First observation of a transitioning Type II solar radio burst using the
Low-Frequency Array (LOFAR) by Nicolina Chrysaphi et al.
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2579
Loss-cone instability modulation due to a magnetohydrodynamic sausage
mode oscillation in the solar corona by E. P. Carley et al.
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2559
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are
short communications written in 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
http://www.facebook.com/solarcesra/ and http://twitter.com/CESRA_community.
MAX MILLENNIUM NEWS
27 May 2020
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
Sunquake with a second-bounce, other sunquakes and emission associated
with X9.3 flare of 6 September 2017. II. Proposed interpretation
-- Valentina Zharkova, Sergei Zharkov, Malcolm Druett, Sarah Matthews, and
Satoshi Inoue
f-mode strengthening from a localized bipolar subsurface magnetic field
-- Nishant K. Singh, Harsha Raichur, Maarit J. Kapyla, Matthias Rheinhardt,
Axel Brandenburg, Petri J. Kapyla
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
20 May 2020
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
Imaging and spectral study on the null point of a fan-spine structure
during a solar flare
-- Shuhong Yang, Qingmin Zhang, Zhi Xu, Jun Zhang, Ze Zhong, Yang Guo
Forecasting Solar Cycle 25 Using Deep Neural Networks
-- B. Benson, W.D. Pan, A. Prasad, G.A. Gary, Q. Hu
An Observational Test of Solar Plasma Heating by Magnetic Flux Cancellation
-- Sung-Hong Park
The Drivers of Active Region Outflows into the Slow Solar Wind
-- David H. Brooks, Amy R. Winebarger, Sabrina Savage, Harry P. Warren,
Bart De Pontieu, Hardi Peter, Jonathan W. Cirtain, Leon Golub, Ken Kobayashi,
Scott W. McIntosh, David McKenzie, Richard Morton, Laurel Rachmeler,
Paola Testa, Sanjiv Tiwari, and Robert Walsh
HXR emission from an activated flux rope and subsequent evolution
of an eruptive long duration solar flare
-- Suraj Sahu, Bhuwan Joshi, Prabir K. Mitra, Astrid M. Veronig, V. Yurchyshyn
A Survey of Computational Tools in Solar Physics
-- Monica G. Bobra, Stuart J. Mumford, Russell J. Hewett, Steven D. Christe,
Kevin Reardon, Sabrina Savage, Jack Ireland, Tiago M. D. Pereira, Bin Chen,
and David Perez-Suarez
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
13 May 2020
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
Sunquake with a second bounce, other sunquakes, and emission associated with
the X9.3 flare of 6 September 2017. I. Observations
-- S. Zharkov, S. Matthews, V. Zharkova, M. Druett, S. Inoue, I. E. Dammasch,
C. Macrae
The PDFI_SS Electric Field Inversion Software
-- George H. Fisher, Maria D. Kazachenko, Brian T. Welsch, Xudong Sun,
Erkka Lumme, David J. Bercik, Marc L. DeRosa, Mark C. M. Cheung
Spatial Distribution of Origin of Umbral Waves in a Sunspot Umbra
-- Vasyl Yurchyshyn, Ali Kilcik, Seray Sahin, Valentina Abramenko, Eun-Kyung Lim
A Unique Resource for Solar Flare Diagnostic Studies:
the SMM Bent Crystal Spectrometer
-- J. Sylwester, B. Sylwester, K. J. H. Phillips, A. Kepa, C. G. Rapley
Inferring Vector Magnetic Fields from Stokes Profiles of GST/NIRIS
Using a Convolutional Neural Network
-- Hao Liu, Yan Xu, Jiasheng Wang, Ju Jing, Chang Liu, Jason T. L. Wang,
Haimin Wang
Global Energetics of Solar Flares, X. Petschek Reconnection Rate
and Alfvén Mach Number of Magnetic Reconnection Outflows
-- Markus J. Aschwanden
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. 378, “Rejuvenating Solar Flare Termination Shocks as Particle Accelerators,” by Bin CHEN: At last, clear evidence for a long-predicted phenomenon.
No. 379, “Quasi-periodic pulsations as indicators of oscillatory processes in solar flare,” by Elena Kupriyanova et al.: Many, many QPPs
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
6 May 2020
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
Transverse coronal loop oscillations excited by homologous circular-ribbon flares
-- Q. M. Zhang, J. Dai, Z. Xu, D. Li, L. Lu, K. V. Tam, A. A. Xu
Temporal evolution of oscillating coronal loops
-- Goddard, C. R.; Nistico, G.
