MAX MILLENNIUM NEWS
27 July 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Quasi-Periodic Pulsations During the Impulsive and Decay Phases
of an X-class Flare
-- Laura A. Hayes, Peter T. Gallagher, Brian R. Dennis, Jack
Ireland, Andrew R. Inglis, Daniel F. Ryan
Projection effects in coronal dimmings and associated EUV wave event
-- K. Dissauer, M. Temmer, A.V. Veronig, K. Vanninathan, J. Magdalenic
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
20 July 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
3D MHD modeling of twisted coronal loops
-- F. Reale, S. Orlando, M. Guarrasi, A. Mignone, G. Peres,
A. W. Hood, E. R. Priest
Influence of the Magnetic Field on Oscillation Spectra in Solar
Faculae
-- Andrei A. Chelpanov, Nikolai I. Kobanov, Dmitry Y. Kolobov
Local Helioseismology of Emerging Active Regions: A Case Study
-- Alexander G. Kosovichev, Junwei Zhao, and Stathis Ilonidis
Reconstruction of Solar Subsurfaces by Local Helioseismology
-- Alexander G. Kosovichev and Junwei Zhao
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
Our current fleet of space-based solar observatories offer us a wealth of opportunities to study solar flares over a range of wavelengths, and the greatest advances in our understanding of flare physics often come from coordinated observations between different instruments. However, finding or keeping track of which flares have been observed by specific combinations of instruments can be cumbersome and time consuming. To alleviate this issue, and provide access to a broader range of flaring events observed by GOES, RHESSI, Hinode (EIS, SOT, and XRT), SDO/EVE (MEGS-A and MEGS-B), and IRIS, a new interface has been developed and incorporated into SSWIDL. After updating your SSWIDL directory, simply type IDL> solar_flare_finder to bring up the widget. After selecting a time range (it defaults to the beginning of the SDO mission to the present day), and which combination of instruments you require to address a given science question, along with options for GOES class, maximum energy observed by RHESSI, and flare location (disk or limb), etc, click the Search button. This will return a list of flares that conform to your search criteria. Clicking on a given flare in this list will call up a plot that containing 1) the GOES X-ray lightcurves with the timing of your chosen observations overlaid, 2) the RHESSI lightcurves up to the maximum recorded energy, and 3) a RHESSI full-disk quicklook image with the fields of view of the different instruments overlaid. The option exists to also download a copy of this .png file to your current working directory, or an IDL .sav file containing the metadata used in generating the plots.
These plots are also accessible via the RHESSI browser (http://sprg.ssl.berkeley.edu/~tohban/browser/) for flares observed by RHESSI since the launch of SDO. Check the box marked “Cross-Mission Synoptic”, and expand it to include the “Hinode/EVE/IRIS” check box. Future improvements to this service will include adding flares that were not observed by RHESSI, adding additional instruments (e.g. Fermi, NoRH, GOES/EUVS, etc), and direct access to the data itself. Please address any questions, comments or requests to r.milligan(a)qub.ac.uk<mailto:r.milligan@qub.ac.uk>. Thanks to Kim Tolbert for her help with designing the widget, Albert Shih for incorporating the plots into the RHESSI browser, and Dominic Zarro for help with the Hinode/EIS software.
MAX MILLENNIUM NEWS
13 July 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
ROAM: a Radial-basis-function Optimization Approximation Method
for diagnosing the three-dimensional coronal magnetic field
-- K. Dalmasse, D. W. Nychka, S. E. Gibson, Y. Fan, N. Flyer
Diagnostics of Coronal Magnetic Fields through the Hanle Effect
in UV and IR Lines
-- Nour E. Raouafi, Pete Riley, Sarah Gibson, Silvano Fineschi and
Sami K. Solanki
Solar Coronal Jets: Observations, Theory, and Modeling
-- N.E. Raouafi, S. Patsourakos, E. Pariat, P.R. Young,
A.C. Sterling, A. Savcheva, M. Shimojo, F. Moreno-Insertis,
C.R. DeVore, V. Archontis, T. Torok, H. Mason, W. Curdt, K. Meyer,
K. Dalmasse, Y. Matsui
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 July 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Flux rope proxies and fan-spine structures in active region NOAA
11897
-- Y. J. Hou, T. Li and J. Zhang
Spatially resolved observation of the fundamental and second harmonic
standing kink modes using SDO/AIA
-- D. J. Pascoe, C. R. Goddard, and V. M. Nakariakov
Plasma sloshing in pulse-heated solar and stellar coronal loops
-- F. Reale
Multi-wavelength Study of Transition Region Penumbral Subarcsecond
Bright Dots Using IRIS and NST
-- Na Deng, Vasyl Yurchyshyn, Hui Tian, Lucia Kleint, Chang Liu,
Yan Xu, and Haimin Wang
Fractal Reconnection in Solar and Stellar Environments
-- Kazunari Shibata and Shinsuke Takasao
Above-the-loop-top Oscillation and Quasi-periodic Coronal Wave
Generation in Solar Flares
-- Shinsuke Takasao and Kazunari Shibata
Magnetohydrodynamics modeling of coronal magnetic field and solar
eruptions based on the photospheric magnetic field
-- Satoshi Inoue
Flaring Rates and the Evolution of Sunspot Group McIntosh
Classifications
-- Aoife E. McCloskey, Peter T. Gallagher, D. Shaun Bloomfield
How did a Major Confined Flare Occur in Super Solar Active Region
12192?
