Flare SOL2012-07-06: on the origin of the circular polarization reversal between 17 GHz and 34 GHz
by Altyntsev et al.*
http://cesra.net/?p=1578<HTTP://cesra.net/?p=1578>
Observations of a radio-quiet solar preflare
by A. Benz et al.*
http://cesra.net/?p=1562<HTTP://cesra.net/?p=1562>
Predicting Flares and Solar Energetic Particle Events: The FORSPEF Tool
by A. Anastasiadis et al.*
http://cesra.net/?p=1551<HTTP://cesra.net/?p=1551>
——————
CESRA publishes Highlights of Solar Radio Physics aka CESRA Nuggets approximately every two weeks. These short communications are written in the language accessible to a non-expert in the specific area and designed to keep solar and heliophysics communities informed and up-to-date about current research. The highlights can be followed, discussed, commented and shared via https://www.facebook.com/solarcesra/ and https://twitter.com/CESRA_community
[University of Glasgow: The Times Scottish University of the Year 2018]
No. 309, “Electron Scattering in the Flaring Corona,” by Sophie Musset: Diffusive transport may contribute to the trapping of energetic electrons in coronal hard X-ray sources.
No. 310, “Valderrama in the 21st Century,” by Hugh Hudson: A newly-describd white-light flare from the 19th century, chronologically the third-ever observed flare.
See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets listing the current series, 2008-present, and http://sprg.ssl.berkeley.edu/~tohban/nuggets/forthe original series, 2005-2008. We publish these at roughly two-week intervals and welcome contributions, which should be related, at least loosely, to RHESSI science.
MAX MILLENNIUM NEWS
25 Ocober 2017
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Solar Energetic Particle Forecasting Algorithms and Associated
False Alarms
-- Swalwell, B., Dalla, S., Walsh, R.
Magnetic swirls and associated fast magnetoacoustic kink waves in
a solar chromospheric flux tube
-- K. Murawski, P. Kayshap, A. K. Srivastava, D. J. Pascoe,
P. Jelínek, B. Kuźma, V. Fedu
High-wavenumber solar f-mode strengthening prior to active region
formation
-- Singh, N. K., Raichur, H., & Brandenburg, A.
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
MAX MILLENNIUM NEWS
18 Ocober 2017
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Block-induced complex structures building the flare-productive solar
active region 12673
-- Shuhong Yang, Jun Zhang, Xiaoshuai Zhu, Qiao Song
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
MAX MILLENNIUM NEWS
11 Ocober 2017
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Reconstruction of a Large-scale Pre-flare Coronal Current Sheet
Associated with an Homologous X-shaped Flare
-- Chaowei Jiang, Xiaoli Yan, Xueshang Feng, Aiying Duan, Qiang Hu,
Pingbing Zuo, Yi Wang
Comparison of Two Coronal Magnetic Field Models for Reconstructing a
Sigmoidal Solar Active Region With Coronal Loops
-- Aiying Duan, Chaowei Jiang, Qiang Hu, Huai Zhang, G. Allen Gary,
S. T. Wu, Jinbin Cao
A Magnetic Bald-Patch Flare in Solar Active Region 11117
-- Chaowei Jiang, Xueshang Feng, S. T. Wu, Qiang Hu
Reply to comment by Usoskin (2017) on the paper "On a role of
quadruple component of magnetic field in defining solar activity in
grand cycles"
-- Zharkova V.V., Popova E., Shepherd S.J. and Zharkov S.
Non-thermal hydrogen Balmer and Paschen emission in solar flares
generated by electron beams
-- Druett M. and Zharkova V.V.
Pulsations in the Earth's Lower Ionosphere Synchronized with Solar
Flare Emission
-- Laura A. Hayes, Peter T. Gallagher, Joseph McCauley,
Brian R. Dennis, Jack Ireland, Andrew Inglis
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
MAX MILLENNIUM NEWS
04 Ocober 2017
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Oscillations Excited by Plasmoids Formed During Magnetic
Reconnection in a Vertical Gravitationally Stratified Current Sheet
-- P. Jelinek, M. Karlicky, T. Van Doorsselaere, M. Barta
Doppler shift oscillations from a hot line observed by IRIS
-- Dong Li, Zongjun Ning, Yu Huang, N.-H. Chen, Qingmin Zhang,
Yingna Su, Wei Su
Dispersive Evolution of Nonlinear Fast Magnetoacoustic Wave Trains
-- D. J. Pascoe, C. R. Goddard, and V. M. Nakariakov
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu