MAX MILLENNIUM NEWS
31 May 2017
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
Estimating Solar Flux Density at Low Radio Frequencies Using a Sky
Brightness Model
-- Divya Oberoi, Rohit Sharma and Alan E.E. Rogers
Center-to-limb observations of the Sun with ALMA
-- C. E. Alissandrakis, S. Patsourakos, A. Nindos, T. S. Bastian
Increase in the amplitude of line-of-sight velocities of the
small-scale motions in a solar filament before eruption
-- Daikichi Seki, Kenichi Otsuji, Hiroaki Isobe, Takako T. Ishii,
Takahito Sakaue, Kumi Hirose
Observing the Sun with the Atacama Large Millimeter-submillimeter
Array (ALMA): Fast-Scan Single-Dish Mapping
-- S.M. White, K. Iwai, N.M. Phillips, R.E. Hills, A. Hirota,
P. Yagoubov, G. Siringo, M. Shimojo, T.S. Bastian, A.S. Hales,
T. Sawada, S. Asayama, M. Sugimoto, R.G. Marson, W. Kawasaki,
E. Muller, T. Nakazato, K. Sugimoto, R. Brajsa, I. Skokic,
M. Barta, S. Kim, A.J. Remijan, I. de Gregorio, S.A. Corder,
H.S. Hudson, M. Loukitcheva, B. Chen, B. De Pontieu,
G.D. Fleishmann, D.E. Gary, A. Kobelski, S. Wedemeyer, Y. Yan
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 richard.canfield at montana.edu
No. 301, “Double Coronal X-ray and Microwave Sources Associated with a Magnetic Breakout Solar Eruption,” by Yao CHEN: a different explanation of the double coronal hard X-ray sources.
No. 300, “A Lasso Model for Solar Gamma-ray Events,” by Hugh Hudson: a toy model hoping to explain the SEP/LAT relationship.
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
24 May 2017
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
Origin and Structures of Solar Eruptions I: Magnetic Flux Rope
(Invited Review)
-- X. Cheng, Y. Guo, M. D. Ding
JHelioviewer - Time-dependent 3D visualisation of solar and
heliospheric data
-- D. Mueller, B. Nicula, S. Felix, F. Verstringe, B. Bourgoignie,
A. Csillaghy, D. Berghmans, P. Jiggens, J. P. Garcia-Ortiz,
J. Ireland, S. Zahniy, B. Fleck
Acceleration and Propagation of Solar Energetic Particles
-- Karl-Ludwig Klein and Silvia Dalla
The First ALMA Observation of a Solar Plasmoid Ejection from an
X-ray Bright Point
-- M. Shimojo, H. S. Hudson, S. M. White, T. S. Bastian, K. Iwai
Observing the Sun with Atacama Large Millimeter/submillimeter Array
(ALMA): High Resolution Interferometric Imaging
-- M. Shimojo, T.S. Bastian, A.S. Hales, S.M. White, K. Iwai,
R.E. Hills, A. Hirota, N.M. Phillips, T. Sawada, P. Yagoubov,
G. Siringo, S. Asayama, M. Sugimoto, R. Brajsa, I. Skokic, M. Barta,
S. Kim, I. de Gregorio, S.A. Corder, H.S. Hudson, S. Wedemeyer,
D.E. Gary, B. De Pontieu, M. Loukitcheva, G.D. Fleishman, B. Chen,
A. Kobelski, Y. Yan
Exoplanet Predictions Based on Harmonic Orbit Resonances
-- Markus J. Aschwanden and Felix Scholkmann
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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
18 May 2017
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 a role of quadruple component of magnetic field in defining
solar activity in grand cycles
-- Popova, E., Zharkova V.V., Shepherd S.J. and Zharkov S.I.
