No. 390, “Prediction of Solar Cycle 25”, by Leif SVALGAARD. Now we know how big the next solar maximum will be.
No. 391, “Electric Current Neutralizationand Eruption”, by Ellis AVALLONE and Xudong SUN. Coronal currents without neutralizing return currents correlate with eruption.
No. 392, “Hot Flare Onsets”, by Hugh HUDSON et al. The pre-impulsive temperatures of solar flares are already hot, 10-15 MK.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
21 October 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
Sub-second time evolution of Type III solar radio burst sources
at fundamental and harmonic frequencies
-- X. Chen, E. P. Kontar, N. Chrysaphi, N. L.S. Jeffrey, M. Gordovskyy,
Y. Yan, B. Tan
Magnetically coupled atmosphere, fast sausage MHD waves, and
forced magnetic field reconnection during the SOL2014-09-10T17:45 flare
-- Hana Meszarosova and Peter Gomory
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. 388, “Submerged Flare Acoustic Sources,” by Juan Camilo BUITRAGA CASAS and Angel MARTINEZ: Flare acoustic radiation emanates from a source _inside_ the Sun.
No. 389, “Flare/CME Cartoon Archive,” by Hugh HUDSON. A new edition of the Flare/CME Archive, now packing 0.4 kilotoons.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
14 October 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
Differential rotation of the solar corona: A new data-adaptive
multiwavelength approach
-- S. Mancuso, S. Giordano, D. Barghini, D. Telloni
Magnetic Helicity Flux across Solar Active Region Photospheres:
I. Hemispheric Sign Preference in Solar Cycle 24
-- Sung-Hong Park, K. D. Leka, Kanya Kusano
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
7 October 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
Seismological constraints on the solar coronal heating function
-- D. Y. Kolotkov, T. J. Duckenfield, V. M. Nakariakov
The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram
and Doppler Data to Determine Coronal Magnetic Field Evolution
-- Todd J. Hoeksema, William P. Abbett, David J. Bercik, Mark C. M. Cheung,
Marc L. DeRosa, George H. Fisher, Keiji Hayashi, Maria D. Kazachenko,
Yang Liu, Erkka Lumme, Benjamin J. Lynch, Xudong Sun, and Brian T. Welsch
Radio and X-ray Observations of Short-lived Episodes of Electron Acceleration
in a Solar Microflare
-- Rohit Sharma, Marina Battaglia, Yingjie Luo, Bin Chen, Sijie Yu
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. 385, “White-light emission and photospheric magnetic field changes in flares,” by J. Sebastian CASTELLANOS DURÁN and Lucia Kleint: There are strong correlations between white-light flare emissions and line-of-sight magnetic field changes.
No. 386, "Relation of Non-neutralized electric currents and the activity in active regions,” by P. VEMAREDDY: Non-neutralized coronal current systems contribute to CME eruptions.
No. 387, “Circular Ribbon Flare at Microwaves,” by Jeongwoo LEE: Breakout reconnection reveals itself via microwave polarization measurements.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
30 September 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
Research progress based on observations of the New Vacuum Solar Telescope
-- Yan,X.L.,Liu,Z.,Zhang,J.,Xu,Z.
Dynamics evolution of a solar active-region filament from quasi-static state
to eruption: rolling motion, untwisting motion, material transfer, and chirality
-- Yan, X.L.; Li, Q.L.; Chen, G.R.; Xue, Z.K.; Feng, L.; Wang, J.C.;
Yang, L.H.; Zhang,Y.
Microwave Study of a Solar Circular Ribbon Flare
-- Jeongwoo Lee, Stephen M. White, Xingyao Chen, Yao Chen, Hao Ning, Bo Li,
Satoshi Masuda
Precise Formation-Flying Telescope in Target-Centric Orbit: the Solar Case
-- Saint-Hilaire, Pascal; Marchese, Jeffrey E.
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
23 September 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
Propagation Effects in Quiet Sun Observations at Meter Wavelengths
-- Rohit Sharma and Divya Oberoi
Twin Null-Point-Associated Major Eruptive Three-Ribbon Flares
with Unusual Microwave Spectra
-- V.V. Grechnev, N.S. Meshalkina, A.M. Uralov, A.A. Kochanov, S.V. Lesovoi,
I.I. Myshyakov, V.I. Kiselev, D.A. Zhdanov, A.T. Altyntsev, M.V. Globa
Trajectory Determination for Coronal Ejecta Observed by WISPR/Parker Solar Probe
-- P. C. Liewer, J. Qiu, P. Penteado, J. R. Hall, A. Vourlidas, R. A. Howard
Recurring Homologous Solar Eruptions in NOAA AR 11429
-- Dhakal, S. K., Zhang, J., Vemareddy, P., Karna, N.
Resonant absorption: transformation of compressive motions into vortical motion
-- M. Goossens, I. Arregui, R. Soler, T. Van Doorsselaere
The depth and the vertical extent of the energy deposition layer
in a medium-class solar flare
-- Krzysztof Radziszewski, Robert Falewicz, Pawel Rudawy
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. 382, "SOL2013-11-10 Eruptive Circular-ribbon Flare with Extended Remote Brightenings," by Chang LIU et al.: a circular-ribbon event can launch an eruption by breaking through its separatrix dome.
No, 383, "Energy Partitioning in a Nonthermally Dominated Two-loop Solar Flare," by Galina MOTORINA et al.: Modeling the prpagation of energy via GX Simulator in an early-impulsive flare.
No. 384, "Sunspot Differential Rotation in an X-class Flare," by Richard GRIMES et al.: Observations suggesting how the coronal tail can wag the photospheric dog.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
16 September 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
Helicity proxies from linear polarisation of solar active regions
-- A. Prabhu, A. Brandenburg, M. J. Kapyla, A. Lagg
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