MAX MILLENNIUM NEWS
31 January 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
Formation and Dynamics of a Solar Eruptive Flux Tube
-- Satoshi Inoue, Kanya Kusano, Jorg Buchner, Jan Skala
The Instruments and Capabilities of the Miniature X-ray Solar
Spectrometer (MinXSS) CubeSats
-- Christopher S. Moore, Amir Caspi, Thomas N. Woods,
Phillip C. Chamberlin, Brian R. Dennis, Andrew R. Jones,
James P. Mason, Richard A. Schwartz, Anne K. Tolbert
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
24 January 2018
CONTENTS
1. NEW MEMBER OF THE MAX MILLENNIUM CHIEF OBSERVER TEAM
2. E-PRINTS POSTED IN THE PAST WEEK
3. FROM THE EDITOR
=====================================================================
1. NEW MEMBER OF THE MAX MILLENNIUM CHIEF OBSERVER TEAM
=======================================================
It is a pleasure to welcome a new Max Millennium Chief Observer.
Aoife McCloskey is presently a PhD student at Trinity College Dublin,
Ireland. Her thesis supervisors are current MM_CO Shaun Bloomfield
and one of the original MM_COs, Peter Gallagher. Aoife is three years
into her PhD and has concentrated on evolution of active regions in
terms of their McIntosh classifications and how these impact on
subsequent 24-hr flaring rates
(http://adsabs.harvard.edu/abs/2016SoPh..291.1711M). Her current work
is in applying these evolution-dependent rates in Poisson-based
forecasting and verification of their performance.
2. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Fine Structures of Solar Radio Type III Bursts and their Possible
Relationship with Coronal Density Turbulence
-- Xingyao Chen, Eduard P. Kontar, Sijie Yu, Yihua Yan, Jing Huang,
Baolin Tan
Influence of misalignments on the performance of externally occulted
solar coronagraphs. Application to PROBA-3/ASPIICS
-- S. V. Shestov, A. N. Zhukov
Observations of Electron-driven Evaporation during a Flare Precursor
-- Dong Li, Ying Li, Wei Su, Yu Huang, Zongjun Ning
The "FIP Effect" and the Origins of Solar Energetic Particles and
of the Solar Wind
-- Donald V. Reames
Sun-to-Earth MHD Simulation of the 14 July 2000 "Bastille Day"
Eruption
-- Tibor Torok, Cooper Downs, Jon Linker, Roberto Lionello,
Viacheslav S. Titov, Zoran Mikic, Pete Riley, Ron M. Caplan,
Janvier Wijaya
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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
17 January 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
The density compression ratio of shock fronts associated with
coronal mass ejections
-- Ryun-Young Kwon, Angelos Vourlidas
Evolution of Photospheric Flow and Magnetic Fields Associated with
the 2015 June 22 M6.5 Flare
-- Jiasheng Wang, Chang Liu, Na Deng, Haimin Wang
Spatially inhomogeneous acceleration of electrons in solar flares
-- Duncan J. Stackhouse and Eduard P. Kontar
Probing Twisted Magnetic Field Using Microwave Observations in
an M Class Solar Flare on 11 February, 2014
-- I.N. Sharykin, A.A. Kuznetsov, I.I. Myshyakov
The origin, early evolution and predictability of solar eruptions
-- L.M. Green, T. Torok, B. Vrsnak, W. Manchester IV, A. Veronig
Polar Field Correction for HMI Line-of-Sight Synoptic Data
-- Xudong Sun, for the HMI Team
Relationship between Intensity of White-Light Flares and Proton Flux
of Solar Energetic Particles
-- Nengyi Huang, Yan Xu, Haimin Wang
Spectroscopic Observations of a Current Sheet in a Solar Flare
-- Y. Li, J. C. Xue, M. D. Ding, X. Cheng, Y. Su, L. Feng,
J. Hong, H. Li, W. Q. Gan
IRIS Observations of Spicules and Structures Near the Solar Limb
-- C. E. Alissandrakis, J.-C. Vial, A. Koukras, E. Buchlin,
M. Chane-Yook
Strong Transverse Photosphere Magnetic Fields and Twist in Light
Bridge Dividing Delta Sunspot of Active Region 12673
-- Wang, Haimin; Yurchyshyn, Vasyl; Liu, Chang; Ahn, Kwangsu;
Toriumi, Shin and Cao, Wenda
Simultaneous observation of a flux rope eruption and magnetic
reconnection during an X-class solar flare
-- X. L. Yan, L. H. Yang, Z. K. Xue, Z. X. Mei, D. F. Kong,
J. C. Wang, Q. L. Li
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
10 January 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
Spectroscopic diagnostics of the non-Maxwellian κ-distributions
using SDO/EVE observations of the 2012 March 7 X-class flare
-- Elena Dzifcakova, Alena Zemanova, Jaroslav Dudik, and
Simon Mackovjak
Transient rotation of photospheric vector magnetic fields associated
with a solar flare
-- Yan Xu, Wenda Cao, Kwangsu Ahn, Ju Jing, Chang Liu, Jongchul Chae,
Nengyi Huang, Na Deng, Dale E. Gary and Haimin Wang
Three-dimensional Forward-fit Modeling of the Hard X-Ray and
Microwave Emissions of the 2015 June 22 M6.5 Flare
-- Natsuha Kuroda, Dale E. Gary, Haimin Wang, Gregory D. Fleishman,
Gelu M. Nita, Ju Jing
Center-to-Limb Variability of Hot Coronal EUV Emissions During Solar
Flares
-- Edward Thiemann, Phillip Chamberlin, Francis Eparvier, Luke Epp
A time dependent relation between EUV solar flare light-curves
from lines with differing formation temperatures
-- Edward M.B. Thiemann, Francis G. Eparvier, Thomas N. Woods
Understanding Breaks in Flare X-Ray Spectra: Evaluation of a
Cospatial Collisional Return-current Model
-- Alaoui, Meriem; Holman, Gordon
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 January 2018
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. THANKS TO THE MAX MILLENNIUM CHIEF OBSERVERS
3. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Solar energetic particles and radio burst emission
-- R. Miteva, S. W. Samwel and V. Krupar
A quasi-periodic fast-propagating magnetosonic wave associated with
the eruption of a magnetic flux rope
-- Yuandeng Shen; Yu Liu; Tengfei Song; Zhanjun Tian
2. THANKS TO THE MAX MILLENNIUM CHIEF OBSERVERS
===============================================
<from richard.canfield at montana.edu>
I'd like to get the year off to a good start by thanking the four
skilled and dedicated volunteers who serve the solar community as
Max Millennium Chief Observers, keeping abreast of solar activity
and sending out the Max Millennium Message of the day:
Bill Marquette (Helio Research), since 2000
Ryan Milligan (University of Glagow and GSFC), since 2007
Shaun Bloomfield (Northumbria University), since 2008
Ying Li (Purple Mountain Observatory, since 2015
When you next see any of them at a meeting, please join me in
thanking them for their many years of service to the NASA RHESSI
mission (which supports the Max Millennium program) and the solar
activity research community.
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 richard.canfield at montana.edu