[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 …
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 …
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 …
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
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 …
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 …
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 …
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
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 …
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 …
this flare/CME event is not related to only one single active region (AR). Activation and …
Observation of interactions and eruptions of two filaments
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 …
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
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 …
configurations have different contributions to short-term and long-term variations of the Sun …