MAX MILLENNIUM NEWS
31 July 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
Photospheric Injection of Magnetic Helicity: Connectivity-based
Flux Density Method
-- K. Dalmasse, E. Pariat, P. Demoulin, G. Aulanier
Chromospheric evaporation in sympathetic coronal bright points
-- Q. M. Zhang and H. S. Ji
Diagnosing Transient Ionization in Dynamic Events
-- J.G. Doyle, A. Giunta, M.S. Madjarska, H. Summers, M. O'Mullane and A. Singh
Magnetic twist: a source and property of space weather
-- Jorn Warnecke, Axel Brandenburg, Dhrubaditya Mitra
Structure of sunspot penumbral filaments: a remarkable uniformity of properties
-- S. K. Tiwari, M. van Noort, A. Lagg, S. K. Solanki
Energetic particle cross-field propagation early in a solar event
-- T. Laitinen, S. Dalla, and M.S. Marsh
Numerical simulations of magnetoacoustic-gravity waves
in the solar coronal curved magnetic field lines structure
-- P. Jelinek, K. Murawski
Imaging coronal magnetic-field reconnection in a solar flare
-- Su, Y., Veronig, A. M., Holman, G. D., Dennis, B. R., Wang, T. J.,
Temmer, M., Gan, W. Q.
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare 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
37. What is our current understanding of solar irradiance variations?<http://www.uksolphys.org/?p=6496>
by William T. Ball (Imperial College London)
How well are we able to reproduce the observed irradiance variations of the Sun?
http://www.uksolphys.org/?p=6496
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
24 July 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
Non-symmetric magnetohydrostatic equilibria: a multigrid approach
-- D. MacTaggart, A. Elsheikh, J. A. McLaughlin and R. D. Simitev
Kelvin-Helmholtz instability of a coronal streamer
-- Li Feng, Bernd Inhester, Weiqun Gan
High Dispersion Spectroscopy of the Superflare Star KIC6934317
-- Shota Notsu, Satoshi Honda, Yuta Notsu, Takashi Nagao, Takuya Shibayama,
Hiroyuki Maehara, Daisaku Nogami, Kazunari Shibata
Production of the Extreme-Ultraviolet Late Phase of an X Class Flare
in a Three-Stage Magnetic Reconnection Process
-- Y. Dai, M. D. DIng, Y. Guo
Optimization of Curvi-Linear Tracing Applied to Solar Physics and Biophysics
-- Markus J. Aschwanden, Bart De Pontieu, and Eugene A. Katrukha
First observational application of a connectivity-based helicity flux density
-- K. Dalmasse, E. Pariat, G. Valori, P. D?moulin, L. M. Green
Coronal magnetic topology and the production of solar impulsive energetic electrons
-- C. Li, L. P. Sun, X. Y. Wang, and Y. Dai
Simulation of f-Mode Propagation Through a Cluster of Small Identical Magnetic Flux Tubes
-- K. Daiffallah
Coronal-Temperature-Diagnostic Capability of the Hinode/X-Ray Telescope
Based on Self-Consistent Calibration. II. Calibration with on-Orbit Data
-- Noriyuki Narukage, Taro Sakao, Ryouhei Kano, Masumi Shimojo,
Amy Winebarger, Mark Weber, Kathy K Reeves
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare 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
17 July 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
High Spatial Resolution Observations of Loops in the Solar Corona
-- David H. Brooks, Harry P. Warren, Ignacio Ugarte-Urra,
Amy R. Winebarger
Magnetic Field Extrapolations in the Corona: Success and Future
Improvements
-- S. Regnier
Solar Energetic Particle drifts in the Parker spiral
-- S. Dalla, M.S. Marsh, J. Kelly, T. Laitinen
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
10 July 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
Apparent Solar Tornado - Like Prominences
-- Olga Panasenco, Sara Martin, Marco Velli
The multi-thermal emission in solar active regions
-- G. Del Zanna
Determination of Stochastic Acceleration Model Characteristics in
Solar Flares
-- Qingrong Chen and Vahe' Petrosian
Cross-sectional area and intensity variations of sausage modes
-- M.G. Moreels, M. Goossens, and T. Van Doorsselaere
A Rapid, Manual Method to Map Coronal-Loop Structures of an Active
Region Using Cubic Bezier Curves and Its Applications to Misalignment
Angle Analysis
-- Gilmer A. Gary, Qiang Hu, and Jong Kwan Lee
Drift-induced perpendicular transport of Solar Energetic Particles
-- M. S. Marsh, S. Dalla, J. Kelly, and T. Laitinen
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
We are pleased to announce the release of a new EIS nugget by J. Schmelz and S. Pathak. This month we look at emission measure distributions of active region cores using EIS.
Please visit the nugget here:
http://solarb.mssl.ucl.ac.uk/SolarB/nuggets/nugget_2013july.jsp
We welcome nugget contributions from the community. Please contact Deb Baker or Lucie Green if you are interested.
--
Dr. Deb Baker
UCL – Mullard Space Science Laboratory
Email: Deborah.Baker(a)ucl.ac.uk
Tel: +44 (0) 1483 204 179
The UKSP nuggets are now 3 years old and to celebrate we collated some of the nugget stats
http://www.uksolphys.org/?p=6729
These stats also featured on a poster at the St. Andrews RAS NAM/UKSP 2013.
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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/
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
RHESSI was given an excellent rating by the Heliophysics Senior Review panel for both "overall scientific merit of the proposed extended mission" and for "Value to the Heliophysics System Observatory." The Panel recommends "the continued operation of the RHESSI extended mission," and states in its report that "RHESSI plays a unique role within the HSO, enabling system-wide studies of energy release and particle acceleration in flares/CMEs and their effects on the interplanetary medium, magnetosphere, and ITM." The full report will be put on line at
http://hesperia.gsfc.nasa.gov/rhessi2/home/mission/documents/
as soon as we receive a corrected version from NASA HQ.
Säm Krucker has been officially appointed by NASA as the RHESSI PI.
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