MAX MILLENNIUM NEWS
29 July 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
Cool transition region loops observed by the Interface Region Imaging
Spectrograph
-- Zhenghua Huang, Lidong Xia, Bo Li, Maria Madjarska
On the speed and acceleration of electron beams triggering
interplanetary type III radio bursts
-- Vratislav Krupar, Eduard P. Kontar, Jan Soucek, Ondrej Santolik,
Milan Maksimovic, Oksana Kruparova
LOFAR tied-array imaging and spectroscopy of solar S bursts
-- D. E. Morosan, P. T. Gallagher, P. Zucca, A. O'Flannagain, R.
Fallows, H. Reid, J. Magdalenic, G. Mann, M. M. Bisi, A. Kerdraon, A.
A. Konovalenko, A. L. MacKinnon, H. O. Rucker, B. Thide, C. Vocks, A.
Alexov, J. Anderson, A. Asgekar, I. M. Avruch, M. J. Bentum, G.
Bernardi, A. Bonafede, F. Breitling, J. W. Broderick, W. N. Brouw, H.
R. Butcher, B. Ciardi, E. de Geus, J. Eisloffel, H. Falcke, W.
Frieswijk, M. A. Garrett, J. Griessmeier, A. W. Gunst, J. W. T.
Hessels, M. Hoeft, A. Karastergiou, V. I. Kondratiev, G. Kuper,
J. van Leeuwen, D. McKay-Bukowski, J. P. McKean, H. Munk, E. Orru,
H. Paas, R. Pizzo, A. G. Polatidis, A. M. M. Scaife, J. Sluman,
C. Tasse, M. C. Toribio, R. Vermeulen, P. Zarka
Magnetic flux concentrations from dynamo-generated fields
-- Sarah Jabbari, Axel Brandenburg, Illa R. Losada, Nathan Kleeorin,
Igor Rogachevskii
A Steady-state Supersonic Downflow in the Transition Region above
a Sunspot Umbra
-- Thomas Straus and Bernhard Fleck and Vincenzo Andretta
Modeling solar coronal bright point oscillations with multiple
nanoflare heated loops
-- K Chandrashekhar, Aveek Sarkar
North-South asymmetry in the magnetic deflection of polar coronal
hole jets
-- Nistico G., Zimbardo G., Patsourakos S., Bothmer V.,
Nakariakov V. M.
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
59. Propagating Sausage Mode Waves Damping in the Chromosphere
by Samuel Grant and David Jess (Queen’s University Belfast)
ROSA observations of energy leaking from MHD waves in pores
http://www.uksolphys.org/?p=10279
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Dear All,
We invite contributions to the session (ID#: 7960) “Flare/CME Coupling from
the Corona to the Deep Solar Interior” at the Fall AGU in San Francisco,
14-18 December 2015. Details on the session follow.
We would like to remind you that the abstract submission deadline is 5
August 23:59 EDT/03:59 +1 GMT.
Abstracts can be submitted using the following link:
https://agu.confex.com/agu/fm15/sh/papers/index.cgi?sessionid=7960
Best regards,
Juan Carlos Martinez Oliveros
Hugh S Hudson
Charles A Lindsey
Angelos Vourlidas
-------------------------------------------------------------------
Session ID#: 7960
Session Description:
Flares and CMEs are two spectacular manifestations of the explosive release
of magnetic energy in the solar atmosphere. The released magnetic energy is
transformed into kinetic (CMEs) and thermal energy, (flares), and into the
injection and subsequent acceleration of particles. A zoo of wave phenomena
accompanies these events and their analysis can provide a wealth of
information about the solar atmosphere. The focus of the discussion is the
manifestation of flare- and CME-induced waves from the corona to the solar
interior and how multiwavelength observations (IRIS, SDO, RHESSI, Hinode,
NoRH, OVSA) can help our understanding of the mechanics of momentum and
energy transfer in the solar atmosphere.
Primary Convener:
Juan Carlos Martinez Oliveros, Space Sciences Laboratory, Berkeley, CA,
United States
Conveners:
Hugh S Hudson, University of California Berkeley, Berkeley, CA, United
States,
Charles A Lindsey, NorthWest Research Associates Boulder, Boulder, CO,
United States and
Angelos Vourlidas, Applied Physics Laboratory, Johns Hopkins University,
Space Department, Laurel, MD, United States
Index Terms:
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7519 Flares [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7522 Helioseismology [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
MAX MILLENNIUM NEWS
22 July 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
DESTRUCTION AND OBSERVATIONAL SIGNATURES OF SUN-IMPACTING COMETS
-- John C Brown, Robert W Carlson, Mark P Toner
Alfven wave phase mixing in flows -- why over-dense solar coronal
open magnetic field structures are cool?
-- D. Tsiklauri
CME propagation: Where does the solar wind drag take over?
-- Nishtha Sachdeva, Prasad Subramanian, Robin Colaninno,
Angelos Vourlidas
The origin of net electric currents in solar active regions
-- K. Dalmasse, G. Aulanier, P. Demoulin, B. Kliem, T. Torok,
E. Pariat
Coronal Sources of the Solar F10.7 Radio Flux
-- S. J. Schonfeld, S. M. White, C. J. Henney, C. N. Arge,
R. T. J. McAteer
Dynamics of High-Velocity Evanescent Clumps [HVECs] Emitted from
Comet C/2011 L4 as Observed by STEREO
-- Raouafi, N.-E.; Lisse, C. M.; Stenborg, G.; Jones, G. H.;
Schmidt, C. A.