-- Chaowei Jiang, Shi Tsan Wu, Vasyl B Yurchyshyn, Haimin Wang,
Xueshang Feng, Qiang Hu
Magnetic flux concentrations from turbulent stratified convection
-- P. J. Kapyla, A. Brandenburg, N. Kleeorin, M. J. Kapyla,
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
29 June 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
Stellar Evidence that the Solar Dynamo may be in Transition
-- Travis S. Metcalfe, Ricky Egeland, Jennifer van Saders
Shock Connectivity in the August 2010 and July 2012 Solar Energetic
Particle Events Inferred from Observations and ENLIL Modeling
-- H. M. Bain, M. L. Mays, J. G. Luhmann, Y. Li, L. K. Jian, and
D. Odstrcil
Measuring Solar Doppler Velocities in the He II 30.38 nm Emission
Using the EUV Variability Experiment (EVE)
-- Phillip C. Chamberlin
Flux cancellation in the evolution of the eruptive filament of
2011 June 7
-- S. L. Yardley, L. M. Green, D. R. Williams, L. van
Driel-Gesztelyi, G. Valori, S. Dacie
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. 277, June 27: “Spotlessness returns,” by Hugh Hudson
No. 276, June 20: “RHESSI has resumed operations,” by Albert Shih, Brian Dennis, and Sa”m Krucker
No. 275, June 6: “Non-thermal recombinationin solar flares and microflares,” by Jeffrey Reep and John Brown
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
22 June 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
Slow-Mode MHD Wave Penetration into a Coronal Null Point due to
the Mode Transmission
-- Andrey Afanasyev and Arkadiy Uralov
Secondary fast magnetoacoustic waves trapped in randomly structured
plasmas
-- Ding Yuan, Bo Li, Robert W. Walsh
Unexpected spatial intensity distributions and onset timing
of solar electron events observed by closely spaced STEREO
spacecraft
-- A. Klassen, N. Dresing, R. Gómez-Herrero, B. Heber
R. Müller-Mellin
Flare Generated Shock Wave Propagation Through Solar Coronal Arcade
Loops and Associated Type II Radio Burst
-- Kumar, Pankaj; Innes, D. E.; Cho, K. S.
Observing the release of twist by magnetic reconnection in a solar
filament eruption
-- Zhike Xue, Xiaoli Yan, Xin Cheng, Liheng Yang, Yingna Su, Bernhard
Kliem, Jun Zhang, Zhong Liu, Yi Bi, Yongyuan Xiang, Kai Yang,
Li Zhao
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
8 June 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
f-mode interaction with models of sunspot: near-field scattering
and multifrequency effects
-- K.Daiffallah
On-line Tools for Solar Data Compiled in the Debrecen Observatory
and their Extensions with the Greenwich Sunspot Data
-- T. Baranyi, L. Gyori, A. Ludmány
Coronal mass ejection-related particle acceleration regions during
a simple eruptive event
-- Carolina Salas-Matamoros, Karl-Ludwig Klein and Alexis P. Rouillard
The First Focused Hard X-ray Images of the Sun with NuSTAR
-- Brian W. Grefenstette, Lindsay Glesener, Säm Krucker, Hugh
Hudson, Iain G. Hannah, David M. Smith, Julia K. Vogel, Stephen M.
White, Kristin K. Madsen, Andrew J. Marsh, Amir Caspi, Bin Chen,
Albert Shih, Matej Kuhar, Steven E. Boggs, Finn E. Christensen,
William W. Craig, Karl Forster, Charles J. Hailey, Fiona A. Harrison,
Hiromasa Miyasaka, Daniel Stern, William W. Zhang
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