , Qiang Yuan , Chuan Yue , JingJing Zang , ShengXia Zhang , WenZhang Zhang , Yan Zhang , Yi Zhang , YongJie Zhang , YunLong Zhang , YaPeng Zhang , YongQiang Zhang , ZhiYong Zhang , Zhe Zhang , Cong Zhao , HongYun Zhao , XunFeng Zhao , ChangYi Zhou , Yan Zhu , Wei Chen , Li Feng , Xi Luo , ChengRui Zhu

Despite over 35 years of constant satellite-based measurements of cloud, reliable evidence of a long-hypothesized link between changes in solar activity and Earth's cloud cover remains elusive. This work examines evidence of a cosmic ray…

Atmospheric and Oceanic Physics · Physics 2012-11-26 Benjamin A. Laken , Enric Palle , Jasa Calogovic , Eimear M. Dunne

The Galactic cosmic ray (GCR) intensity has been postulated by others to vary cyclically with a peak to valley ratio of ~3:1, as the Solar System moves from the Spiral Arm to the Inter-Arm regions of the Galaxy. These intensities have been…

Solar and Stellar Astrophysics · Physics 2015-06-15 T. Sloan , A. W. Wolfendale

It has been claimed by others that observed temporal correlations of terrestrial cloud cover with `the cosmic ray intensity' are causal. The possibility arises, therefore, of a connection between cosmic rays and Global Warming. If true, the…

Astrophysics · Physics 2007-07-11 T. Sloan , A W Wolfendale

Forbush decrease (FD), discovered by Scott E. Forbush about 80 years ago, is reffered to as the non-repetitive short-term depression in galactic cosmic ray (GCR) flux, presumed to be associated with large-scale perturbations in solar wind…

Space Physics · Physics 2021-11-17 Jibrin A. Alhassan. , Ogbonnaya Okike , Augustine E. Chukwude

Recent satellite data have revealed a surprising correlation between galactic cosmic ray (GCR) intensity and the fraction of the Earth covered by clouds. If this correlation were to be established by a causal mechanism, it could provide a…

Atmospheric and Oceanic Physics · Physics 2012-08-27 The Cloud Collaboration

The short-term rapid CR flux depressions, generally referred to as Forbush decreases (FDs), are the most spectacular time-intensity CR variation. The need for analytical transformation of the observational CR time series data, to account…

Instrumentation and Methods for Astrophysics · Physics 2024-06-11 O. Okike , J. A. Alhassan , I. O. Eya

The Forbush decrease (FD) of cosmic rays is an important probe of the interplanetary environment disturbed by solar activities. In this work, we study the properties of 8 FDs electrons (including positrons) between 2 GeV and 20 GeV from…

