"The Formation of Kappa Distributions in Solar Flares," by Nicolas Bian and Duncan Stackpole. It turns out that a kappa distribution can arise naturally from Coulomb collisions, as in a coronal thick target.
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
08 October 2014
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 the Magnetic Flux of Solar Eruptions and the Ap Index
of Geomagnetic Storms
-- I. M. Chertok, M. A. Abunina, A. A. Abunin, A. V. Belov, V. V. Grechnev
Early Evolution of an Energetic Coronal Mass Ejection and Its Relation
to EUV Waves
-- Rui Liu, Yuming Wang, and Chenglong Shen
The Formation of Kappa-Distribution Accelerated Electron Populations
in Solar Flares
-- Bian, Nicolas H., Emslie, A. Gordon, Stackhouse, Duncan J., Kontar, Eduard P.
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
Dear all,
A new EIS Nugget entitled 'Measurement of outflow velocities in plumes from EIS observations' by Hui Fu, Lidong Xia, Bo Li, Zhenghua Huang, Fangran Jiao and Chaozhou MouLen of Shandong University, China is available here:
http://solarb.mssl.ucl.ac.uk/SolarB/eisnuggets.jsp
We welcome contributions from the community.
Regards,
Deb Baker
UCL-MSSL
--
Dr. Deb Baker
UCL - Mullard Space Science Laboratory
Email: Deborah.Baker(a)ucl.ac.uk
Tel: +44 (0) 1483 204 179
Dear RHESSI'ers,
We are soliciting input for the NASA 2015 Senior Review of Heliophysics operating missions. Please send us summaries of your RHESSI-related work over the last two years and, as importantly, your plans for future work.
To help you decide what will be most useful to us in preparing the proposal, here are excerpts from the Instructions to Proposers:
The objectives of the 2015 HPD Senior Review for MO&DA is to assess the science merits and performance of these 15 missions (in alphabetical order): ACE, AIM, CINDI, Hinode, IBEX, IRIS, RHESSI, SDO, STEREO, THEMIS, TIMED, TWINS, Van Allen Probes, Voyager, and Wind. Performance factors to be evaluated will include mission scientific productivity, technical status, budget efficiency, data quality and accessibility, and contribution to the "Heliophysics System Observatory (HSO)."
"The period for this Senior Review will cover FY16 to FY20. Each mission that is invited to this Senior Review will submit a proposal outlining how its science investigations will benefit the Heliophysics research objectives. These objectives and focus areas are described in the Science Plan for NASA's Science Mission Directorate 2014" - the SMD Science Plan available at -
http://science.nasa.gov/media/medialibrary/2014/05/02/2014_Science_Plan-050…
Previous Senior Review proposals and panel reports at the following location:
http://hesperia.gsfc.nasa.gov/rhessi2/home/mission/documents/
Finally, please make sure that all of your RHESSI-related publications are included in Markus Aschwanden's list at the following web site:
http://www.lmsal.com/~aschwand/publications/rhessi.html<http://www.lmsal.com/%7Easchwand/publications/rhessi.html>
Thanks and best wishes,
Sam Krucker, Brian Dennis, and Albert Shih
Samuel Krucker, RHESSI PI
Space Sciences Lab.
University of California
7 Gauss Way
Berkeley, CA 94720
Phone: (510) 643-3101
Cell: 510-502-5220
FAX: 510-643-8302
Email: krucker(a)ssl.berkeley.edu<mailto:krucker@ssl.berkeley.edu>
Brian R. Dennis, RHESSI Mission Scientist
Solar Physics Laboratory - Code 671
Heliophysics Science Division
Sciences and Exploration Directorate
Greenbelt, MD 20771
Phone: 301-286-7983
FAX: 301-286-1617
Email: brian.r.dennis_at_nasa.gov
Albert Y. Shih, RHESSI Deputy Mission Scientist
Solar Physics Laboratory - Code 671
Heliophysics Science Division
Sciences and Exploration Directorate
Greenbelt, MD 20771
Phone: 301-286-1843
FAX: 301-286-1617
Email: albert.y.shih_at_nasa.gov
51. Observational signatures of magnetic reconnection in kink-unstable coronal loops
by Mykola Gordovskyy, Philippa Browning (University of Manchester) and Rui Pinto (Observatoire de Paris)
What would the flare X-ray emission from a twisted loop look like?
http://www.uksolphys.org/?p=8930
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
MAX MILLENNIUM NEWS
01 October 2014
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
Superflare occurrence and energies on G-, K- and M-type dwarfs
-- Candelaresi, S., Hillier, A., Maehara, H., Brandenburg, A., &
Shibata, K.
