MAX MILLENNIUM NEWS
29 August 2018
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 condensations caused by magnetic reconnection between solar
coronal loops
-- Leping Li, Jun Zhang, Hardi Peter, Lakshmi Pradeep Chitta,
Jiangtao Su, Chun Xia, Hongqiang Song, Yijun Hou
Measurement of Vector Magnetic Field in a Flare kernel with a
Spectropolarimetric Observation in He I 10830 A
-- Tetsu Anan, Takurou Yoneya, Kiyoshi Ichimoto, Satoru Ueno,
Daikou Shiota, Satoshi Nozawa, Shinsuke Takasao, Tomoko Kawate
The Relation Between Escape and Scattering Times of Energetic
Particles in a Turbulent Magnetized Plasma: Application to Solar
Flares
-- Frederic Effenberger and Vahe Petrosian
Implications of loop-top origin for microwave, hard X-ray, and
low-energy gamma-ray emissions from behind the limb flares
-- Vahe Petrosian
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
22 August 2018
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
Solar radio emission as a disturbance of aeronautical radionavigation
-- Christophe Marque, Karl-Ludwig Klein, Christian Monstein, Hermann
Opgenoorth, Antti Pulkkinen, Stephan Buchert, Sam Krucker, Rudiger
Van Hoof, Peter Thulesen
A Diagnostic of Coronal Elemental Behavior during the Inverse FIP
Effect in Solar Flares
-- David H. Brooks
Observations of Turbulent Magnetic Reconnection Within a Solar
Current Sheet
-- X. Cheng, Y. Li, L. F. Wan, M. D. Ding, P. F. Chen, J. Zhang,
J. J. Liu
Diagnostic Analysis of the Solar Proton Flares of September 2017
by Their Radio Bursts
-- I. M. Chertok
Densities Probed by Coronal Type III Radio Burst Imaging
-- Patrick I. McCauley, Iver H. Cairns, John Morgan
The Minimum Energy Principle Applied to Parker's Coronal Braiding and
Nanoflaring Scenario
-- Aschwanden, M.J. and van Ballegooijen,A.A.
Eruptions from quiet Sun coronal bright points. I. Observations
-- Chauzhou Mou, Maria S. Madjarska, Klaus Galsgaard, and Lidong Xia
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
15 August 2018
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
Evolution of the transverse density structure of oscillating
coronal loops inferred by forward modelling of EUV intensity
-- C. R. Goddard, P. Antolin, D. J. Pascoe
Non-stationary quasi-periodic pulsations in solar and stellar flares
-- Nakariakov, V.M., Kolotkov, D., Kupriyanova, E.G., Mehta, T., Pugh,
C.E., Lee, D.-H., Broomhall, A.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 richard.canfield at montana.edu
After more than 16 years of successful operations, the RHESSI spacecraft is now planned to be decommissioned on October 1 of this year. The on-board receiver has been slowly degrading since 2017, and commanding from the ground has become increasingly difficult to the point where we have not had a successful command since mid-July. We will continue to try to establish contact, but success is very unlikely. The spacecraft has no further scheduled transmissions and is programmed to automatically decommission itself on October 1.
Because of the communication difficulty, the detectors have not been turned back on following the sixth anneal, which started on April 12. Observations ended on April 11 at 01:50 UT and the last flare in the RHESSI catalog was a B5 on March 3. We have already started implementing the Mission Archive Plan as described in the latest RHESSI Senior Review Proposal
(http://hesperia.gsfc.nasa.gov/senior_review/2017/senior_review_proposal_201…).
For the next few years, RHESSI data products will continue to be accessible on the usual servers. In the future, the archive will be available through the Solar Data Analysis Center (SDAC).
Sam Krucker, PI
krucker(a)ssl.berkeley.edu<mailto:krucker@ssl.berkeley.edu>
Brian Dennis, Mission Scientist
brian.r.dennis(a)nasa.gov<mailto:brian.r.dennis@nasa.gov>
Albert Shih, Deputy Mission Scientist
albert.y.shih(a)nasa.gov<mailto:albert.y.shih@nasa.gov>
It appears inevitable that the RHESSI spacecraft will be
decommissioned on October 1 of this year. The Max Millennium
program is supported by the RHESSI PI team, with NASA funding for
RHESSI operations, which will end on this date.
In the near term, the Max Millennium team will continue to carry out
all current functions: the Message of the Day, the Solar Physics
E-Print Archive, Max Millennium News, the MMscience, MMmotd,
and RHESSI_Data_Analysis mailing lists and archives, and all other
functions of the Max Millennium website at Montana State University:
<http://solar.physics.montana.edu/max_millennium/>.