High Energy Astrophysical Phenomena · Physics 2026-03-17 F. Alemanno , Q. An , P. Azzarello , F. C. T. Barbato , P. Bernardini , X. J. Bi , H. Boutin , I. Cagnoli , M. S. Cai , E. Casilli , J. Chang , D. Y. Chen , J. L. Chen , Z. F. Chen , Z. X. Chen , P. Coppin , M. Y. Cui , T. S. Cui , I. De Mitri , F. de Palma , A. Di Giovanni , T. K. Dong , Z. X. Dong , G. Donvito , J. L. Duan , K. K. Duan , R. R. Fan , Y. Z. Fan , F. Fang , K. Fang , C. Q. Feng , L. Feng , S. Fogliacco , J. M. Frieden , P. Fusco , M. Gao , F. Gargano , E. Ghose , K. Gong , Y. Z. Gong , D. Y. Guo , J. H. Guo , S. X. Han , Y. M. Hu , G. S. Huang , X. Y. Huang , Y. Y. Huang , M. Ionica , L. Y. Jiang , W. Jiang , Y. Z. Jiang , J. Kong , A. Kotenko , D. Kyratzis , S. J. Lei , B. Li , M. B. Li , W. H. Li , W. L. Li , X. Li , X. Q. Li , Y. M. Liang , C. M. Liu , H. Liu , J. Liu , S. B. Liu , Y. Liu , F. Loparco , M. Ma , P. X. Ma , T. Ma , X. Y. Ma , G. Marsella , M. N. Mazziotta , D. Mo , Y. Nie , X. Y. Niu , A. Parenti , W. X. Peng , X. Y. Peng , C. Perrina , E. Putti-Garcia , R. Qiao , J. N. Rao , Y. Rong , R. Sarkar , P. Savina , A. Serpolla , Z. Shangguan , W. H. Shen , Z. Q. Shen , Z. T. Shen , L. Silveri , J. X. Song , M. Stolpovskiy , H. Su , M. Su , H. R. Sun , Z. Y. Sun , A. Surdo , X. J. Teng , A. Tykhonov , G. F. Wang , J. Z. Wang , L. G. Wang , S. Wang , X. L. Wang , Y. F. Wang , D. M. Wei , J. J. Wei , Y. F. Wei , D. Wu , J. Wu , S. S. Wu , X. Wu , Z. Q. Xia , Z. Xiong , E. H. Xu , H. T. Xu , J. Xu , Z. H. Xu , Z. L. Xu , Z. Z. Xu , G. F. Xue , M. Y. Yan , H. B. Yang , P. Yang , Y. Q. Yang , H. J. Yao , Y. H. Yu , Q. Yuan , C. Yue , J. J. Zang , S. X. Zhang , W. Z. Zhang , Yan Zhang , Yi Zhang , Y. J. Zhang , Y. L. Zhang , Y. P. Zhang , Y. Q. Zhang , Z. Zhang , Z. Y. Zhang , C. Zhao , H. Y. Zhao , X. F. Zhao , C. Y. Zhou , X. Zhu , Y. Zhu , X. Luo

Forbush decreases (FDs) are depletions in the galactic cosmic ray (GCR) count rate that last typically for about a week and can be caused by coronal mass ejections (CMEs) or corotating interacting regions (CIRs). Fast CMEs that drive shocks…

Space Physics · Physics 2020-02-24 Anamarija Kirin , Bojan Vršnak , Mateja Dumbović , Bernd Heber

We examine the results linking cosmic ray flux (CRF) variations to global climate change. We then proceed to study various periods over which there are estimates for the radiative forcing, temperature change and CRF variations relative to…

Atmospheric and Oceanic Physics · Physics 2015-06-26 Nir J. Shaviv

The modulation of galactic cosmic rays (GCRs) by interplanetary disturbances, manifested as Forbush decreases (FDs), has long been recognized as a signature of coronal mass ejection (CME) passages through the heliosphere. While individual…

Solar and Stellar Astrophysics · Physics 2026-02-05 Haoyang Li , Zongyuan Ge , Zhaoming Wang

This paper presents the global analysis of two extended decreases of the galactic cosmic ray intensity observed by world-wide networks of ground-based detectors in 2012. This analysis is capable of separately deriving the cosmic ray density…

Various aspects of the connection between cloud cover (CC) and cosmic rays (CR) are analysed. Many features of this connection indicate that there is no direct causal connection between low cloud cover (LCC) and CR in spite of the evident…

Earth and Planetary Astrophysics · Physics 2015-05-13 A. D. Erlykin , G. Gyalai , K. Kudela , T. Sloan , A. W. Wolfendale

Aims. Forbush decrease (FD) is a transient decrease followed by a gradual recovery in the observed galactic cosmic ray intensity. We seek to understand the relationship between the FDs and near-Earth interplanetary magnetic field (IMF)…

Solar and Stellar Astrophysics · Physics 2015-07-29 K. P. Arunbabu , H. M. Antia , S. R. Dugad , S. K. Gupta , Y. Hayashi , S. Kawakami , P. K. Mohanty , A. Oshima , P. Subramanian

We analyze solar, geomagnetic and cosmic ray flux data along with rainfall and temperature data for almost five solar cycles. We provide evidence of significant influence of solar variability on climate. Specifically, we demonstrate…

Atmospheric and Oceanic Physics · Physics 2013-12-03 Badruddin , O. P. M. Aslam , M. Singh
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