MAX MILLENNIUM NEWS
27 September 2017
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
Detection of 3-Minute Oscillations in Full-disk Lya Emission During
A Solar Flare
-- Ryan O. Milligan, Bernhard Fleck, Jack Ireland, Lyndsay Fletcher,
Brian R. Dennis
A Compressed Sensing-based Image Reconstruction Algorithm for
Solar Flare X-Ray Observations
-- Simon Felix, Roman Bolzern, Marina Battaglia
Comparison of Helioseismic Far-side Active Region Detections with
STEREO Far-Side EUV Observations of Solar Activity
-- P. C. Liewer, J. Qiu, C. Lindsey
Observations of a Radio-quiet Solar Preflare
-- Arnold O. Benz, Marina Battaglia, Manuel Guedel
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
No. 306, “The Last Best Flare of Cycle 24,” by Sa”m Krucker and Hugh Hudson: Right on schedule, Cycle 24 has produced a great flare (and a GLE).
No. 307, “The Kelvin Force and Loop-Top Concentration,” by Kiyoto SHIBASAKI: New physics can explain the perplexing overpressure at the flare looptop regions.
No. 308, “The Power of Turbulence,” by Nic Bian: Turbulent energy content may underlie flare energy transfer, recconnection, and particle acceleration.
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
20 September 2017
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
Energy release in the solar atmosphere from a stream of infalling
prominence debris
-- A. R. Inglis, H. R. Gilbert and L. Ofman
Estimation of a Coronal Mass Ejection Magnetic Field Strength using
Radio Observations of Gyrosynchrotron Radiation
-- Eoin P. Carley, Nicole Vilmer, Paulo J. A. Simoes, Brian O Fearraigh
QUASI-PERIODIC OSCILLATIONS IN FLARES AND CORONAL MASS EJECTIONS
ASSOCIATED WITH MAGNETIC RECONNECTION
-- Takuya Takahashi, Jiong Qiu and Kazunari Shibata
The 17 February 2013 sunquake in the context of the active region's
magnetic field configuration
-- Lucie M. Green, Gherardo Valori, Francesco P. Zuccarello, Sergei
Zharkov, Sarah Matthews, Salvo L. Guglielmino
Optimal Energy Growth in Current Sheets
-- David MacTaggart, Peter Stewart
Long- and Mid-Term Variations of the Soft X-ray Flare Type in Solar
Cycles
-- I.M. Chertok and A.V. Belov
The Abundance of Helium in the Source Plasma of Solar Energetic
Particles
-- Donald V. Reames
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 September 2017
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
Flare Ribbons Approach Observed by the IRIS and the SDO
-- Ting Li, Jun Zhang & Yijun Hou
Slippage of Jets Explained by the Magnetic Topology of NOAA
Active Region 12035
-- R. Joshi, B. Schmieder, R. Chandra, G. Aulanier, F.P. Zuccarello,
W. Uddin
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
06 September 2017
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
Development and Parameters of a Non-Self-Similar CME Caused by
Eruption of a Quiescent Prominence
-- Kuzmenko, I.V.; Grechnev, V.V.
Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb
Active Region: Spatial and Temporal Properties
-- Susanna Parenti, Giulio del Zanna, Antonino Petralia, Fabio Reale,
Luca Teriaca, Paola Testa, and Helen E. Mason
Time variations of observed Hα line profiles and precipitation
depths of non-thermal electrons in a solar flare
-- R. Falewicz, K. Radziszewski, P. Rudawy, A. Berlicki
A Solar cycle correlation of coronal element abundances in
Sun-as-a-star observations
-- David H. Brooks, Deborah Baker, Lidia van Driel-Gesztelyi,
Harry P. Warren
A Database of Flare Ribbon Properties from the Solar Dynamics
Observatory. I. Reconnection Flux
-- Kazachenko, Maria D.; Lynch, Benjamin J.; Welsch, Brian T.;
Sun, Xudong
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