MAX MILLENNIUM NEWS
29 March 2017
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
High-resolution observations of flare precursors in the low solar
atmosphere
-- Haimin Wang, Chang Liu, Kwangsu Ahn, Yan Xu, Ju Jing, Na Deng,
Nengyi Huang, Rui Liu, Kanya Kusano, Gregory D. Fleishman, Dale E.
Gary and Wenda Cao
Solar Energetic Particle transport near a Heliospheric Current
Sheet
-- Battarbee, M., Dalla, S., and Marsh, M.S.
Investigating the Magnetic Imprints of Major Solar Eruptions with
SDO/HMI High-Cadence Vector Magnetograms
-- Xudong Sun, J. Todd Hoeksema, Yang Liu, Maria Kazachenko, Ruizhu Chen
Coronal loop density profile estimated by forward modelling of
EUV intensity
-- D. J. Pascoe, C. R. Goddard, S. Anfinogentov, and
V. M. Nakariakov
The magnetic connectivity of coronal shocks to the visible solar
surface during long-duration gamma-ray events
-- Illya Plotnikov, Alexis P. Rouillard, Gerald H. Share
Dissipative instability in a partially ionised prominence slab
-- I. Ballai, B. Pinter, R. Oliver and M. Alexandrou
Significance testing for quasi-periodic pulsations in solar and
stellar flares
-- C. E. Pugh, A.-M. Broomhall, V. M. Nakariakov
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. 296, “Suppression of Hydrogen Emission in an X-class White-light Solar Flare,” by Ondřej Procházka and Ryan Milligan. The absence of hydrogen signatures suggests an event buried in the deep solar atmosphere.
No. 295, “Radio Emissions from Double RHESSI TGFs”, by Andrey Mezentsev and Thomas Gjesteland: Lightning helps with microsecond timing calibrations, and is really interesting as a phenomenon of high-energy astrophysics.
No. 294, “Edward Chupp”
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
22 March 2017
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
High Resolution Observations of a White Light Flare with NST
-- Yurchyshyn, V., Kumar, P., Abramenko, V., Xu, Y., Goode, P., Cho,
K.S., Lim, E.K 2017-03-21
Flare forecasting at the Met Office Space Weather Operations Centre
-- Sophie A. Murray, Suzy Bingham, Michael Sharpe, David Jackson
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
15 March 2017
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 Effectiveness of Multi-Instrument Solar Flare Observations
During Solar Cycle 24
-- Ryan Milligan, Jack Ireland
The Grad-Shafranov Reconstruction of Toroidal Magnetic Flux Ropes:
Method Development and Benchmark Studies
-- Qiang Hu
Long-Period Intensity Pulsations in Coronal Loops Explained by
Thermal Non-Equilibrium Cycles
-- Clara Froment, Frederic Auchere, Guillaume Aulanier, Zoran Mikic,
Karine Bocchialini, Eric Buchlin, Jacques Solomon
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. 294, “Edward Chupp”
No. 295, “Radio Emissions from Double RHESSI TGFs”, by Andrey Mezentsev and Thomas Gjesteland: Lightning helps with microsecond timing calibrations, and is really interesting as a phenomenon of high-energy astrophysics.
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
08 March 2017
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
Differences between Doppler velocities of ions and neutral atoms
in a solar prominence
-- Tetsu Anan, Kiyoshi Ichimoto, Andrew Hillier
Interaction of Two Active Region Filaments Observed by NVST and
SDO
-- Liheng Yang, Xiaoli Yan, Ting Li, Zhike Xue, Yongyuan Xiang
On flare-CME characteristics from Sun to Earth combining
remote-sensing image data with in-situ measurements supported by
modeling
-- M. Temmer, J.K. Thalmann, K. Dissauer, A.M. Veronig,
J. Tschernitz, J. Hinterreiter, L. Rodriguez
High-frequency transverse oscillations and intensity perturbations
in spicular-type events
-- J. Shetye, D. Kuridze, M. Stangalini, J. G. Doyle, E. Scullion,
V. Henriques, T. Ray
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
01 March 2017
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
Sheath-Accumulating Propagation of Interplanetary Coronal Mass
Ejection
-- Takuya Takahashi, Kazunari Shibata
Investigating the Wave Nature of the Outer Envelope of Halo Coronal
Mass Ejections
-- Ryun-Young Kwon and Angelos Vourlidas
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. 292, “RHESSI’s 15th Anniversary”, by Brian Dennis, Sa”m Krucker, and Albert Shih. We celebrate 15 years in orbit!
No. 293, “PIerre Kaufmann”. RHESSI has lost a friend.
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
22 February 2017
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
Apparent and Intrinsic Evolution of Active Region Upflows
-- Deb Baker, Miho Janvier, Pascal Demoulin, Cristina Mandrini
An Early Diagnostics of the Geoeffectiveness of Solar Eruptions
from Photospheric Magnetic Flux Observations: The Transition from
SOHO to SDO
-- I.M. Chertok, V.V. Grechnev, A.A. Abunin
Plasma Brightenings in a Failed Solar Filament Eruption
-- Y. Li, M. D. Ding
Interactive Multi-Instrument Database of Solar Flares
-- Viacheslav M Sadykov, Rishabh Gupta, Alexander G Kosovichev,
Vincent Oria, Gelu M Nita
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
15 February 2017
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
Moreton and EUV Waves Associated with an X1.0 Flare and CME
Ejection
-- Carlos Francile, Fernando M. López, Hebe Cremades, Cristina
H. Mandrini, Maria Luisa Luoni, David M. Long
The transition from eruptive to confined flares in the same active
region
-- Zuccarello, Francesco P.; Chandra, Ramesh; Schmieder, Brigitte;
Aulanier, Guillaume; Joshi, Reetika
Vortex and sink flows in eruptive flares as a model for coronal
implosions
-- Zuccarello, Francesco P.; Aulanier, Guillaume; Dudik, Jaroslav;
Demoulin, Pascal; Schmieder, Brigitte; Gilchrist, Stuart A.
A 17 June 2011 polar jet and its presence in the background solar
wind
-- H.-S. Yu, B.V. Jackson, Y.-H. Yang, N.-H. Chen, A. Buffington,
P. P. Hick
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