Comment on ``Detection and characterization of 0.5--8 MeV neutrons
near Mercury: Evidence for a solar origin"
-- Gerald H. Share, Ronald J. Murphy, Allan J. Tylka, Brian
R. Dennis, and James M. Ryan
How Can Active Region Plasma Escape into the Solar Wind from below a
Closed Helmet Streamer?
-- C.H. Mandrini, F.A. Nuevo, A.M. Vasquez, P. Demoulin, L. van
Driel-Gesztelyi, D. Baker, J.L. Culhane, G.D. Cristiani, M. Pick
On the Area Expansion of Magnetic Flux-Tubes in Solar Active Regions
-- Dudik, J., Dzifcakova, E., Cirtain, J. W.
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
No. 237, "The Balmer continuum observed from IRIS!" by Petr Heinzel and Lucia Kleint. For the first time we have clear and direct observations of the Balmer continuum, from space.
No. 236, "Energy goes up... but doesn't come back down! Coronal heating?" by Brian Welsch. The Poynting flux responsible for coronal heating may have been spotted.
No. 235, "Which detectors can I use to analyze this flare?" by Brian Dennis and Kim Tolbert. A new Browser feature helps to answer this question.
No. 234, "RHESSI resumes observations," by Albert Shih and Sa"m Krucker. Back to normal, the anneal was a success.
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 September 2014
CONTENTS
1. NEW COORDINATED FLARE OBSERVING PLAN
2. E-PRINTS POSTED IN THE PAST WEEK
3. FROM THE EDITOR
=====================================================================
1. NEW COORDINATED FLARE OBSERVING PLAN
From Ryan Milligan <r.milligan (at) qub.ac.uk>
In October 2014, the Dunn Solar Telescope (DST) of NSO will
conduct a full month of Service Mode Operations dedicated to
observations of solar flares. The campaign shall utilize the full
suite of instruments at the DST (ROSA, IBIS, and FIRS), and will
be supported by SDO, Hinode, IRIS, and RHESSI when possible. The
Max Millennium Chief Observers have therefore formulated a new
Max Millennium Observing Plan (MM_OP) - MM#020 DST Service Mode
Support - that will be implemented throughout October (and future
Service Modes) whenever solar activity is at moderate levels and
seeing conditions at the DST are favorable. The specific observing
plans for each instrument for this and other MM_OPs can be found at
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml.
If you have any questions or comments about this new observing
plan, or its implementation, please contact Ryan Milligan
<r.milligan (at) qub.ac.uk>.
2. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
NEW INSIGHTS INTO THE PHYSICAL NATURE OF CORONAL MASS EJECTIONS AND
ASSOCIATED WAVES/SHOCKS WITHIN THE FRAMEWORK OF THREE-DIMENSIONAL
STRUCTURE
-- Ryun-Young Kwon, Jie Zhang, and Oscar Olmedo
Three-dimensional Magnetic Restructuring in Two Homologous Solar
Flares in the Seismically Active NOAA AR 11283
-- Chang Liu, Na Deng, Jeongwoo Lee, Thomas Wiegelmann, Chaowei
Jiang, Brian R. Dennis, Yang Su, Alina Donea, Haimin Wang
Signatures of the non-Maxwellian kappa-distributions in optically
thin line spectra I. Theory and synthetic Fe IX--XIII spectra
-- Dudik, J, Del Zanna, G., Mason, H.E., Dzifcakova, E.
The Relation Between Large-Scale Coronal Propagating Fronts and
Type II Radio Bursts
-- Nariaki V. Nitta, Wei Liu, Nat Gopalswamy, Seiji Yashiro
A simple model of chromospheric evaporation and condensation driven
conductively in a solar flare
-- Dana Longcope
3. 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
We are pleased to announce a new EIS Nugget entitled:
"Tracking Solar Active Region Outflow Plasma from its Source to the near-Earth Environment" by Prof. Len Culhane of UCL-MSSL.
The nugget is located here: http://solarb.mssl.ucl.ac.uk/SolarB/eisnuggets.jsp
We welcome contributions from the community.
Regards,
--
Dr. Deb Baker
UCL - Mullard Space Science Laboratory
Email: Deborah.Baker(a)ucl.ac.uk
Tel: +44 (0) 1483 204 179