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
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> 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
MAX MILLENNIUM NEWS
27 November 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
On magnetic reconnection and flux rope topology in solar flux
emergence
-- D. MacTaggart, A.L. Haynes
Toward an Efficient Prediction of Solar Flares: Which Parameters,
and How?
-- Georgoulis, M. K.
Long-Period Oscillations of Sunspots With SOHO/MDI Data
-- Efremov Vyacheslav, Parfinenko Leonid, Solov'ev Alexandr,
Kirichek Elena
Study of the solar wind-magnetosphere coupling on different time
scales
-- Badruddin and Aslam, O.P.M.
Solar Modulation of Cosmic Rays during the Declining and Minimum
Phases of Solar Cycle 23: Comparison with Past Three Solar Cycles
-- Aslam, O.P.M., and Badruddin
Sunspot splitting triggering an eruptive flare
-- Rohan E. Louis, Klaus G. Puschmann, Bernhard Kliem, Horst
Balthasar, Carsten Denker
3D Prominence-hosting Magnetic Configurations: Creating a Helical
Magnetic Flux Rope
-- Chun Xia, Rony Keppens, Yang Guo
Probing latitudinal variations of the solar magnetic field in
cycles 21--23 by Parker's Two-Layer Dynamo Model with meridional
circulation
-- Popova E., Zharkova V. and Zharkov S.
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
20 November 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
Rossby waves and polar spots in rapidly rotating stars: Implications
for stellar wind evolution
-- Zaqarashvili, T.V., Oliver, R., Ballester, J.L., Carbonell, M.,
Khodachenko, M.L., Lammer, H., Leitzinger, M. and Odert, P.
Kelvin-Helmholtz instability of twisted magnetic flux tubes in the
solar wind
-- Zaqarashvili, T.V., V"or"os, Z. and Zhelyazkov, I.
Radio seismology of the outer solar corona
-- Zaqarashvili, T.V., Melnik, V.N., Brazhenko, A.I., Panchenko, M.,
Konovalenko, A.A., Franzuzenko, A.V., Dorovskyy, V.V., Rucker, H.O.
Torsional Alfven waves in partially ionized solar plasma: effects of
neutral helium and stratification
-- Zaqarashvili, T.V., Khodachenko, M.L. and Soler, R.
Cut-off wavenumber of Alfven waves in partially ionized plasmas of
the solar atmosphere
-- Zaqarashvili, T. V., Carbonell, M., Ballester J. L. and
Khodachenko, M. L.
Nonlinear Force-Free Extrapolation of the Coronal Magnetic Field
Based on the MHD Relaxation Method
-- S. Inoue, T. Magara, V. S. Pandey, D. Shiota, K. Kusano,
G. S. Choe and K. S. Kim
Force-free field modeling of twist and braiding-induced magnetic
energy in an active-region corona
-- Thalmann, J. K., Tiwari, S. K., Wiegelmann, T.
Bipolar magnetic structures driven by stratified turbulence with
a coronal envelope
-- J. Warnecke, I. R. Losada, A. Brandenburg, N. Kleeorin,
I. Rogachevskii
An Investigation of the CME of 3 November 2011 and its Associated
Widespread Solar Energetic Particle Event
-- A. J. Prise, L. K. Harra, S. A. Matthews, D. M. Long, A. D. Aylward
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
I am asking for your help in assessing the value of our Fermi Guest investigator project to make the Fermi GBM and LAT data readily available to the solar physics community. We are writing a follow-on proposal to continue this project, and it will be important to show how widely the Fermi solar observations are being used, and how useful the capabilities are that we are providing to access and analyze the data.
Please let me know of any use you are making of Fermi X-ray and gamma-ray observations of solar flares. Are you using or are you planning to use any of the solar-specific access and analysis tools we have provided? Here is a short description of them:
* Fermi solar flare page at
http://hesperia.gsfc.nasa.gov/fermi_solar/
* Fermi GBM Flare List at
http://hesperia.gsfc.nasa.gov/fermi/gbm/qlook/fermi_gbm_flare_list.txt
* Quick-look count-rate light curves for both the Gamma-ray Burst Monitor (GBM) NaI and BGO detectors available on the RHESSI Browser at
http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth1+qlpcr+gbmd+gbmo&da…
* LAT quick-look time lines available on the RHESSI Browser coming soon.
* Spectral analysis of GBM data in OSPEX
* Spectral analysis of LAT data in OSPEX coming soon
If you have been accessing and using Fermi data, even if it is just looking at the time lines on the RHESSI Browser, please drop me a line. Let me know how you access the data, how you have used them, and what you think of our web site and the ease of access and data analysis. Also, please include references to any use or mention of Fermi data in a presentation or publication.
Thanks for your help,
Brian
Brian R. Dennis
Solar Physics Laboratory, Code 671
Goddard Space Flight Center
Greenbelt, MD 20771
301-286-7983
brian.r.dennis(a)nasa.gov
MAX MILLENNIUM NEWS
13 November 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
Twist Accumulation and Topology Structure of a Solar Magnetic Flux
Rope
-- Y. Guo, M. D. Ding, X. Cheng, J. Zhao, E. Pariat
Magnetic reconnection: from ``open'' EUV loops to closed post-flare
ones observed by SDO
-- Jun Zhang, Shuhong Yang, Ting Li, Yuzong Zhang, Leping Li and
Chaowei Jiang
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
06 November 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
Dynamics of coronal rain and descending plasma blobs in solar
prominences: I. Fully ionised case
-- R. Oliver, R. Soler, J. Terradas, T. V. Zaqarashvili,
M. L. Khodachenko
Fast magnetoacoustic wave trains in magnetic funnels of the solar
corona
-- D. J. Pascoe, V. M. Nakariakov, and E. G. Kupriyanova
Particle Densities within the Acceleration Region of a Solar Flare
-- Sam Krucker, Marina Battaglia
Formation and Eruption of an Active Region Sigmoid: I. Study by
Nonlinear Force-Free Field Modeling
-- Chaowei Jiang, S. T. Wu, Xueshang Feng, Qiang Hu
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
40. Once in a blue-shift moon
by David Williams (MSSL/UCL)
Hinode/EIS and SDO/AIA catch an erupting filament simultaneously
http://www.uksolphys.org/?p=7233
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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/
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~