MAX MILLENNIUM NEWS
6 February 2019
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
Determining normal mode features from numerical simulations using
CEOF analysis: I. Test case using transverse oscillations of a
magnetic slab
-- S. Rial, I. Arregui, R. Oliver, and J. Terradas
Modelling the Effect of Mass-Draining on Prominence Eruptions
-- Jack M. Jenkins, Matthew Hopwood, Pascal Demoulin,
Gherardo Valori, Guillaume Aulanier, David M. Long,
Lidia van Driel-Gesztelyi
Transverse waves in coronal flux tubes with thick boundaries:
The effect of longitudinal flows
-- R. Soler
Electron distribution and energy release in magnetic reconnection
outflow regions during the pre-impulsive phase of a solar flare
-- Marina Battaglia, Eduard P. Kontar, Galina Motorina
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
The special issue is available online:
https://www.sciencedirect.com/journal/advances-in-space-research/vol/63/iss…
The Guest Editors are grateful to all the authors for their valuable
time and efforts, without which the publication of this issue would have
been impossible, and we congratulate them for the acceptance of their
manuscripts. We also thank all the referees for their hard work and
invaluable advice, that profoundly improved the Issue.
Guest Editors:
Manolis K.Georgoulis,
Eduard P.Kontar
MAX MILLENNIUM NEWS
30 January 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
Benchmarking CME arrival time and impact: Progress on metadata,
metrics, and events
-- C. Verbeke, M. L. Mays, M. Temmer, S. Bingham, R. Steenburgh,
M. Dumbovic, M. Nunez, L. K. Jian, P. Hess, C. Wiegand,
A. Taktakishvili, J. Andries
First Unambiguous Imaging of Large-Scale Quasi-Periodic
Extreme-Ultraviolet Wave or Shock
-- Shen, Yuandeng; Chen, P. F.; Liu, Ying D.; Shibata, Kazunari;
Tang, Zehao; Liu, Yu
Coronal Imaging with the Solar UltraViolet Imager
-- Sivakumara K. Tadikonda, Douglas C. Freesland, Robin R. Minor,
Daniel B. Seaton, Gustave J. Comeyne, Alexander Krimchansky
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
Coronal Mass Ejection-driven Type II solar radio burst structure with
LOFAR and radio-wave scattering
by Nicolina Chrysaphi et al.*
http://cesra.net/?p=2109
Synthetic Radio Imaging in Quiet and Eruptive Solar Cases
by S. P. Moschou et. al.*
http://cesra.net/?p=2101
Simulation of Focusing Effect of Traveling Ionospheric Disturbances on
Meter-Decameter Solar Dynamic Spectra
by A. Koval et al*
http://cesra.net/?p=2090
---
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
No. 343, “Short-period Waves”, by Sijie YU and Bin CHEN. New decimetric imaging spectroscopy suggests Alfvenic energy transport in solar flares.
No. 342, “The Interesting RHESSI/SAS Archive”, by Hugh Hudson and Martin Fivian. The full mission database shows RHESSI to have been very stable geometrically.
Although RHESSI is off the air, results continue to appear. We welcome contributions on a variety of solar research areas, especially those involving RHESSI, and will welcome more for at least the duration of 2019. 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/ for the original series, 2005-2008.
MAX MILLENNIUM NEWS
22 January 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
Investigation of pre-flare dynamics using the weighted horizontal
magnetic gradient method: From small to major flare classes
-- Marianna B. Korsos, Shuhong Yang, Robert Erdelyi
Seismological determination of the Alfven speed and plasma-beta in
solar photospheric bright points
-- Il-Hyun Cho, Yong-Jae Moon, Valery M. Nakariakov, Dae Jung Yu,
Jin-Yi Lee, Su-Chan Bong, Rok-Soon Kim, Kyung-Suk Cho,
Yeon-Han Kim, Jae-Ok Lee
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
16 January 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
Dynamo Wave Patterns Inside the Sun Revealed by Torsional
Oscillations
-- Alexander G. Kosovichev and Valery V. Pipin
Evidence of Twisting and Mixed-polarity Solar Photospheric Magnetic
Field in Large Penumbral Jets: IRIS and Hinode Observations
-- Tiwari, Sanjiv K.; Moore, Ronald L.; De Pontieu, Bart;
Tarbell, Theodore D.; Panesar, Navdeep K.; Winebarger, Amy R.;
Sterling, Alphonse C.
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
No. 342, the first of 2019: “The Interesting RHESSI/SAS Archive”, by Hugh Hudson and Martin Fivian. The full mission database shows RHESSI to have been very stable geometrically.
Three Nuggets in December 2018:
No. 341, “Homologous White Light Solar Flares”, by Paolo Roman and Abouazza Elmhamdi. Homologous white-light flares, in rapid succession, and coronal null points.
No. 340, “The Flight of FOXSI-3”, by Lindsay Glesener and Noriyuki Narukage. Single-photon counting and direct focusing across hard and soft X-ray energies.
No. 339, “Stellar Flares and Starspots”, by Lauren Doyle. Stellar flares don’t spatially match their starspots.
In 2018 we had 28 Nuggets, ranging over a wide variety of HXR-themed solar research matters, and welcome more for 2019. 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/ for the 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
02 January 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
Dissipation scale lengths of density turbulence in the inner solar
wind
-- K. Sasikumar Raja, Prasad Subramanian, Madhusudan Ingale,
R. Ramesh
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
02 January 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
On the Possibility of Generating Harmonics of the Electron Plasma
Frequency in the Solar Atmosphere due to Explosive Instability in
a System of Interpenetrating Electron and Ion Flows
-- V. V. Fomichev, S. M. Fainshtein, and G. P. Chernov
Determination of the total accelerated electron rate and power
using solar flare hard X-ray spectra
-- Eduard P. Kontar, Natasha L. S. Jeffrey, and A. Gordon Emslie
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