Dear All,
We invite contributions to the session (ID#: ST27) “New Insights Into The
Physics Of White-light Flares” at the AOGS meeting in Beijing, 31 Jul to
5 Aug, 2016. Details on the session follow.
We would like to remind you that the abstract submission deadline is 19
February 2016.
Abstracts can be submitted using the following link:
http://www.asiaoceania.org/aogs2016/public.asp?page=abstract.htm
Best regards,
Juan Carlos Martinez Oliveros
Hugh S Hudson
Lucia Kleint
Mingde Ding
---------------------------------------------
Session Title:
New Insights Into The Physics Of White-light Flares
Session Description:
The white-light continuum of a solar flare was the first manifestation of a
flare ever detected, and this continuum emission contains a large fraction
of the total luminous energy of a flare. Thus its identification has always
posed an important problem for solar and stellar physics. A zoo of
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 in the visible continuum of flares, from the corona to
the solar interior and how multi wavelength observations (RHESSI, IRIS,
SDO, Hinode, infrared, NoRH, OVSA) can help our understanding of the
mechanics of momentum and energy transfer in the solar atmosphere.
MAX MILLENNIUM NEWS
27 January 2016
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
Coronal Magnetic Fields Derived from Simultaneous Microwave and
EUV Observations and Comparison with the Potential Field Model
-- S. Miyawaki, K. Iwai, K. Shibasaki, D. Shiota, and S. Nozawa
Ultra-narrow Negative Flare Front Observed in Helium-10830 A using
the 1.6 m New Solar Telescope
-- Yan Xu, Wenda Cao, Mingde Ding, Lucia Kleint, Jiangtao Su,
Chang Liu, Haisheng Ji, Jongchul Chae, Ju Jing, Kyuhyoun Cho,
Kyungsuk Cho, Dale Gary, and Haimin Wang
The Impact of the Revised Sunspot Record on Solar Irradiance
Reconstructions
-- G. Kopp, N. Krivova, J. Lean, and C.J. Wu
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
The next RHESSI Workshop (number XV in the series) will be held in Graz,
Austria, from July 26-30, 2016.
This workshop is now open for registration/abstract submission
athttp://rhessi15.uni-graz.at/en/ <http://rhessi15.uni-graz.at/en/>
This workshop will consist of a blend of plenary sessions (at the
beginning and end), with topical sessions in between.
Topics include integration of RHESSI and IRIS observations, analysis of
RHESSI/Fermi data, the SXR
and EUV response of the solar atmosphere to flare heating, joint
radio/HXR studies, next steps in RHESSI imaging,
and theory and modeling of flare processes.
<http://rhessi15.uni-graz.at/en/>
MAX MILLENNIUM NEWS
20 January 2016
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 multiple blobs in homologous solar coronal jets in
closed loops
-- Q. M. Zhang, H. S. Ji, and Y. N. Su
Intense bipolar structures from stratified helical dynamos
-- Dhrubaditya Mitra, A. Brandenburg, N. Kleeorin, I. Rogachevskii
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
13 January 2016
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
Radiative transfer in cylindrical threads with incident radiation
VII. Multi-thread models
-- N. Labrosse and A.S. Rodger
Sources of Quasi-Periodic Pulses in the 18 August 2012 Flare
-- A. Altyntsev, N. Meshalkina, H. Meszarosova, M. Karlicky,
V. Palshin, S. Lesovoi
Alfvenic Wave Heating of the Upper Chromosphere in Flares
-- Reep, J.W., & Russell, A.J.B.
Thermal and non-thermal emission from reconnecting twisted coronal
loops
-- R. F. Pinto, M. Gordovskyy, P.K. Browning and N. Vilmer
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
64. 3D Electron Density Distributions in the Solar Corona during Solar Minimum
by Judith de Patoul and Claire Foullon (Exeter) and Pete Riley (Predictive Science)
A new tomographic method promises better solar wind models
http://www.uksolphys.org/?p=10950
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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#: ST26) “Multiwavelength and
In-situ Observations of CME and Flare Evolution and Dynamics” at the
AOGS meeting
in Beijing from July 31 to August 5, 2016. Details on the session follow.
We would like to remind you that the abstract submission deadline is 19
February 2016.
Abstracts can be submitted using the following link:
http://www.asiaoceania.org/aogs2016/public.asp?page=abstract.htm
Best regards,
Juan Carlos Martinez Oliveros
Ying Liu
Hazel Bain
David Sundkvist
---------------------------------------------
Session Title:
*Multiwavelength and In-situ Observations Of CME and Flare Evolution and
Dynamics*
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 and thermal energy and radiations. The focus of
this session is to discuss how multi-wavelength observations and in situ
measurements from current (IRIS, SDO, RHESSI, Hinode, NoRH, NRH, OVSA,
STEREO, Wind, ACE) and future (Solar Orbiter, Solar Probe Plus) instruments
and theoretical modeling can help our understanding of the mechanics,
dynamics and evolution of these phenomena in the corona and interplanetary
space.
MAX MILLENNIUM NEWS
06 January 2016
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
Injection of solar energetic particles into both loop legs of a
magnetic cloud
-- Nina Dresing, Raul Gomez-Herrero, Bernd Heber, Miguel Angel Hidalgo,
Andreas Klassen, Manuela Temmer, Astrid Veronig
X-ray Source Heights in a Solar Flare: Thick-target versus Thermal
Conduction Front Heating
-- Reep, J.W., Bradshaw, S.J., Holman, G.D.
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 All,
We invite contributions to the session (ID#: ST27) “New Insights Into The
Physics Of White-light Flares” at the AOGS meeting in Beijing, 31 Jul to
5 Aug, 2016. Details on the session follow.
We would like to remind you that the abstract submission deadline is 19
February 2016.
Abstracts can be submitted using the following link:
http://www.asiaoceania.org/aogs2016/public.asp?page=abstract.htm
Best regards,
Juan Carlos Martinez Oliveros
Hugh S Hudson
Lucia Kleint
Mingde Ding
---------------------------------------------
Session Title:
New Insights Into The Physics Of White-light Flares
Session Description:
The white-light continuum of a solar flare was the first manifestation of a
flare ever detected, and this continuum emission contains a large fraction
of the total luminous energy of a flare. Thus its identification has always
posed an important problem for solar and stellar physics. A zoo of
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 in the visible continuum of flares, from the corona to
the solar interior and how multi wavelength observations (RHESSI, IRIS,
SDO, Hinode, infrared, NoRH, OVSA) can help our understanding of the
mechanics of momentum and energy transfer in the solar atmosphere.
MAX MILLENNIUM NEWS
30 December 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
The Hinode /XRT Full-Sun Image Corrections and the Improved Synoptic
Composite Image Archive
-- Takeda, A., Yoshimura, K., Saar, S.
On-Orbit Performance and Calibration of the Soft X-ray Telescope
on Yohkoh
-- Loren Acton
Last news on zebra pattern
-- Gennady Chernov
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