MAX MILLENNIUM NEWS
02 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
Advances in Observing Various Coronal EUV Waves in the SDO Era
and Their Seismological Applications (Invited Review)
-- Wei Liu, Leon Ofman
Anomalous Expansion of Coronal Mass Ejections during Solar Cycle 24
and its Space Weather Implications
-- Nat Gopalswamy, Sachiko Akiyama, Seiji Yashiro, Hong Xie, and
Pertti Makela, Grzegorz Michalek
The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field
Pipeline: SHARPs - Space-weather HMI Active Region Patches
-- Monica Bobra, X. Sun, J.T. Hoeksema, M. Turmon, Y Liu, K. Hayashi,
G. Barnes, K.D. Leka
Compound Effect of Alfven Waves and Ion-cyclotron Waves on
Heating/Acceleration of Minor Ions via the Pickup Process
-- Wang, C.B.; Bin Wang; L. C. Lee
CorPITA: An Automated Algorithm for the Identification and Analysis
of Coronal "EIT Waves"
-- David M. Long, D. Shaun Bloomfield, Peter T. Gallagher, David
Perez-Suarez
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
45. A new approach to unveil the shape of interplanetary structures
by Miho Janvier (University of Dundee), Pascal Démoulin (Observatoire de Paris) & Sergio Dasso (IAFE-DF-DCAO)
How local in situ data can still reveal the mean shape of interplanetary structures.
http://www.uksolphys.org/?p=7933
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
No. 220, "A Wonderful Cycle 24 Flare," by Sa"m Krucker: There have been quite a few Cycle 24 X-class flares, but this was one of the nicest.
No. 221, "Imaging Quasi-Periodic Fluctuations in a Simple Flare," by Zhongjun Ning: Time-series spectroscopy in a B8 flare.
No. 222, "Empirical Constructs and Cartoons," by Forrest Mozer. How our mental images may relate to what's really going on.
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
26 March 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
Differential Emission Measure Analysis of A Limb Solar Flare on
2012 July 19
-- J. Q. Sun, X. Cheng, M. D. Ding
Observations of linear polarization in a solar coronal loop
prominence system near 6173 A
-- Pascal Saint-Hilaire, Jesper Schou, Juan-Carlos Martinez Oliveros,
Hugh S. Hudson, Sam Krucker, Hazel Bain, Sebastien Couvidat.
25 Years of Self-Organized Criticality: Solar and Astrophysics
-- Aschwanden, M.J., Crosby, N., Dimitropoulou, M., Geogoulis, M.K.,
Hergarten, S., McAteer, J., Milovanov, A.V., Mineshige, S., Morales,
L., Nishizuka, N., Pruessner, G., Sanchez, R., Sharma, S., Strugarek,
A., and Uritsky, V.
Magnetic helicity and energy spectra of a solar active region
-- Hongqi Zhang, Axel Brandenburg, D.D. Sokoloff
The formation heights of coronal shocks from 2D density and Alfven
speed maps
-- Pietro Zucca, Eoin P. Carley, D. Shaun Bloomfield, Peter T. Gallagher
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
19 March 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
Deciphering Solar Magnetic Activity I: On The Relationship Between
The Sunspot Cycle And The Evolution Of Small Magnetic Features
-- Scott W. McIntosh, Xin Wang, Robert J. Leamon, Alisdair R. Davey,
Rachel Howe, Larisza D. Krista, Anna V. Malanushenko, Jonathan
W. Cirtain, Joseph B. Gurman, Michael J. Thompson
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
12 March 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
Solar Energetic Particle Events in the 23rd Solar Cycle:
Interplanetary Magnetic Field Configuration and Statistical
Relationship with Flares and CMEs
-- Miteva, R.; Klein, K.-L.; Malandraki, O.; Dorrian, G.
Radio Signatures of Solar Energetic Particles During the 23rd Solar
Cycle
-- Miteva, R.; Klein, K.-L.; Samwel, S. W.; Nindos, A.; Kouloumvakos,
A.; Reid, H.
Thermal structure of hot non-flaring corona from Hinode/EIS
-- A. Petralia, F. Reale, P. Testa, G. Del Zanna
Evolution of Magnetic Flux Rope and Its Overlying Arcade Based on
Nonlinear Force-free Field Extrapolations
-- Ju Jing, Chang Liu, Jeongwoo Lee, Shuo Wang, Thomas Wiegelmann,
Yan Xu, and Haimin Wang
Two Sun-like Superflare Stars Rotating as Slow as the Sun
-- Daisaku Nogami, Yuta Notsu, Satoshi Honda, Hiroyuki Maehara, Shota
Notsu, Takuya Shibayama, Kazunari Shibata
The Evolution of Writhe in Kink-Unstable Flux Ropes and Erupting
Filaments
-- Tibor Torok, Bernhard Kliem, Mitchell A. Berger, Mark G. Linton,
Pascal Demoulin, Lidia van Driel-Gesztelyi
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
05 March 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
Observations and Implications of Large-Amplitude Longitudinal
Oscillations in a Solar Filament
-- M. Luna, K. Knizhnik, K. Muglach, J. Karpen, H. Gilbert,
T.A. Kucera, V. Uritsky
Energy and helicity budgets of solar quiet regions
-- Tziotziou, K., Tsiropoula, G., Georgoulis, M.K., Kontogiannis, I.
New Vacuum Solar Telescope observations of a flux rope tracked by
a filament activation
-- Shuhong Yang, Jun Zhang, Zhong Liu, Yongyuan Xiang
Asymmetry in the CME-CME interaction process for the events from 2011
February 14-15
-- M. Temmer, A. M. Veronig, V. Peinhart, B. Vrsnak
Rayleigh-Taylor instabilities with sheared magnetic fields
-- Ruderman, M. S., Terradas, J., Ballester, J. L.
The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field
Pipeline: Overview and Performance
-- J.T. Hoeksema, Y. Liu, K. Hayashi, X. Sun, J. Schou, S. Couvidat,
A. Norton, M. Bobra, R. Centeno, K.D. Leka, G. Barnes, M. Turmon
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
New HMI Science Nuggets are available at
http://hmi.stanford.edu/hminuggetsfeaturing
#1 "Evidence of Double-cell Meridional Circulation inside the Sun"
contributed by Junwei Zhao
Acoustic travel time reveals an equatorward meridional flow in the middle
of the solar convection zone. Inversion reveals an evidence of double-cell
meridional circulation inside the Sun.
We invite those who use HMI data for their research, or whose research is
closely related to HMI science objectives, to contribute to the HMI science
nuggets. -- SDO/HMI team
>
New HMI Science Nuggets are available at http://hmi.stanford.edu/hminuggets,
featuring the following topic
#2 "Testing Hemispheric Rule of Helicity with HMI Data" contributed by Yang
Liu
Hemispheric helicity preference in groups of active regions with different
properties suggests different origins of magnetic twist.
We invite those who use HMI data for their research, or whose research is
closely related to HMI science objectives, to contribute to the HMI science
nuggets. -- SDO/HMI team
New HMI Science Nuggets are available at http://hmi.stanford.edu/hminuggets,
featuring the following topic
#3 "The Biggest Sunspots Produced by Cycle 24" contributed by Aimee Norton
Even though Solar Cycle 24 is weak, it has still produced some large
sunspots. We list the largest sunspots as observed by HMI and discuss some
aspects of the data.
We invite those who use HMI data for their research, or whose research is
closely related to HMI science objectives, to contribute to the HMI science
nuggets. -- SDO/HMI team