CME dynamics using STEREO & LASCO observations: the relative
importance of Lorentz forces and solar wind drag
-- Nishtha Sachdeva, Prasad Subramanian, Angelos Vourlidas,
Volker Bothmer
Impulsive plasma outflows due to wave driven magnetic reconnection
-- Yamini K. Rao, A.K. Srivastava, J.G. Doyle and Bhola N. Dwivedi
Propagation of Torsional Alfven Waves from the Photosphere to the
Corona: Reflection, Transmission, and Heating in Expanding Flux Tubes
-- R. Soler, J. Terradas, R. Oliver, J. L. Ballester
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 richard.canfield at montana.edu
“A Lasso Model for Solar Gamma-Ray Events,” by Hugh Hudson. Retracting large-scale coronal magnetic fields can trap SEP particles to support a long-duration gamma-ray 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
10 May 2017
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
Plasma parameters and geometry of cool and warm active region loops
-- Haixia Xie, Maria S. Madjarska, Bo Li, Zhenghua Huang, Lidong Xia,
Thomas Wiegelmann, Hui Fu, Chaozhou Mou
Explosive chromospheric evaporation driven by nonthermal electrons
around one footpoint of a solar flare loop
-- Li, Dong; Ning, Zongjun; Huang, Yu; Zhang, Qingmin
Nonlinear evolution of short-wavelength torsional Alfven waves ?
-- S.V. Shestov and V. M. Nakariakov and A. S. Ulyanov and A. A. Reva
and S. V. Kuzin
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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
03 May 2017
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
Siberian Radioheliograph: First Results
-- S.V. Lesovoi, A.T. Altyntsev, A.A. Kochanov, V.V. Grechnev,
A.V. Gubin, D.A. Zhdanov, E.F. Ivanov, A.M. Uralov, L.K. Kashapova,
A.A. Kuznetsov, N.S. Meshalkina, R.A. Sych
Two Step Filament Eruption During 14-15 March 2015
-- R. Chandra, B. Filippov, R. Joshi, B. Schmieder
Magnetic nulls and super-radial expansion in the solar corona
-- Sarah E. Gibson, Kevin Dalmasse, Laurel A. Rachmeler, Marc L.
De Rosa, Steven Tomczyk, Giuliana de Toma, Joan Burkepile,
Michael Galloy
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 richard.canfield at montana.edu
No. 297: "Multi-Instrument Solar Flare Observations I: Solar Flare Finder," by Ryan Milligan. Retrospective searches for your favorite flare
No. 298: "Multi-Instrument Solar Flare Observations II: A SC24 Retrospective," by Ryan Milligan and Jack Ireland. How the widget did in Cycle 24
No. 299: "High Resolution Temporal and Spatial Structure of a White Light Flare," by Vasyl Yurchyshyn. The biggest solar telescope finds still smaller scales for white-light flare kernels
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
26 April 2017
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
Evidence for two-loop interaction from IRIS and SDO observations
of penumbral brightenings
-- C. E. Alissandrakis, A. Koukras, S. Patsourakos, A. Nindos
Coronal cavities: observations and implications for the magnetic
environment of prominences
-- Sarah E. Gibson
A parameter study for modeling MgII h and k emission during solar
flares
-- F. Rubio da Costa; L. Kleint
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 richard.canfield at montana.edu
Dear solar X-ray colleagues,
REMINDER: the deadline to register and submit abstracts is April 22, in just one week! I heartily encourage and invite you to attend this joint meeting.
Registration and abstract submission are NOW OPEN for the RHESSI 16th Workshop, co-hosted with the MinXSS 1st Workshop, to be held at the University of Colorado in Boulder, CO, USA from June 19 to 24, 2017. The workshop website, https://rhessi16.boulder.swri.edu, includes registration and abstract information, as well as logistical (travel, hotels, etc.) information. Anyone with an interest in high-energy solar physics is invited to attend.
Registration and abstracts are due April 22. The registration fee of $325 includes the entire week of the workshop. There is no separate abstract fee. The Welcome Reception, Banquet dinner, and all morning and afternoon coffee breaks are free to registered attendees. Companion tickets are available.
Specially-priced room blocks are available at selected Boulder hotels until May 18.
The workshop format will be a blend of plenaries at the beginning and end, with various topical working group sessions in between, covering a range of high-energy solar physics topics including acceleration and transport of electrons and ions, the solar atmospheric response to energy release (including thermal plasma), multi-wavelength observations (EUV, radio, etc.), and pertinent theory. There will also be sessions on next steps in RHESSI imaging; the MinXSS CubeSat status and data access; new results from MinXSS-1 on flare thermal emission and quiescent soft X-ray emission; and a discussion of future instrumentation.
The final science program will be determined based on your contributed abstracts, so please submit a presentation and help guide the scientific goals of this event.
Please feel free to contact me directly if you have any questions about the workshop.
We look forward to seeing you all in Boulder this June!
On behalf of the Local Organizing Committee,
--- Amir, LOC chair
amir(a)boulder.swri.edu
+1-303-546-6351