MAX MILLENNIUM NEWS
27 February 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
Helical Twisting Number and Braiding Linkage Number of Solar Coronal
Loops
-- Markus J. Aschwanden
Small-scale motions in solar filaments as the precursors of eruptions
-- Daikichi SEKI, Kenichi OTSUJI, Hiroaki ISOBE, Takako T. ISHII,
Kiyoshi ICHIMOTO and Kazunari SHIBATA
Modeling of Heliospheric Modulation of Cosmic-Ray Positrons in
a Very Quiet Heliosphere
-- O. P. M. Aslam, D. Bisschoff, M. S. Potgieter, M. Boezio, and
R. Munini
Interpreting magnetic helicity flux in solar flux emergence
-- Prior, C. and MacTaggart, D.
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
20 February 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
Transient Inverse-FIP Plasma Composition Evolution within a Confined
Solar Flare
-- Deborah Baker, Lidia van Driel-Gesztelyi, David H. Brooks,
Gherardo Valori, Alexander W. James, J. Martin Laming, David M. Long,
Pascal Demoulin, Lucie M. Green, Sarah A. Matthews, Katalin Olah,
Zsolt Kovari
The Role of a Tiny Brightening in a Huge Geo-effective Solar Eruption
Leading to the St Patrick's Day Storm
-- Yumi Bamba, Satoshi Inoue, and Keiji Hayashi
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. 345, “A Energetic Pre-flare: Electron Distributions in Magnetic Reconnection Outflows,” by Marina BATTAGLIA, Eduard KONTAR, and Galina MOTORINA. Assessing energy partition in a very interesting pre-impulsive flare development.
No. 344, “Linear Polarization in H-alpha Flares,” by Tomoko KAWATE and Yoichiro HANAOKA. H-alpha polarization (perhaps implying electron beams) is rarely observable, but in one case there are suggstive results.
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
MAX MILLENNIUM NEWS
13 February 2019
CONTENTS
0. A MILESTONE, AND THANKS, FOR THE E-PRINT ARCHIVE
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
0. A MILESTONE, AND THANKS, FOR THE E-PRINT ARCHIVE
===================================================
<richard.canfield at montana.edu>
This week the Max Millennum Solar Physics E-Print Archive logged it's
4000th submission! That's trivial on the scale of the Cornell/LANL
arXiv, of course, but it demonstrates empirically what we all know --
there is value to us in an archive that is specific to a
subdiscipline -- solar and heliospheric actvity, in this case.
It gives me great pleasure to thank Alisdair Davey for his seminal
role in creating the E-Print Archive in mid-2000 and maintaining it
ever since. I searched the Max Millennium Science Mail Archive
to get a sense of the duration of his committment. I found that
the Max Millennium News message announcing the availability of the
enhanced E-Print archive came shortly after a message from Bob Lin,
reporting that RHESSI had been reconfirmed for flight after the
spacecraft was severely damaged as the result of the shake table
malfunction during a vibration test!
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
A basal contribution from p-modes to the Alfvénic wave flu in the
Sun's Corona
-- R. J. Morton, M. Weberg, J. A. McLaughlin
Multiwavelength Study of Equatorial Coronal-Hole Jets
-- Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos,
Peter F. Wyper, C. Richard DeVore, Craig E. DeForest
Non-thermal hydrogen Lyman line and continuum emission in solar
flares generated by electron beams
-- Druett, M.K. and Zharkova V.V.
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
6 February 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
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