[图书][B] Plasma astrophysics, part II: reconnection and flares

BV Somov - 2012 - books.google.com
This two-part book is devoted to classic fundamentals and current practices and
perspectives of modern plasma astrophysics. This second part discusses the physics of …

Photospheric magnetic field properties of flaring versus flare-quiet active regions. II. Discriminant analysis

KD Leka, G Barnes - The Astrophysical Journal, 2003 - iopscience.iop.org
We apply statistical tests based on discriminant analysis to the wide range of photospheric
magnetic parameters described in a companion paper by Leka & Barnes, with the goal of …

Photospheric magnetic field properties of flaring versus flare-quiet active regions. I. Data, general approach, and sample results

KD Leka, G Barnes - The Astrophysical Journal, 2003 - iopscience.iop.org
Photospheric vector magnetic field data from the University of Hawai'i Imaging Vector
Magnetograph, with good spatial and temporal sampling, are used to study the question of …

Rapid change of δ spot structure associated with seven major flares

C Liu, N Deng, Y Liu, D Falconer… - The Astrophysical …, 2005 - iopscience.iop.org
A large fraction of major flares occur in active regions that exhibit a δ configuration. The
formation and disintegration of δ configurations is very important in understanding the …

[HTML][HTML] Conference note: a taxonomy of extended radio sources in clusters of galaxies

JC Kempner, EL Blanton, TE Clarke… - The riddle of cooling …, 2004 - adsabs.harvard.edu
At the request of the conference attendees, we have compiled a classification of extended
radio sources in clusters. These range from scales of tens of parsecs to over a megaparsec …

The magnetic field, horizontal motion and helicity in a fast emerging flux region which eventually forms a delta spot

J Liu, H Zhang - Solar Physics, 2006 - Springer
We studied the behavior of magnetic field, horizontal motion and helicity in a fast emerging
flux region NOAA 10488 which eventually forms a δ spot. It is found that the rotation of …

A quantitative study on magnetic configuration for active regions

J Guo, H Zhang, OV Chumak, Y Liu - Solar Physics, 2006 - Springer
As compared with the Mount Wilson Magnetic Classification (MWMC), effective distance (d
E) is a useful parameter because it gives a quantitative measure of magnetic configuration in …

Transequatorial filament eruption and its link to a coronal mass ejection

JX Wang, GP Zhou, YY Wen, YZ Zhang… - Chinese Journal of …, 2006 - iopscience.iop.org
Abstract We revisit the Bastille Day flare/CME Event of 2000 July 14, and demonstrate that
this flare/CME event is not related to only one single active region (AR). Activation and …

Observation of interactions and eruptions of two filaments

J Su, Y Liu, H Kurokawa, X Mao, S Yang, H Zhang… - Solar Physics, 2007 - Springer
We present new observations of the interactions of two close, but distinct, Hα filaments and
their successive eruptions on 5 November 1998. The magnetic fields of the filaments are …

Different contributions to space weather and space climate from different big solar active regions

J Jiang, Q Song, JX Wang, T Baranyi - The Astrophysical Journal, 2019 - iopscience.iop.org
The purpose of this paper is to show that large active regions (ARs) with different magnetic
configurations have different contributions to short-term and long-term variations of the Sun …