The Max Millennium program, and the solar activity observing
community as a whole, has long benefitted from the generosity of the
volunteer Max Millennium Chief Observers. All current MM_COs have
expressed their desire to continue in that role: Shaun Bloomfield
(Northumbria University), Ying Li (Purple Mountain Observatory and
Montana State University), Bill Marquette (Hello Research), Aoife
McCloskey (Trinity College Dublin), and Ryan Milligan (University
of Glasgow).
The last two decades have resoundingly demonstrated the value of
multi-mission and multi-observatory coordination of solar activity
and space weather observations. Powerful new facilities have come on
line recently, and others will come in the next few years. Many of
them have high-resolution and limited field of view, which motivate
coordinated observation. We in the Max Millennium program will
solicit support for continuing such coordination in the future.
MAX MILLENNIUM NEWS
8 August 2018
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
Lost and found sunquake in the 6 September 2011 flare caused by beam
electrons
-- Connor Macrae, Sergei Zharkov, Valentina Zharkova, Malcolm Druett,
Sarah Matthews, and Tomoko Kawate
Nonkinematic solar dynamo models with double-cell meridional
circulation
-- V.V. Pipin
Solar Kinetic Energy and Cross Helicity Spectra
-- Hongqi Zhang, Axel Brandenburg
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
1 August 2018
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
Collective Study of Polar Crown Filaments in the Past Four Solar
Cycles
-- Yan Xu, Werner Potzi, Hewei Zhang, Nengyi Huang, Ju Jing, and
Haimin Wang
Highly Ionized Calcium and Argon X-ray Spectra from a Large Solar
Flare
-- K. J. H. Phillips, J. Sylwester, B. Sylwester, M. Kowalinski,
M. Siarkowski, W. Trzebinski, S. Plocieniak, and Z. Kordylewski
Detecting the solar new magnetic flux regions on the base of vector
magnetograms
-- A.A.GolovkoI, I.I.Salakhutdinova
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
Reminder: please consider submitting to session SH008 for the AGU Fall
Meeting; details and link are below. Abstracts are due TOMORROW at 23:59
EDT!
Hope to see you there!
--- Amir
On 07/25/2018, 6:13 PM, "Amir Caspi" <amir(a)boulder.swri.edu> wrote:
> Dear colleagues,
>
> You are cordially invited to submit abstracts to Session SH008 ³High-Energy
> Solar Investigations Through Next-Generation Spectroscopy: X-rays, Gamma-rays,
> and EUV,² for the 2018 AGU Fall Meeting, to be held in Washington, DC, 10 14
> December 2018.
>
> Spectrally resolved measurements in X-rays, gamma-rays, and EUV are critical
> for advancing our understanding of energetic phenomena on the Sun, during both
> flares and quiescence. To that end, this session invites presentations
> covering new instrumentation, enabling technology, missions, and mission
> concepts for next-generation X-ray, gamma-ray, and EUV solar spectroscopy,
> including spatially-resolved measurements, and the science that would be
> enabled by such new observations.
>
> The full session description and abstract submission are here:
> https://agu.confex.com/agu/fm18/prelim.cgi/Session/52561
>
> The deadline to submit an abstract is Wednesday, 1 Aug 2018, at 23:59 EDT.
>
> We welcome your submissions to this exciting session!
>
> --- Amir Caspi, Lindsay Glesener, and Amy Winebarger
>
Dear colleagues,
You are cordially invited to submit abstracts to Session SH008 ³High-Energy
Solar Investigations Through Next-Generation Spectroscopy: X-rays,
Gamma-rays, and EUV,² for the 2018 AGU Fall Meeting, to be held in
Washington, DC, 10 14 December 2018.
Spectrally resolved measurements in X-rays, gamma-rays, and EUV are critical
for advancing our understanding of energetic phenomena on the Sun, during
both flares and quiescence. To that end, this session invites presentations
covering new instrumentation, enabling technology, missions, and mission
concepts for next-generation X-ray, gamma-ray, and EUV solar spectroscopy,
including spatially-resolved measurements, and the science that would be
enabled by such new observations.
The full session description and abstract submission are here:
https://agu.confex.com/agu/fm18/prelim.cgi/Session/52561
The deadline to submit an abstract is Wednesday, 1 Aug 2018, at 23:59 EDT.
We welcome your submissions to this exciting session!
--- Amir Caspi, Lindsay Glesener, and Amy Winebarger
MAX MILLENNIUM NEWS
25 July 2018
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
A Truly Global EUV Wave From the SOL2017-09-10 X8.2 Solar Flare-CME
Eruption
-- Wei Liu, Meng Jin, Cooper Downs, Leon Ofman, Mark Cheung, and
Nariaki Nitta
ALTERNATIVE ZEBRA-STRUCTURE MODELS IN SOLAR RADIO EMISSION
-- G.P. Chernov
Photospheric Shear Flows in Solar Active Regions and Their
Relation to Flare Occurrence
-- S.-H. Park, J. A. Guerra, P. T. Gallagher, M. K. Georgoulis,
D. S. Bloomfield
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