MAX MILLENNIUM NEWS
28 May 2014
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
MAGNETOACOUSTIC WAVES PROPAGATING ALONG A DENSE SLAB AND HARRIS
CURRENT SHEET AND THEIR WAVELET SPECTRA
-- Meszarosova, H., Karlicky, M., Jelinek, P., Rybak, J.
Constraining solar flare differential emission measures with EVE
and RHESSI
-- Amir Caspi, James M. McTiernan, Harry P. Warren
A Prominence Eruption Driven by Flux Feeding from Chromospheric
Fibrils
-- Quanhao Zhang, Rui Liu, Yuming Wang, Chenglong Shen, Kai Liu,
Jiajia Liu, and S. Wang
An Unorthodox X-Class Long-Duration Confined Flare
-- Rui Liu, Viacheslav S. Titov, Tingyu Gou, Yuming Wang, Kai Liu,
Haimin Wang
Plasma heating in solar flares and their soft and hard X-ray
emissions
-- Robert Falewicz
High-resolution observations of active region moss and its dynamics
-- R J Morton & J A McLaughlin
Filament eruption with apparent reshuffle of endpoints
-- Boris Filippov
Investigating the differential emission measure and energetics
of microflares with combined SDO/AIA and RHESSI observations
-- A. R. Inglis, S. Christe
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 canfield at physics.montana.edu
MAX MILLENNIUM NEWS
21 May 2014
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
Blobs in recurring EUV jets
-- Q. M. Zhang and H. S. Ji
Formation of a Double-decker Magnetic Flux Rope in the Sigmoidal
Solar Active Region 11520
-- X. Cheng, M. D. Ding, J. Zhang, X. D. Sun, Y. Guo, Y. M. Wang,
B. Kliem, Y. Y. Deng
Where is the chromospheric response to conductive energy input from a
hot pre-flare coronal loop?
-- Marina Battaglia, Lyndsay Fletcher, Paulo J. A. Simoes
Sausage oscillations of coronal plasma slabs
-- Hornsey, C., Nakariakov, V.M. and Fludra, A.
Hinode 7: Conference Summary and Future Suggestions
-- Priest, ER
A Life of Fun Playing With Solar Magnetic Fields (Special Historical
Review)
-- Priest, ER
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 canfield at physics.montana.edu
MAX MILLENNIUM NEWS
14 May 2014
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
Magneto-seismological insights into the penumbral chromosphere and
evidence for wave damping in spicules
-- R J Morton
Validation of Spherically Symmetric Inversion by Use of a Tomographic
Reconstructed Three-Dimensional Electron Density of the Solar Corona
-- Tongjiang Wang and Joseph M. Devila
MHD modeling of coronal loops: injection of high-speed chromospheric
flows
-- A. Petralia, F. Reale, S. Orlando, J. A. Klimchuk
The effect of guide-field and boundary conditions on collisionless
magnetic reconnection in a stressed X-point collapse
-- J. Graf von der Pahlen, D. Tsiklauri
3D particle-in-cell simulation of electron acceleration by Langmuir
waves in an inhomogeneous plasma
-- R. Pechhacker, D. Tsiklauri
Whistler wave generation by non-gyrotropic, relativistic, electron
beams
-- Marina Skender, David Tsiklauri
3D MHD simulation of linearly polarised Alfven wave dynamics in
Arnold-Beltrami-Childress magnetic field
-- D. Tsiklauri
H α spectroscopy and multi-wavelength imaging of a solar flare
caused by filament eruption
-- Z. Huang, M. S. Madjarska, K. Koleva, J. G. Doyle, P. Duchlev,
M. Dechev, and K. Reardon
Dynamic Evolution of an X-shaped Structure above a Trans-equatorial
Quadrupole Solar Active Region Group
-- J. Q. Sun , X. Cheng, Y. Guo , M. D. Ding, and Y. Li
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 canfield at physics.montana.edu
MAX MILLENNIUM NEWS
07 May 2014
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
Response of Hinode XRT to quiet Sun, active region and flare plasma
-- O'Dwyer B., Del Zanna, G. and Mason, H.E.