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 July 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
Relationship Between Solar Wind Speed and Coronal Magnetic Field
Properties
-- Ken'ichi Fujiki, Munetoshi Tokumaru, Tomoya Iju, Kazuyuki Hakamada,
Masayoshi Kojima
Hard X-ray emitting energetic electrons and photospheric electric
currents
-- Sophie Musset, Nicole Vilmer, Veronique Bommier
A Two-ribbon White-light Flare Associated with a Failed Solar
Eruption Observed by ONSET, SDO, and IRIS
-- X. Cheng, Q. Hao, M. D. Ding, K. Liu, P. F. Chen, C. Fang,
Y. D. Liu
Parallel Evolution of Quasi-separatrix Layers and Active Region
Upflows
-- Mandrini, C. H.; Baker, D.; D?moulin, P.; Cristiani, G. D.; van
Driel-Gesztelyi, L.; Vargas Dominguez, S.; Nuevo, F. A.; Vasquez,
A. M.; Pick, M.
Collisional relaxation of electrons in a warm plasma and accelerated
nonthermal electron spectra in solar flares
-- Kontar, E. P.; Jeffrey, N. L. S.; Emslie, A. G.; Bian, N. H.
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
"A two-ribbon white-light flare associated with a failed solar eruption,” by Xin CHENG. The new ONSET facility in Yunnan observes an interesting flare event.
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 July 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
Calibration of Hinode/XRT for Coalignment
-- Yoshimura, K., McKenzie, David E.
Formation of Magnetic Flux Ropes during Confined Flaring Well Before
the Onset of a Pair of Major Coronal Mass Ejections
-- Georgios Chintzoglou, Spiros Patsourakos, Angelos Vourlidas
Optimal Electron Energies for Driving Chromospheric Evaporation in
Solar Flares
-- Reep, J.W., Bradshaw, S.J., & Alexander, D.
Confined Flares in Solar Active Region 12192 from 2014 October
18 to 29
-- Huadong Chen, Jun Zhang, Suli Ma, Shuhong Yang, Leping Li, Xin Huang,
Junmin Xiao
Are tornado-like magnetic structures able to support solar prominence
plasma?
-- M. Luna, F. Moreno-Insertis & E. Priest
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
Dear All,
We invite contributions to the session (ID#: 7960) “Flare/CME Coupling from
the Corona to the Deep Solar Interior” at the Fall AGU in San Francisco,
14-18 December 2015. Details on the session follow.
We would like to remind you that the abstract submission deadline is 5
August 23:59 EDT/03:59 +1 GMT.
Abstracts can be submitted using the following link:
https://agu.confex.com/agu/fm15/sh/papers/index.cgi?sessionid=7960
Best regards,
Juan Carlos Martinez Oliveros
Hugh S Hudson
Charles A Lindsey
Angelos Vourlidas
-------------------------------------------------------------------
Session ID#: 7960
Session Description:
Flares and CMEs are two spectacular manifestations of the explosive release
of magnetic energy in the solar atmosphere. The released magnetic energy is
transformed into kinetic (CMEs) and thermal energy, (flares), and into the
injection and subsequent acceleration of particles. A zoo of wave phenomena
accompanies these events and their analysis can provide a wealth of
information about the solar atmosphere. The focus of the discussion is the
manifestation of flare- and CME-induced waves from the corona to the solar
interior and how multiwavelength observations (IRIS, SDO, RHESSI, Hinode,
NoRH, OVSA) can help our understanding of the mechanics of momentum and
energy transfer in the solar atmosphere.
Primary Convener:
Juan Carlos Martinez Oliveros, Space Sciences Laboratory, Berkeley, CA,
United States
Conveners:
Hugh S Hudson, University of California Berkeley, Berkeley, CA, United
States,
Charles A Lindsey, NorthWest Research Associates Boulder, Boulder, CO,
United States and
Angelos Vourlidas, Applied Physics Laboratory, Johns Hopkins University,
Space Department, Laurel, MD, United States
Index Terms:
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7519 Flares [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7522 Helioseismology [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
MAX MILLENNIUM NEWS
1 July 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
Using the transit of Venus to probe the upper planetary atmosphere
-- Fabio Reale, Angelo F. Gambino, Giuseppina Micela, Antonio Maggio,
Thomas Widemann, Giuseppe Piccioni
Testing magnetic helicity conservation in a solar-like active event
-- E. Pariat; G. Valori; P. Demoulin & K. Dalmasse
An automated classification approach to ranking photospheric proxies
of magnetic energy build-up
-- A. Al-Ghraibah, L.E. Boucheron, R.T.J. McAteer
Intensity Conserving Spline Interpolation (ICSI): A New Tool for
Spectroscopic Analysis
-- J. A. Klimchuk, S. Patsourakos, D. Tripathi
Triggering an eruptive flare by emerging flux in a solar
active-region complex
-- Louis, Rohan E.; Kliem, Bernhard; Ravindra, B.; Chintzoglou, Georgios
First simultaneous observations of a near-relativistic electron
spike event by both STEREO spacecraft
-- A. Klassen, N. Dresing, R. Gomez-Herrero, B. Heber
Extreme Ultraviolet Imaging of Three-dimensional Magnetic
Reconnection in a Solar Eruption
-- J. Q. Sun, X. Cheng, M. D. Ding, Y. Guo, E. R. Priest, C. E. Parnell,
S. J. Edwards, J. Zhang, P. F. Chen, C. Fang
Performance Testing of an Off-Limb Solar Adaptive Optics System
-- G.E. Taylor, D. Schmidt, J. Marino, T.R. Rimmele, R.T.James McAteer
25 Years of Self-Organized Criticality: Numerical Detection Methods
-- R.T. James McAteer, Markus J. Aschwanden, Michaila Dimitropoulou,
Manolis K. Georgoulis, Gunnar Pruessner, Laura Morales, Jack Ireland,
Valentyna Abramenko
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