MAX MILLENNIUM NEWS
11 April 2012
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
4pi Models of CMEs and ICMEs -- Kleimann, J.
Observations of Multiple Surges Associated with Magnetic Activities
in AR10484 on 25 October 2003 -- Wahab Uddin, B. Schmieder, R. Chandra,
Abhishek K. Srivastava, Pankaj Kumar, S. Bisht
Growing transverse oscillations of a multistranded loop observed by SDO/AIA
-- Tongjiang Wang, Leon Ofman, Joseph M. Davila, Yang Su
Flows at the Edge of an Active Region: Observation and Interpretation
-- C. Boutry, E. Buchlin, J.-C. Vial, S. Regnier
Numerical simulations of chromospheric hard X-ray source sizes in solar flares
-- M. Battaglia, E. P. Kontar, L. Fletcher, A. L. MacKinnon
Observation of Ultrafine Channels of Solar Corona Heating
-- Haisheng Ji, Wenda Cao, Philip R. Goode
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
4 April 2012
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 of Low Frequency Solar Radio Bursts from the Rosse
Solar-Terrestrial Observatory -- P. Zucca, E. P. Carley, J. McCauley,
P. T. Gallagher, C. Monstein, R. T. J. McAteer
Effect of Solar Wind Drag on the Determination of the Properties of
Coronal Mass Ejections from Heliospheric Images -- N. Lugaz and P. Kintner
Generation of Quasi-periodic Waves and Flows in the Solar Atmosphere
by Oscillatory Reconnection -- McLaughlin, J. A., Verth, G., Fedun, V.,
Erdelyi, R.
Energetic Particle Diffusion In Structured Turbulence -- Laitinen, T.,
Dalla, S. and Kelly, J.
Scale-dependence of magnetic helicity in the solar wind -- Brandenburg, A.,
Subramanian, K., Balogh, A., & Goldstein, M. L.
Multi-spacecraft Study of the 8 November 2000 SEP Event: Electron
Injection Histories 100 Degrees Apart -- N. Agueda, D. Lario, V. Ontiveros,
E. Kilpua, B. Sanahuja and R. Vainio
Multiwavelength Observations of Supersonic Plasma Blob Triggered by
Reconnection Generated Velocity Pulse in AR10808 -- A.K. Srivastava,
R Erdelyi, K. Murawski, P. Kumar
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
From: Gopalswamy, Natchimuthuk (GSFC-6710)
Sent: Thursday, March 29, 2012 1:40 PM
To: larry.paxton(a)jhuapl.edu; Dennis, Brian R. (GSFC-6710); Pfaff, Robert F. (GSFC-6740); Macdowall, Robert J. (GSFC-6950)
Subject: SOMCOSE campaign please circulate
SCOSTEP Observing and Modeling Campaign On Space Weather Events (SOMCOSE)
Active region NOAA 1429 is returning on the east limb of the Sun. This region produced one of the two biggest space weather events of solar cycle 24. An observing campaign known as SCOSTEP Observing and Modeling Campaign On Space Weather Events (SOMCOSE) has been initiated to track this region for a month, starting March 29, 2012. Observations made during its previous disk passage also will be used for further studies. The campaign is conducted under the aegis of the Scientific Committee on Solar Terrestrial Physics (SCOSTEP, see www.yorku.ca/scostep<http://www.yorku.ca/scostep>). The campaign is to observe, track, model and analyze the space weather impacts of all the solar events that happen during the interval. Observations can start right away. RHESSI, SOHO, STEREO, SDO, Wind, ACE, TIMED, CNOFS, and ground observation networks will take data during this interval. Note that the list is not inclusive. Modelers can do real time prediction as well as do post-campaign analysis. Results can be submitted to the International Symposium on Solar Terrestrial Physics (ISSTP 2012), Fall AGU and the CAWSES Symposium 2013 in Nagoya.
If you are interested in participating in the campaign, please contact nat.gopalswamy(a)nasa.gov<mailto:nat.gopalswamy@nasa.gov> or shibata(a)kwasan.kyoto-u.ac.jp<mailto:shibata@kwasan.kyoto-u.ac.jp>. Thanks!