Elemental abundances and temperatures of quiescent solar active
region cores from X-ray observations
-- Del Zanna, G. and Mason, H.E.
Infrared Solar Physics
-- M Penn
Statistical relationship between the succeeding solar flares detected
by the RHESSI satellite
-- L. G. Balazs; N. Gyenge; M. B. Korsos; T. Baranyi;
E. Forgacs-Dajka; I. Ballai
3D Coronal Density Reconstruction and Retrieving the Magnetic Field
Structure during Solar Minimum
-- M. Kramar, V. Airapetian, Z. Mikic, J. Davila
Magnetic flux concentrations in a polytropic atmosphere
-- I. R. Losada, A. Brandenburg, N. Kleeorin, I. Rogachevskii
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 canfield at physics.montana.edu
MAX MILLENNIUM NEWS
30 April 2014
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 Chromospheric Jets in Sunspot Umbra
-- Yurchyshyn, V., Abramenko, V., Kosovichev, A., and Goode, P.
Comparison of Emission Properties of two Homologous Flares in AR
11283
-- Yan Xu, Ju Jing, Shuo Wang, Haimin Wang
Electric current in flares ribbons: observations and 3D standard
model
-- M. Janvier, G. Aulanier, V. Bommier, B. Schmieder, P. Demoulin,
E. Pariat
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 canfield at physics.montana.edu
46. The source of the slow solar wind revealed by heliospheric observations
by Matt Owens (University of Reading)
Heliospheric magnetic flux topology and connectivity deduced from suprathermal electrons sheds light on the slow wind formation.
http://www.uksolphys.org/?p=7936
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
UKSP Nuggets are published on a monthly basis highlighting solar physics research led from the UK.
http://www.uksolphys.org/uksp-nuggets
Iain Hannah and Lyndsay Fletcher
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Dr. Iain G. Hannah
Royal Society Research Fellow,
Astronomy & Astrophysics Group,
SUPA School of Physics & Astronomy,
Kelvin Building,
University of Glasgow,
Glasgow, UK, G12 8QQ
Web: http://www.astro.gla.ac.uk/~iain/
Eml: iain.hannah(a)glasgow.ac.uk<mailto:iain.hannah@glasgow.ac.uk>
Tel: +44 (0)141 330 6427
Fax: +44 (0)141 330 5183
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
MAX MILLENNIUM NEWS
23 April 2014
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
Fine structure of flare ribbons and evolution of electric currents
-- I.N. Sharykin, A.G. Kosovichev
Temporal Evolution of the Magnetic Topology of the NOAA Active Region
11158
-- Jie Zhao, Hui Li, Etienne Pariat, Brigitte Schmieder, Yang Guo,
Thomas Wiegelmann
A Comprehensive Method of Estimating Electric Fields from Vector
Magnetic Field and Doppler Measurements
-- Kazachenko, Maria D.; Fisher, George H.; Welsch, Brian T.
Magnetic-Reconnection Generated Shock Waves as a Driver of Surges
-- Heesu Yang, Jongchul Chae , Eun-Kyung Lim, Kyoung-Sun Lee , Hyungmin
Park , Dong-uk Song , Kyuhyoun Cho
Fast Magnetic Twister and Plasma Perturbations in a 3-D Coronal
Arcade
-- K. Murawski, A.K. Srivastava, Z. E. Musielak
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 canfield at physics.montana.edu
No. 223, "Homing in on Flare Energy," by Hugh Hudson and Ryan Milligan: representing the spectral energy distribution of a flare.
No. 224, "Abundances in Solar Flares," by Harry Warren: wrinkles in the FIP effect for flares.
No. 225: "Microwave Images of a Single-Loop Flare: Observations and Simulations," by Alexey Kuznetsov and Eduard Kontar: a flare analysis making use of the new GX Simulator modeling software.
