MAX MILLENNIUM NEWS
01 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
Fermi-LAT Observations of High-energy Behind-the-limb Solar Flares
-- M. Ackermann, A. Allafort, L. Baldini, G. Barbiellini, D. Bastieri,
R. Bellazzini, E. Bissaldi, R. Bonino, E. Bottacini, J. Bregeon,
P. Bruel, R. Buehler, R. A. Cameron, M. Caragiulo, P. A. Caraveo,
E. Cavazzuti, C. Cecchi, E. Charles, S. Ciprini, F. Costanza,
S. Cutini, F. D'Ammando, F. de Palma, R. Desiante, S. W. Digel,
N. Di Lalla, M. Di Mauro, L. Di Venere, P. S. Drell, C. Favuzzi,
Y. Fukazawa, P. Fusco, F. Gargano, N. Giglietto, F. Giordano,
M. Giroletti, I. A. Grenier, L. Guillemot, S. Guiriec, T.
Jogler, G. Jóhannesson, L. Kashapova, S. Krucker, M. Kuss,
G. La Mura, S. Larsson, L. Latronico, J. Li, W. Liu, F. Longo,
F. Loparco, P. Lubrano, J. D. Magill, S. Maldera, A. Manfreda,
M. N. Mazziotta, W. Mitthumsiri, T. Mizuno, M. E. Monzani,
A. Morselli, I. V. Moskalenko, M. Negro, E. Nuss, T. Ohsugi,
N. Omodei, E. Orlando, V. Pal'shin, D. Paneque, J. S. Perkins,
M. Pesce-Rollins, V. Petrosian, F. Piron, G. Principe, S. Rainò,
R. Rando, M. Razzano, O. Reimer, F. Rubio da Costa, C. Sgrò,
D. Simone, E. J. Siskind, F. Spada, G. Spandre, P. Spinelli,
H. Tajima, J. B. Thayer, D. F. Torres, E. Troja, and G. Vianello
Determining the Intrinsic CME Flux Rope Type Using Remote-sensing
Solar Disk Observations
-- Palmerio, E., Kilpua, E. K. J., James, A. W., Green, L. M.,
Pomoell, J., Isavnin, A., and Valori, G.
Observational Evidence of Magnetic Reconnection for Brightenings
and Transition Region Arcades in IRIS observations
-- Jie Zhao, Brigitte Schmieder, Hui Li, Etienne Pariat, Xiaoshuai
Zhu, Li Feng, Michalina Grubecka
Shock-Cloud Interaction in the Solar Corona
-- Takuya Takahashi
Harmonic Resonances of Planet and Moon Orbits - From the Titius-Bode
Law to Self-Organizing Systems
-- Markus J. Aschwanden and L.A. McFadden
Charge states and FIP bias of the solar wind from coronal holes,
active regions, and quiet Sun
-- Hui Fu, Maria S. Madjarska, LiDong Xia, Bo Li, ZhengHua Huang,
Zhipeng Wangguan
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
Emission of radiation by plasmas with counter-streaming electron beams
by L. F. Ziebell et al.*
http://cesra.net/?p=1200
Simultaneous near-Sun observations of a moving type IV radio burst and
the associated white-light CME by K. Hariharan et al.*
http://cesra.net/?p=1169
Observation of quasi-periodic solar radio bursts associated with
propagating fast-mode waves by C. R. Goddard et al.*
http://cesra.net/?p=1159
*************
The Highlight of Solar Radio Physics aka CESRA Nugget are short
communications based on peer-reviewed research published bi-weekly. The
highlights are written in the language accessible to a non-expert in the
specific area and are designed to keep broader solar-heliospheric
community informed and up-to-date. The highlights can be followed,
commented, discussed etc at
http://twitter.com/CESRA_community/http://www.facebook.com/solarcesra/
No. 290, “GOES Hard X-rays?” by Hugh Hudson, Janet Machol, and Rodney Viereck. Solar minimum conditions reveal interesting properties of the GOES X-ray observations.
No. 291, “Hard X-ray Emission fro Partially Occulted Solar Flares,” by Frederic Effenberger and Fatima Rubio da Costa. Systematic use of occultationlets us observe the corona in hard X-rays.
