中文
相关论文

相关论文: Extreme space weather events caused by super activ…

200 篇论文

We report on a study of all major solar eruptions that occurred on the front-side of the Sun during the rise to peak phase of cycle 24 (first 62 months) in order to understand the key factors affecting the occurrence of large solar…

太阳与恒星天体物理 · 物理学 2015-06-22 N. Gopalswamy , H. Xie , S. Akiyama , P. Makela , S. Yashiro

Solar eruptions generally refer to coronal mass ejections (CMEs) and flares. Both are important sources of space weather. Solar flares cause sudden change in the ionization level in the ionosphere. CMEs cause solar energetic particle (SEP)…

太阳与恒星天体物理 · 物理学 2017-09-12 Nat Gopalswamy

Severe geomagnetic storms appear to be ordered by the solar cycle in a number of ways. They occur more frequently close to solar maximum and declining phase, are more common in larger solar cycles and show different patterns of occurrence…

太阳与恒星天体物理 · 物理学 2022-08-31 Mathew Owens , Luke Barnard , Benjamin Pope , Mike Lockwood , Ilya Usoskin , Eleanna Asvestari

In this work, we examine the association between solar active regions and 152 solar flares, coronal mass ejections, and solar energetic particle (SEP) events over solar cycles 23-24 (1997-2017). The CDAW center's GOES data in the energy…

太阳与恒星天体物理 · 物理学 2025-04-21 Raj Kumar , Ramesh Chandra , Bimal Pande , Seema Pande

Ground level events (GLEs) occupy the high-energy end of gradual solar energetic particle (SEP) events. They are associated with coronal mass ejections (CMEs) and solar flares, but we still do not clearly understand the special conditions…

太阳与恒星天体物理 · 物理学 2015-06-04 N. V. Nitta , Y. Liu , M. L. DeRosa , R. W. Nightingale

Solar flares stronger than X10 (S-flares, >X10) are the highest class flares which significantly impact on the Sun's evolution and space weather. Based on observations of Geostationary Orbiting Environmental Satellites (GOES) at soft X-ray…

太阳与恒星天体物理 · 物理学 2025-01-10 Baolin Tan , Yin Zhang , Jing Huang , Kaifan Ji

Solar flares and coronal mass ejections (CMEs), especially the larger ones, emanate from active regions (ARs). With the aim to understand the magnetic properties that govern such flares and eruptions, we systematically survey all flare…

太阳与恒星天体物理 · 物理学 2017-01-11 Shin Toriumi , Carolus J. Schrijver , Louise K. Harra , Hugh Hudson , Kaori Nagashima

In this paper, we present the multi-wavelength study of a high level of solar activity during which a single active region produced multiple flares/CMEs. According to the sunspot observations, the current solar cycle 24 manifest to be less…

太阳与恒星天体物理 · 物理学 2020-12-10 Shirsh Lata Soni , Manohar Lal Yadav , Radhe Syam Gupta , Pyare lal Verma

The extreme solar and SEP event of 20 January 2005 is analyzed from two perspectives. Firstly, we study features of the main phase of the flare, when the strongest emissions from microwaves up to 200 MeV gamma-rays were observed. Secondly,…

Solar flares are one of the most energetic events in the solar system, their impact on Earth at ground level and its atmosphere remains under study. The repercussions of this phenomenon in our technological infrastructure includes radio…

太阳与恒星天体物理 · 物理学 2018-08-29 V. De la Luz , E. P. Balanzario , T. Tsiftsi

We present an overview of the observed properties of the GLEs and those of the associated flares and CMEs. The solar eruptions are very intense involving X-class flares and extreme CME speeds (average ~2000 km/s). The active regions in…

太阳与恒星天体物理 · 物理学 2015-06-05 N. Gopalswamy , H. Xie , S. Yashiro , S. Akiyama , P. Mäkelä , I. G. Usoskin

Charged particles, generated in solar flares, sometimes can get extremely high energy, above the 500 MeV level, and produce abrupt ground level enhancements (GLEs) on the ground-based detectors of cosmic rays. The initial flares are strong…

太阳与恒星天体物理 · 物理学 2024-04-11 Regina A. Suleymanova , Leonty I. Miroshnichenko , Valentina I. Abramenko

NOAA Active Region (AR) 13664/8 produced the most intense geomagnetic effects since the ``Halloween'' event of 2003. The resulting extreme solar storm is believed to be the consequence of multiple interacting coronal mass ejections (CMEs).…

太阳与恒星天体物理 · 物理学 2024-12-04 Rui Wang , Ying D. Liu , Xiaowei Zhao , Huidong Hu

An interval of exceptional solar activity was registered in early September 2017, late in the decay phase of solar cycle 24, involving the complex Active Region 12673 as it rotated across the western hemisphere with respect to Earth. A…

空间物理 · 物理学 2019-07-16 A. Bruno , E. R. Christian , G. A. de Nolfo , I. G. Richardson , J. M. Ryan

Large solar flares and eruptions may influence remote regions through perturbations in the outer-atmospheric magnetic field, leading to causally related events outside of the primary or triggering eruptions that are referred to as…

太阳与恒星天体物理 · 物理学 2015-11-04 Carolus J. Schrijver , Paul A. Higgins

Sunspots or active regions (ARs) with a delta-magnetic configuration are known to be associated with strong eruptions such as flares and mass ejections. This article investigates the relationship between delta-ARs and flares over the course…

太阳与恒星天体物理 · 物理学 2025-10-28 Rohan E. Louis

We report on four large filament eruptions (FEs) from solar cycles 23 and 24 that were associated with large solar energetic particle (SEP) events and interplanetary type II radio bursts. The post-eruption arcades corresponded to mostly…

太阳与恒星天体物理 · 物理学 2015-06-11 N. Gopalswamy , P. Makela , S. Akiyama , S. Yashiro , H. Xie , N. Thakur , S. W. Kahler

The most powerful explosions on the Sun [...] drive the most severe space-weather storms. Proxy records of flare energies based on SEPs in principle may offer the longest time base to study infrequent large events. We conclude that one…

We study the solar sources of an intense geomagnetic storm of solar cycle 23 that occurred on 20 November 2003, based on ground- and space-based multiwavelength observations. The coronal mass ejections (CMEs) responsible for the above…

太阳与恒星天体物理 · 物理学 2015-05-28 Pankaj Kumar , P. K. Manoharan , Wahab Uddin

The sustained gamma ray emission (SGRE) from the Sun is one of the fascinating high energy phenomena closely related to the acceleration of protons to energies >300 MeV. Here we report on the solar cycle variation of SGRE events based on…

高能天体物理现象 · 物理学 2025-10-16 N. Gopalswamy , P. Mäkela , S. Akiyama , S. Yashiro , H. Xie
‹ 上一页 1 2 3 10 下一页 ›