See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets .
Older Nuggets are also available at
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
(the current series, 2008-present), and at
http://sprg.ssl.berkeley.edu/~tohban/nuggets/ (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
16 April 2014
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
Evidence of Electron Acceleration around the Reconnection X-point in
a Solar Flare
-- Noriyuki Narukage, Masumi Shimojo and Taro Sakao
On the helicity of open magnetic fields
-- Prior, C., Yeates, A. R.
The coronal energy input from magnetic braiding
-- Yeates, A.R., Bianchi, F., Welsch, B. T., Bushby, P. J.
Connecting speeds, directions and arrival times of 22 coronal mass
ejections from the Sun to 1 AU
-- C. Moestl, K. Amla, J. R. Hall, P. C. Liewer, E. M. De Jong, R. C.
Colaninno, A. M. Veronig, T. Rollett, M. Temmer, V. Peinhart, J. A.
Davies, N. Lugaz, Y. D. Liu, C.J. Farrugia, J. G. Luhmann, B. Vrsnak,
R. A. Harrison, A. B. Galvin
A Challenging Solar Eruptive Event of 18 November 2003 and the Causes
of the 20 November Geomagnetic Superstorm. III. Catastrophe of
the Eruptive Filament in a Magnetic Null Point and Formation of an
Opposite-Handedness CME
-- Uralov, A.M., Grechnev, V.V., Rudenko, G.V., Myshyakov, I.I.,
Chertok, I.M., Filippov, B.P., Slemzin, V.A.
On the variation of solar flare coronal X-ray source sizes with
energy
-- Jeffrey, Natasha L. S., Kontar, Eduard P., Bian, Nicolas H.,
Emslie, A. Gordon
Observational Evidence of Torus Instability as Trigger Mechanism
for Coronal Mass Ejections: The 2011 August 4 Filament Eruption
-- Zuccarello, F. P.; Seaton, D. B.; Mierla, M.; Poedts, S.; Rachmeler,
L. A.; Romano, P.; Zuccarello, F.
Fast magnetohydrodynamic oscillation of longitudinally inhomogeneous
prominence threads: an analogue with quantum harmonic oscillator
-- Lomineishvili, S.N., Zaqarashvili, T.V., Zhelyazkov, I. and
Tevzadze, A.G.
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 canfield at physics.montana.edu
MAX MILLENNIUM NEWS
09 April 2014
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
The Low-High-Low Trend of Type III Radio Burst Starting Frequencies
and Solar Flare Hard X-rays
-- Reid, H. A. S., Vilmer, N., Kontar, E. P.
Observations of a Hybrid Double-Streamer/Pseudostreamer in the
Solar Corona
-- Rachmeler, L. A., Platten, S. J., Bethge, C. W., Seaton, D. B.,
Yeates, A. R.
A Chain of Winking (Oscillating) Filaments Triggered by an Invisible
Extreme-Ultraviolet Wave
-- Yuandeng Shen, Kiyoshi Ichimoto, Takako T. Ishii, Zhanjun Tian,
Ruijuan Zhao, Kazunari Shibata
Coronal Condensation in Funnel Prominences as Return Flows of the
Chromosphere-Corona Mass Cycle
-- Wei Liu, Thomas E. Berger, B. C. Low
Nonlinear Force-Free Field Extrapolation of a Coronal Magnetic Flux
Rope Supporting a Large-Scale Filament from Photospheric Vector
Magnetogram
-- Chaowei Jiang, S. T. Wu, Xueshang Feng, Qiang Hu
Determination of the cross-field density structuring in coronal
waveguides using the damping of transverse waves
-- I. Arregui and A. Asensio Ramos
RATAN-600 Observations of Small Scale Structures with High Spectral
Resolution
-- V. M. Bogod, C. E. Alissandrakis, T. I. Kaltman,
S. Kh. Tokhchukova
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 canfield at physics.montana.edu