Nat Gopalswamy
MAX MILLENNIUM NEWS
28 March 2012
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
Off-limb (spicule) DEM distribution from SoHO/SUMER observations
-- K. Vanninathan, M. S. Madjarska, E. Scullion, J. G. Doyle
Time delays in quasi-periodic pulsations observed during the X2.2 solar
flare on 2011 February 15
-- L. Dolla, C. Marqu?, D. B. Seaton, T. Van Doorsselaere,
M. Dominique, D. Berghmans, C. Cabanas, A. De Groof, W. Schmutz, A. Verdini,
M. J. West, J. Zender and A. N. Zhukov
The Solar Flare Sulphur Abundance from RESIK Observations
-- J. Sylwester, B. Sylwester, K. J. H. Phillips, V. D. Kuznetsov
Large amplitude longitudinal oscillations in a solar filament
-- Manuel Luna, Judith Karpen
H-alpha counterparts of X-ray bright points in the solar atmosphere
-- Ping Zhang, Cheng Fang, Qingmin Zhang
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
21. Plasma parameters in eruptive prominences from SDO/AIA observations
by Kristopher McGlinchey and Nicolas Labrosse, University of Glasgow
Non-LTE radiative transfer models help us to understand intensity
variations observed by SDO/AIA in prominence eruptions
http://www.uksolphys.org/?p=4247
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
UKSP Nuggets are published on a monthly basis highlighting solar physics
research in the UK.
http://www.uksolphys.org/uksp-nuggets
Iain Hannah and Lyndsay Fletcher
--
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Dr. Iain G. Hannah Eml: iain.hannah(a)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, Scotland, UK
G12 8QQ Web: http://www.astro.gla.ac.uk/~iain/
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
MAX MILLENNIUM NEWS
21 March 2012
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
The role of Rayleigh-Taylor instabilities in filament threads
-- J. Terradas, R. Oliver, J. L. Ballester
Observation of An Evolving Magnetic Flux Rope Prior To and During
A Solar Eruption -- J. Zhang, X. Cheng, and M. D. Ding
Comparison of Line-of-Sight Magnetograms Taken by the Solar Dynamics
Observatory/Helioseismic and Magnetic Imager and Solar and Heliospheric
Observatory/Michelson Doppler Imager -- Y. Liu, J.T. Hoeksema, P.H. Scherrer,
J. Schou, S. Couvidat, R.I. Bush, T.L.Duvall Jr, K. Hayashi, X. Sun, X. Zhao
Magneto-Acoustic Energetics Study of the Seismically Active Flare of
15 February 2011 -- J.D. Alvarado-G?mez, J.C. Buitrago-Casas,
J.C. Mart?nez-Oliveros, C. Lindsey, H. Hudson, B. Calvo-Mozo
Morphological evolution of a 3D CME cloud reconstructed from three viewpoints
-- L. Feng, B. Inhester, Y. Wei, W.Q. Gan, T.L. Zhang, M.Y. Wang
Inversion of physical parameters in solar atmospheric seismology
-- I. Arregui
A multiwavelength study of an M-class flare and the origin of an associated
eruption from NOAA AR 11045 -- Dwivedi, B. N.; Srivastava, Abhishek K.;
Kumar, Mukul; Kumar, Pankaj
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
14 March 2012
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
Rapid Transition of Uncombed Penumbrae to Faculae during Large Flares
-- Haimin Wang, Na Deng, Chang Liu
Helioseismic Detection of Emerging Magnetic Flux -- Stathis Ilonidis,
Junwei Zhao, Alexander G. Kosovichev
Initiation and Development of the white-light and radio CME on 15 April 2001
-- P. Demoulin, A. Vourlidas, M. Pick, A. Bouteille
Systematic Center-to-Limb Variation in Measured Helioseismic Travel Times
and Its Effect on Inferences of Solar Interior Meridional Flows
-- Junwei Zhao, Kaori Nagashima, R. S. Bogart, A. G. Kosovichev, T. L. Duvall Jr
The Occurrence and Speed of CMEs Related to Two Characteristic
Evolution Patterns of Helicity Injection in Their Solar Source Regions
-- Sung-Hong Park, Kyung-Suk Cho, Su-Chan Bong, Pankaj Kumar,
Jongchul Chae, Rui Liu, Haimin Wang
Chromospheric Magnetic Field Measurements in a Flare and
an Active Region Filament -- Harvey, J.W.
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