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
25 January 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
Observations and Modelling of the 29 March 2014 X1 Flare
-- M. M. Woods, L. K. Harra, S. A. Matthews, D. H. Mackay, S. Dacie,
D. M. Long
Coronal loop seismology using damping of standing kink oscillations
by mode coupling II. additional physical effects and Bayesian
analysis
-- D. J. Pascoe, S. Anfinogentov, G. Nistico, C. R. Goddard,
and V. M. Nakariakov
Vector Magnetic Field Measurements along a Cooled Stereo-imaged
Coronal Loop
-- T.A. Schad, M.J. Penn, H. Lin, P.G. Judge
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
18 January 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
Time Evolution of Elemental Ratios in Solar Energetic Particle
events
-- P. Zelina, S. Dalla, C. M. S. Cohen, R. A. Mewaldt
Vector Magnetic Field Synoptic Charts from the Helioseismic and
Magnetic Imager (HMI)
-- Yang Liu, J. T. Hoeksema, Xudong Sun, Keiji Hayashi
Microwave radio emissions as a proxy for coronal mass ejection speed
in arrival predictions of interplanetary coronal mass ejections at
1 AU
-- Carolina Salas Matamoros, Karl-Ludwig Klein, Gerard Trottet
Magneto-static modelling from SUNRISE/IMaX: Application to an active
region observed with SUNRISE II
-- T. Wiegelmann, T. Neukirch, D.H. Nickeler, S.K. Solanki,
P. Barthol, A. Gandorfer, L. Gizon, J. Hirzberger, T.L. Riethmuller,
M. van Noort, J. Blanco Rodriguez, J. C. Del Toro Iniesta, D. Orozco
Suarez, W. Schmidt, V. Martinez Pillet, M. Knolker
Improved Determination of the Location of the Temperature Maximum
in the Corona
-- Joseph Lemaire, Koen Stegen
Data Constrained Coronal Mass Ejections in A Global Magneto-
hydrodynamics Model
-- M. Jin, W. B. Manchester, B. van der Holst, I. Sokolov, G. Toth,
R. E. Mullinix, A. Taktakishvili, A. Chulaki, and T. I. Gombosi
Chromosphere to 1 AU Simulation of the 2011 March 7th Event: A
Comprehensive Study of Coronal Mass Ejection Propagation
-- M. Jin, W. B. Manchester, B. van der Holst, I. Sokolov,
G. Toth, A. Vourlidas, C. A. de Koning, and T. I. Gombosi
An exploration of heating mechanisms in a supra-arcade plasma
sheet formed after a coronal mass ejection
-- Katharine K. Reeves, Michael S. Freed, David E. McKenzie,
Sabrina L. Savage
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
Hi Everyone,
We're trying to update the list of RHESSI-related theses prior to the
RHESSI Senior Review. Could you please let me know if you know of any
recent PhD, Master, Diploma, Bachelor, or Senior theses that use RHESSI
observations? This is what we have so far:
https://hesperia.gsfc.nasa.gov/rhessi3/news-and-resources/theses/
Also, if you know of any we've missed from earlier years, please let me
know.
Thanks,
Kim
MAX MILLENNIUM NEWS
11 January 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
Observation of a Short Period Quasi-Periodic Pulsation in Solar
X-ray, Microwave and EUV Emissions
-- Pankaj Kumar, Valery M. Nakariakov, Kyung-Suk Cho
The Width Distribution of Loops and Strands in the Solar Corona -
Are we Hitting Rock Bottom ?
-- Markus J. Aschwanden and Hardi Peter
Global Energetics of Solar Flares and CMEs: V. Energy Closure
-- Markus J. Aschwanden, Amir Caspi, Christina M.S. Cohen, Gordon
Holman, Ju Jing, Matthieu, Kretzschmar, Eduard P. Kontar,
James M. McTiernan, Richard A. Mewaldt, Aidan O'Flannagain, Ian
G. Richardson, Daniel Ryan, Harry P. Warren, Yan Xu
The role of diffusion in the transport of energetic electrons during
solar flares
-- Bian, Nicolas H., Emslie, A. Gordon, and Kontar, Eduard P.
Imaging Observations of Magnetic Reconnection in a Solar Eruptive
Flare
-- Y. Li, X. Sun, M. D. Ding, J. Qiu, E. R. Priest
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
04 January 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
Flux-Rope Twist in Eruptive Flares and CMEs: due to Zipper and
Main-Phase Reconnection
-- Eric Priest and Dana Longcope
"Dandelion" Filament Eruption and Coronal Waves Associated with a
Solar Flare on 2011 February 16
-- D.P. Cabezas, L.M. Martinez, Y.J. Buleje, M. Ishitsuka,
J.K. Ishitsuka, S. Morita, A. Asai, S. UeNo, T.T. Ishii, R. Kitai,
S. Takasao, Y. Yoshinaga, K. Otsuji, and K. Shibata
Flare-production potential associated with different sunspot groups
-- Eren, S.; Kilcik, A.; Atay, T.; Miteva, R.; Yurchyshyn, V.; Rozelot,
J. P.; Ozguc, A
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. 288, “Statistical Link Between Electrons Emitting X-rays and Type III Radio Bursts,” by Hamish Reid and Nicole Vilmer: understanding the statistical links between type III bursts and hard X-rays.
No. 289, “Syrovatskii’s ‘Constant Density’ approximation.” Remembering S. I. Syrovatskii, and noting that the relevance of his “constant density” approximation has been verified by modern high-resolution obserfvations.
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
28 December 2016
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
Stellar mixing length theory with entropy rain
-- Axel Brandenburg
Scientific considerations for future spectroscopic measurements
from space of activity on the Sun
-- Gordon D. Holman
Long-period quasi-periodic oscillations of a small-scale
magnetic structure on the Sun
-- D. Y. Kolotkov, V. V. Smirnova, P. V. Strekalova, A. Riehokainen,
and V. M. Nakariakov
Collisionless, phase-mixed, dispersive, Gaussian pulse in
transversely inhomogeneous plasma
-- D. Tsiklauri
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