MAX MILLENNIUM NEWS
26 December 2013
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
Study of Two Successive Three-Ribbon Solar Flares on 2012 July 6
-- Haimin Wang, Chang Liu, Na Deng, Zhicheng Zeng, Yan Xu, Ju Jing
and Wenda Cao
Solar Magnetized ''Tornadoes': Evidence for Rotational Motion in a
Tornado-like Prominence
-- Yang Su, Peter Gomory, Astrid Veronig, Manuela Temmer, Tongjiang
Wang, Kamalam Vanninathan, Weiqun Gan, Youping Li
Variation of the solar magnetic flux spectrum during solar cycle 23
-- Chunlan Jin & Jingxiu Wang
The behavior of transverse waves in nonuniform solar flux
tubes. II. Implications for coronal loop seismology
-- Roberto Soler, Marcel Goossens, Jaume Terradas, Ramon Oliver
Heating and Dynamics of Two Flare Loop Systems Observed by AIA and EIS
-- Y. Li, J. Qiu, M. D. Ding
Solar Cycle Variations of the Radio Brightness of the Solar Polar
Regions as Observed by the Nobeyama Radioheliograph
-- Nariaki V. Nitta, Xudong Sun, J. Todd Hoeksema, Marc L. DeRosa
Using Coronal Loops to Reconstruct the Magnetic Field of an Active
Region Before and After a Major Flare
-- A. Malanushenko, C. Schrijver, M. L. DeRosa, M. S. Wheatland
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
42. SDO observations of a flare’s coronal “implosion”
by Paulo Simões, L. Fletcher and H. Hudson (University of Glasgow) & A. Russell (University of Dundee)
The corona collapses at the start of a flare.
http://www.uksolphys.org/?p=7616
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
No. 214, "CMEs on young, solar-type stars," by Alicia Aarnio: stellar flares and CMEs behave like solar ones.
No. 215, "The HEROES Misson: High Energy Replicated Optics to Explore the Sun," by Steven Christe and Albert Shih: focusing optics to explore the high-energy Sun.
No. 216, "Flare Coronal Rain," by Hugh Hudson and Sa"m Krucker: thermal collapse seen in flare loops in a wonderful new way.
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
18 December 2013
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
Injection of thermal and suprathermal seed particles into coronal
shocks of varying obliquity
-- Battarbee, M.; Vainio, R.; Laitinen, T.; Hietala, H.
Calibrating Data from the Hinode/X-Ray Telescope and Associated
Uncertainties
-- Adam R. Kobelski, Steven H. Saar, Mark A. Weber, David E. McKenzie,
Katharine K. Reeves
Plasma radio emission from inhomogeneous collisional plasma of a
flaring loop
-- Heather Ratcliffe, Eduard. P. Kontar
Reversals of the Sun's polar magnetic fields in relation to activity
complexes and coronal holes
-- A.V. Mordvinov and S.A. Yazev
Forward-Modeling of Doppler Shifts in EUV Spectral Lines
-- Y. Taroyan, S. J. Bradshaw
Quiescent Reconnection Rate Between Emerging Active Regions and
Preexisting Field, with Associated Heating: NOAA AR 11112,
-- Tarr, L.A., Longcope, D.W., McKenzie, D.E., and Yoshimura, K.
Turbulent pitch-angle scattering and diffusive transport of
hard-X-ray producing electrons in flaring coronal loops
-- Kontar, E. P.; Bian, N. H.; Emslie, A. G.; Vilmer, N.
Observation of Heating by Flare-accelerated Electrons in a Solar
Coronal Mass Ejection
-- Lindsay Glesener, Sam Krucker, Hazel Bain, Robert Lin
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
41. Magnetic Reconnection in an X-point Collapse
by Jan Graf von der Pahlen and David Tsiklauri (Queen Mary University)
The effects of the guide-field and boundary conditions.
<http://www.uksolphys.org/?p=7423>http://www.uksolphys.org/?p=7423
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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 Eml: iain.hannah(a)glasgow.ac.uk<mailto:iain.hannah@glasgow.ac.uk>
Astronomy & Astrophysics Group, Tel: +44 (0)141 330 6427
School of Physics & Astronomy, Fax: +44 (0)141 330 5183
Kelvin Building,
University of Glasgow,
Glasgow, UK, G12 8QQ
Web: http://www.astro.gla.ac.uk/~iain/
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
MAX MILLENNIUM NEWS
11 December 2013
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
Chromospheric and Coronal Observations of Solar Flares with the
Helioseismic and Magnetic Imager
-- Juan-Carlos Martinez Oliveros, Sam Krucker, Hugh S. Hudson, Pascal
Saint-Hilaire, Hazel Bain, Charles Lindsey, Rick Bogart, Sebastien
Couvidat, Phil Scherrer, Jesper Schou
Fluctuations in the interplanetary electric potential and energy
coupling between the solar-wind and the magnetosphere
-- Badruddin and Aslam, O.P.M.
Similarities and Distinctions in Cosmic-Ray Modulation during
Different Phases of Solar and Magnetic Activity Cycles
-- Aslam, O.P.M., and Badruddin
Spoke-like differential rotation in a convective dynamo
with a coronal envelope
-- J. Warnecke, P. J. Kapyla, Maarit. J. Mantere, A. Brandenburg
A swirling flare-related EUV jet
-- Q. M. Zhang and H. S. Ji
Comparative Study of MHD Modeling of the Background Solar Wind
-- C. Gressl, A. M. Veronig, M. Temmer, D. Odstrcil, J. A. Linker,
Z. Mikic, P. Riley
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
04 December 2013
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
CME Expansion as the Driver of Metric Type II Shock Emission as
Revealed by Self-Consistent Analysis of High Cadence EUV Images and
Radio Spectrograms
-- Kouloumvakos, A.; Patsourakos, S.; Hillaris, A.; Vourlidas, A.;
Preka-Papadema, P.; Moussas, X.; Caroubalos, C.; Tsitsipis, P.;
Kontogeorgos, A.
Properties of Solar Ephemeral Regions at the Emergence Stage
-- Shuhong Yang, Jun Zhang
Statistical Properties of Super-hot Solar Flares
-- Amir Caspi, Sam Krucker, R. P. Lin
Influence of solar and cosmic-ray variablity on climate
-- Badruddin, O.P.M. Aslam and M. Singh
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