MAX MILLENNIUM NEWS
29 April 2015
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 flare predictability based on sunspot group evolution
-- Marianna Korsos, Andras Ludmany, Robert Erdelyi, Tunde Baranyi
How are Forbush decreases related with interplanetary magnetic
field enhancements?
-- K. P. Arunbabu, H. M. Antia, S. R. Dugad, S. K. Gupta, Y. Hayashi,
S. Kawakami, P. K. Mohanty, A. Oshima, P. Subramanian
Correcting for interplanetary scattering in velocity
dispersion analysis of solar energetic particles
-- T. Laitinen, K. Huttunen-Heikinmaa, E. Valtonen, S. Dalla
Magnetohydrodynamic shocks in and above post-flare loops:
two-dimensional simulation and a simplified model
-- Shinsuke Takasao, Takuma Matsumoto, Naoki Nakamura, and Kazunari
Shibata
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
57. First direct measurements of transverse waves in solar polar plumes using SDO/AIA
by Jonathan Thurgood (Queen Mary University of London) & Richard Morton, James McLaughlin (Northumbria University)
AIA observations of kink waves in coronal holes suggest they can't accelerate the fast solar wind.
http://www.uksolphys.org/?p=9993
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
“Ionospheric Effects, Flare History, and Dick Donnelly,” by Hugh Hudson and Peter Gallagher: Recogning the world’s largest X-ray detector, its ionosphere.
See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series, 2008-present, and
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
for 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
22 April 2015
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
Onset of the Kelvin-Helmholtz instability in partially ionized
magnetic flux tubes
-- David Martinez-Gomez, Roberto Soler and Jaume Terradas
Analysis of a Coronal Mass Ejection and a Co-rotating Interaction
Region as they travel from the Sun, passing Venus, Earth, Mars
and Saturn
-- A. J. Prise, L. K. Harra, S. A. Matthews, C. S. Arridge,
N. Achilleos
Additional acceleration of solar-wind particles in current sheets
of the heliosphere
-- Zharkova V.V. and Khabarova O.
Why Is the Great Solar Active Region 12192 Flare-Rich But CME-Poor?
-- Xudong Sun, Monica Bobra, Todd Hoeksema, Yang Liu, Yan Li, Chenglong
Shen, Sebastien Couvidat, Aimee Norton, George Fisher
Ensemble modeling of CMEs using the WSA-ENLIL+Cone model
-- M. L. Mays, A. Taktakishvili, A. A. Pulkkinen, D. Odstrcil, P.
J. MacNeice, L. Rastaetter, J. A. LaSota, Y. Zheng, M. M. Kuznetsova
Fast single-dish scans of the Sun using ALMA
-- Neil Phillips, Richard Hills, Tim Bastian, Hugh Hudson, Ralph
Marson, and Sven Wedemeyer
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
15 April 2015
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
Oscillating light wall above a sunspot light bridge
-- Shuhong Yang, Jun Zhang, Fayu Jiang, Yongyuan Xiang
Magnetic Energy Dissipation during the 2014 March 29 Solar Flare
-- Markus J. Aschwanden
Direct Spatial Association of an X-Ray Flare with the Eruption
of a Solar Quiescent Filament
-- Gordon D. Holman & Adi Foord
Alfven instability of steady state flux tubes II.
Upflows in stratified atmospheres
-- Y. Taroyan
Stopping frequency of type III solar radio bursts
in expanding magnetic flux tubes
-- Hamish A. S. Reid & Eduard P. Kontar
A Scenario for the Fine Structures of Solar Type IIIb Radio Bursts
Based on the Electron Cyclotron Maser Emission
-- C. B. Wang
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
“RHESSI Detection of X-ray Emission from a Quiet-Sun Filament Eruption,” by Gordon Holman and Adi Foord: A RHESSI flare is detected outside an active region.
See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series, 2008-present, and
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
for 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
8 April 2015
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
Kinematics of ICMEs/Shocks: Blast Wave Reconstruction Using Type-II Emissions
-- P. Corona-Romero, J.A. Gonzalez-Esparza, E. Aguilar-Rodriguez, V. De-la-Luz,
J.C. Mejia-Ambriz
Quasi-periodic Slipping Magnetic Reconnection During an X-class Solar Flare
Observed by the Solar Dynamics Observatory and Interface Region Imaging
Spectrograph
-- Ting Li, Jun Zhang
Filament Activation in Response to Magnetic Flux Emergence and Cancellation
in Filament Channels
-- Ting Li, Jun Zhang, Haisheng Ji
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
1 April 2015
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 the Statistical Relationship between CME Speed and Soft X-ray Flux
and Fluence of the Associated Flare
-- C. Salas Matamoros, K.-L. Klein
Intensity and Doppler Velocity Oscillations in Pore Atmospheres
-- Cho, K.-S., Bong, S.-C., Nakariakov, V. M., Lim, E.-K., Park, Y.-D.,
Chae, J. C., Yang, H.-S., Park, H.-M., Yurchyshyn, V.
Dissipative instability in partially ionised prominence plasmas
-- I. Ballai, R. OIiver, M. Alexandrou
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