Intrusion of Magnetic Peninsula toward the Neighboring Opposite-polarity Region
That Triggers the Largest Solar Flare in Solar Cycle 24
-- Yumi Bamba, Satoshi Inoue, Shinsuke Imada
On the Relationship Between Transit Time of ICMEs and Strength of the Initiated
Geomagnetic Storms
-- I.M. Chertok
Standing kink waves in sigmoid solar coronal loops: implications for coronal seismology
-- N. Magyar; V. 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
Solar polarization observations at 3 and 13 mm
by J. Kallunki and M. Tornikoski
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2549
Observing onset of turbulent fast magnetic reconnection in solar
microflares
by L. P. Chitta and A. Lazarian
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2539
------
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are short
communications written in 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
http://www.facebook.com/solarcesra/ and http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
29 April 2020
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
Excitation of negative energy surface magnetohydrodynamic waves
in an incompressible cylindrical plasma
-- Yu, D.J., Nakariakov, V.M.
Solar Flares Forecasting Using Time Series and Extreme Gradient
Boosting Ensembles
-- Cinto, T., Gradvohl, A. L. S., Coelho, G. P. , da Silva, A. E. A.
Statistical Study of GOES X-ray Quasi-Periodic Pulsations in Solar Flares
-- Laura A. Hayes, Andrew R. Inglis, Steven Christe, Brian Dennis,
Peter T. Gallagher
Particle acceleration and transport during 3D CME eruptions
-- Qian Xia, Joel Dahlin, Valentina Zharkova and Spiro Antiochos
First Observation of a Type II Solar Radio Burst Transitioning
between a Stationary and Drifting State
-- Chrysaphi, N., Reid, H. A. S., and Kontar, E. P.
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
22 April 2020
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
Plasma Diagnostics from Active Region and Quiet-Sun Spectra Observed
by Hinode/EIS: Quantifying the Departures from a Maxwellian Distribution
-- Juraj Lorincik, Jaroslav Dudík, Giulio del Zanna, Elena Dzifcakova,
Helen E. Mason
Sunquakes of Solar Cycle 24
-- I.N. Sharykin, A.G. Kosovichev
Flare Energy Release at the Magnetic Field Polarity Inversion Line
During M1.2 Solar Flare of 2015 March 15. II. Investigation of Photospheric
Electric Current and Magnetic Field Variations Using HMI 135-second
Vector Magnetograms
-- I.N. Sharykin, I.V. Zimovets, I.I.Myshyakov
Flare Energy Release in the Magnetic Field Polarity Inversion Line
During M1.2 Solar Flare of March 15, 2015. I. Onset of Plasma Heating
and Electrons Acceleration
-- I.N. Sharykin, I.V. Zimovets, I.I. Myshyakov, N.S. Meshalkina
The nature of mean-field generation in three classes of optimal dynamos
-- Axel Brandenburg, Long Chen
Active-Region Tilt Angles from White-Light Images and Magnetograms:
The Role of Magnetic Tongues
-- M. Poisson, P. Demoulin, C.H. Mandrini, M.C. Lopez Fuentes
Transient brightenings in the quiet Sun detected by ALMA at 3 mm
-- A. Nindos, C.E. Alissandrakis, S. Patsourakos, T.S. Bastian
Magneto-acoustic waves in a magnetic slab embedded in an asymmetric
magnetic environment II: Thin and wide slabs, hot and cold plasmas
-- Noemi Kinga Zsamberger, Robert Erdelyi
The Relationship between Chirality, Sense of Rotation, and Hemispheric
Preference of Solar Eruptive Filaments
-- Zhenjun Zhou , Rui Liu, Xing Cheng, Chaowei Jiang, Yuming Wang, Lijuan Liu,
and Jun Cui
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. 375: “Evidence for a Coronal Shock Wave Origin for Relativistic Protons Producing Solar Gamma-Rays and Observed by Neutron Monitors at Earth,” by Athanasios Kouloumvakos and Gerry Share. Successful modeling of prolonged solar gamma-ray emissions and terrestrial ground-level cosmic-ray events.
No. 376: "Phenomena in the unusually long pre-impulsive phase of SOL2011-06-07,” by Marian Karlický, Jana Kašparová, and Robert Sych. A massive and slowly-rising filament eruption reveals important new signatures of the physics.
No. 377: "Broad symmetrical Doppler-shifted Fe XXI line profiles,” by Vanessa Polito. It is difficult to explain “evaporation” line profiles by superposition of unresolved flows.
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.