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
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> 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
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> 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.
MAX MILLENNIUM NEWS
15 April 2020
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Wave amplitude modulation in fan loops as observed by AIA/SDO
-- Aishawnnya Sharma, Durgesh Tripathi, Robertus Erdelyi, G. R. Gupta,
G. A. Ahmed
Simulating White-Light Images of Coronal Structures
for Parker Solar Probe/WISPR: Study of the Total Brightness Profiles
-- Giuseppe Nistico, Volker Bothmer, Angelos Vourlidas, Paulett Liewer,
Arnaud Thernisien, Guillermo Stenborg, Russell Howard
Transverse oscillations of a double-strutured solar filament
-- P. Jelínek, M. Karlicky, V. V. Smirnova, A. A. Solov'ev
Predicting Coronal Mass Ejections Using SDO/HMI Vector Magnetic Data Products
and Recurrent Neural Networks
-- Hao Liu, Chang Liu, Jason T. L. Wang, Haimin Wang
Magnetic Structure of an Erupting Filament
-- Shuo Wang, Jack M. Jenkins, Valentin Martinez Pillet, Christian Beck,
David M. Long, Debi Prasad Choudhary, Karin Muglach, James McAteer
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
10 April 2020
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Initiation and Early Kinematic Evolution of Solar Eruptions
-- X. Cheng, J. Zhang, B. Kliem, T. Török, C. Xing, Z. J. Zhou, B. Inhester,
M. D. Ding
QUASI-PERIODIC PULSATIONS IN SOLAR AND STELLAR FLARES. REVIEW
-- E.G. Kupriyanova, D.Yu. Kolotkov, V.M. Nakariakov, A.S. Kaufman
Solar Active Region Heating Diagnostics from High-temperature Emission
Using the MaGIXS
-- P. S. Athiray, Amy R. Winebarger, Will T. Barnes, Stephen J. Bradshaw,
Sabrina Savage, Harry P. Warren, Ken Kobayashi, Patrick Champey, Leon Golub,
and Lindsay Glesener
Loss-cone instability modulation due to a magnetohydrodynamic sausage mode
oscillation in the solar corona
-- Carley, Eoin P.; Hayes, Laura A.; Murray, Sophie A.; Morosan, Diana E.;
Shelley, Warren; Vilmer, Nicole; Gallagher, Peter T.
FOXSI-2 Solar Microflares.
I. Multi-instrument Differential Emission Measure Analysis and Thermal Energies
-- P. S. Athiray, Juliana Vievering, Lindsay Glesener, Shin-nosuke Ishikawa,
Noriyuki Narukage, Juan Camilo Buitrago-Casas, Sophie Musset, Andrew Inglis,
Steven Christe, Säm Krucker, and Daniel Ryan
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
1 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
HATS: A Ground-Based Telescope to Explore the THz Domain
-- C.G. Giménez de Castro, J.-P. Raulin, A. Valio, G. Alaia, V. Alvarenga,
E.C. Bortolucci, S.H. Fernandes, C. Francile, T. Giorgetti, A.S. Kudaka,
F.M. Lopez, R. Marcon, A. Marun, M. Zaquela
Failed prominence eruptions near 24 cycle maximum
-- B. Filippov
Properties of Streamer Wave Events Observed During the STEREO Era
-- Bieke Decraemer, Andrei N. Zhukov, Tom Van Doorsselaere
Simulating Solar Flare Irradiance with Multithreaded Models of Flare Arcades
-- Jeffrey W. Reep, Harry P. Warren, Christopher S. Moore, Crisel Suarez,
Laura A. Hayes
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. 372: “Heating of the Solar Photosphere during a White-Light Flare”, by Jan Jurčak: the best-ever spectrum of the flaring photosphere.
No. 373: "SOL2017-09-04 (M5.5) 2017 as a Source of Relativistic Electrons and Protons,” by Alexei Struminsky: Flare-accelerated particles, rather than SEPs, energize sustained gamma-ray emission.
No. 374: "Using overlappogram data to find hot flare plasma,” by Louise Harra: imaging Fe XXIV at high resolution with the EIS slot data
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
25 March 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
Counter-streaming strahls and heat flux dropouts as possible signatures
of local particle acceleration in the solar wind
-- O. Khabarova, V. Zharkova, Q. Xia, and O. E. Malandraki
New Star Observations with NuSTAR: Flares from Young Stellar Objects
in the rho Ophiuchi Cloud Complex in Hard X-Rays
-- Juliana T. Vievering, Lindsay Glesener, Brian W. Grefenstette, and
David M. Smith
Accelerated Electrons Observed Down to <7 keV in a NuSTAR Solar Microflare
-- Lindsay Glesener, Sam Krucker, Jessie Duncan, Iain G. Hannah,
Brian W. Grefenstette, Bin Chen, David M. Smith, Stephen M. White, and
Hugh Hudson
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
18 March 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
Magnetic helicity dissipation and production in an ideal MHD code
-- Axel Brandenburg, Evan Scannapieco
Magnetic twist profile inside magnetic clouds derived with a superposed
epoch analysis
-- Lanabere V., Dasso S., Demoulin P., Janvier M., Rodriguez L. and
Masias-Meza J.J.
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