MAX MILLENNIUM NEWS
30 October 2019
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
A Very Narrow RHESSI X-ray Flare on 25 September 2011
-- Brian R. Dennis, Anne K. Tolbert
First Detection of Plasmoids from Breakout Reconnection on the Sun
-- Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos, Peter F. Wyper,
C. Richard DeVore
2. FROM THE EDITOR
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The Max Millennium program exists to enhance all aspects of solar
flare 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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
23 October 2019
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
A New Type of Jets in a Polar Limb of Solar Coronal Hole
-- Il-Hyun Cho, Yong-Jae Moon, Kyung-Suk Cho, Valery M. Nakariakov, Jin-Yi Lee,
Yeon-Han Kim
First imaging spectroscopy observations of solar drift pair bursts
-- Alexey Kuznetsov, Eduard Kontar
Round-Trip Slipping Magnetic Reconnection Observed in a Fan-Spine Jet
-- Yuandeng Shen; Zhining Qu; Chengrui Zhou; Yadan Duan; Zehao Tang; Ding Yuan
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare 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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
16 October 2019
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
A global two-scale helicity proxy from pi-ambiguous solar magnetic fields
-- Axel Brandenburg
Multi-layered Kelvin-Helmholtz Instability in the Solar Corona
-- Ding Yuan, Yuandeng Shen, Yu Liu, Xueshang Feng, Rony Keppens
Magnetohydrodynamic Seismology of Quiet Solar Active Regions
-- Sergey A. Anfinogentov; Valery M. Nakariakov
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare 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 keiji.yoshimura at montana.edu
No. 358: “The Last Best Flares”, by Hugh Hudson, Ed Cliver, and Brian Dennis. Major flares tend to happen at the very ends of sunspot cycles.
No. 359: “Submillimeter Radiation as the Thermal Component of the Neupert Effect,” by Guigue Giménez de Castro: Flare emission at the highest radio frequencies can be bremsstrahlung.
No. 360: “Searching SOLfully within the Nuggets,“ by Hugh Hudson: The IAU identifier works well for finding items about a particular event.
No. 361: “Non-radial jets on the edges of active regions,” by Peter Wyper: The very common jet structures we see can naturally combine twist and breakout.
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets for these and others. Comments about specific flares can be found by searching for their "SOLyyyy-mm-dd" identifier from this home page.
MAX MILLENNIUM NEWS
9 October 2019
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
Test magnetohydrostatic extrapolation with radiative MHD simulation
of a solar flare
-- Xiaoshuai Zhu & Thomas Wiegelmann
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare 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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
2 October 2019
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
Real-time solar image classification: assessing spectral, pixel-based approaches
-- J. Marcus Hughes, Vicki W. Hsu, Daniel B. Seaton, Hazel M. Bain,
Jonathan M. Darnel, Larisza Krista
Modelling Mg II During Solar Flares. II. Non-equilibrium Effects
-- Kerr, Graham S., Carlsson, Mats and Allred, J.C.
Calibration of the Instrumental Crosstalk for the Near-IR Imaging
Spectropolarimeter at the NST
-- K. Ahn and W. Cao
On the Source Position and Duration of a Solar Type III Radio Burst
Observed by LOFAR
-- PeiJin Zhang, SiJie Yu, Eduard Kontar, ChuanBing Wang
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare 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 keiji.yoshimura at montana.edu
No. 356: “EVE-RHESSI DEM Models and the Low-Energy Cutoff for Non-thermal Electrons”, by Jim McTiernan. Characterizing flare temperature distributions helps to define the non-thermal energy release.
No. 357: “Dynamic Processes of the Moreton Wave on 2014 March 29”, by Denis Cabezas and the FMT team. A beautiful chromospheric wave was excited by the best-observed flare ever.
No. 358: “The Last Best Flares”, by Hugh Hudson, Ed Cliver, and Brian Dennis. Major flares tend to happen at the very ends of sunspot cycles.
No. 359: “Submillimeter Radiation as the Thermal Component of the Neupert Effect.” Flare emission at the highest radio frequencies can be bremsstrahlung.
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets for these and others. Comments about specific flares can be found by searching for their SOLyyyy-mm-dd identifier from this home page.