“When the Earth’s atmosphere becomes dynamic…”, by Temmer, Krauss, and Veronig: The Earth’s atmosphere reacts strongly to the occurrence of flares and CMEs.
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.
This workshop, "The Sun's Chromosphere in the Era of ALMA, IRIS, and DKIST,"
will take place March 15-18 in Boulder, CO (USA). See
http://www.nso.edu/workshops/SunAID
and its links for full details. The workshop aims at exploiting new data and
simulations from existing facilities in anticipation of the revolutionary
capabilities of ALMA and DKIST. The program is complete and includes
practical demonstrations as well as planning aids for the first ALMA
solicitation for solar proposals. Some additional registrations (and poster
presentations) would be welcome.
MAX MILLENNIUM NEWS
10 February 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
Three-Year Global Survey of Coronal Null Points
from Potential-Field-Source-Surface (PFSS) Modeling and
Solar Dynamics Observatory (SDO) Observations
-- M. S. Freed, D. W. Longcope, and D. E. McKenzie
Analysis of Flows Inside Quiescent Prominences as Captured by
Hinode/Solar Optical Telescope
-- M. S. Freed, D. E. McKenzie, D. W. Longcope, and M. Wilburn
Ground-based Observations of the Solar Sources of Space Weather
(Invited Review)
-- Astrid M. Veronig, W. Poetzi
Irreversible Rapid Changes of Magnetic Field Associated with
the 2012 October 23 Circular Near-limb X1.8 Flare
-- Dandan Ye, Chang Liu and Haimin Wang
Tracing the Chromospheric and Coronal Magnetic Field with AIA,
IRIS, IBIS, and ROSA Data
-- Aschwanden, M.J., Reardon, K., and Jess, D.
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
03 February 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
The Vertical Current Approximation Nonlinear Force-Free Field Code -
Description, Performance Tests, and Measurements of Magnetic Energies
Dissipated in Solar Flares
-- Markus J. Aschwanden
High--cadence observations of spicular-type events on the Sun
-- J. Shetye, J.G. Doyle, E. Scullion, C. J. Nelson, D. Kuridze,
V. Henriques, F. Woeger, T. Ray
Transition-region/Coronal Signatures and Magnetic Setting of Sunspot
Penumbral Jets: Hinode (SOT/FG), Hi-C, and SDO/AIA Observations
-- Tiwari, Sanjiv K.; Moore, Ronald L.; Winebarger, Amy R.; Alpert,
Shane E.
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
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~