“Soft X-ray emission in kink-unstable coronal loops,” by Rui Pinto, Nicole Vilmer, and Sacha Brun. Kinking flux ropes can create flare emission, but their detection may be deceptive.
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
25 March 2015
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
Spatially resolved observations of a coronal type II radio burst
with multiple lanes
-- Zimovets I.V., Sadykov V.M.
On the support of neutrals against gravity in solar prominences
-- J. Terradas, R. Soler, R. Oliver, \& J. L., Ballester
The effects of ion mass variation and domain size on octupolar out-of-plane
magnetic field generation in collisionless magnetic reconnection
-- Jan Graf von der Pahlen, David Tsiklauri
New Observations of the Solar 0.5-5 keV Soft X-ray Spectrum
-- Amir Caspi, Thomas N. Woods, Harry P. Warren
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
MAX MILLENNIUM NEWS
18 March 2015
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
JOINT HIGH TEMPERATURE OBSERVATION OF A SMALL C6.5 SOLAR FLARE WITH
IRIS/EIS/AIA
-- Polito V., Reeves, K.K., Del Zanna, G., Golub, L., Mason, H.E.
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
“Daily solar mm-observations at Aalto University Metsahovi Radio Observatory," by Juha Kallunki and Minttu Uunila: systematic microwave and mm-wave solar observations from Finland, with long summers.
See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series of RHESSI Nuggets, 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.
Thanks for all the input for the 6th RHESSI Senior Review Proposal. It was submitted last week to NASA Headquarters. You can access it through the RHESSI web site at the following location:
http://hesperia.gsfc.nasa.gov/rhessi3/mission/documents/index.html
The oral presentation to the Senior Review Committee will be on Tuesday, April 21.
Brian
Brian R. Dennis
Solar Physics Laboratory, Code 671
Goddard Space Flight Center
Greenbelt, MD 20771
301-286-7983
brian.r.dennis(a)nasa.gov
MAX MILLENNIUM NEWS
11 March 2015
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
Multiwavelength observations of a partially eruptive filament
on 2011 September 8
-- Q. M. Zhang, Z. J. Ning, Y. Guo, T. H. Zhou, X. Cheng, H. S. Ji,
L. Feng, T. Wiegelmann
DESAT: an SSW tool for SDO/AIA image de-saturation
-- Richard A Schwartz, Gabriele Torre, Anna Maria Massone, Michele Piana
Solar Flare Element Abundances from the Solar Assembly for
X-rays (SAX) on MESSENGER
-- B. R. Dennis, K. J. H. Phillips, R. A. Schwartz, A. K. Tolbert,
R. D. Starr, and L. R. Nittler
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
“Solar Physics during the March 2015 Solar Eclipse,” by Hamish Reid and Hugh Hudson. A total solar eclipse is coming on 2015 March 20, presenting a good opportunity for many observatories - in particular, European radio observatories.
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
04 March 2015
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
RESIK SOLAR X-RAY FLARE ELEMENT ABUNDANCES ON A NON-ISOTHERMAL
ASSUMPTION
-- B. Sylwester, K. J. H. Phillips, J. Sylwester, A.. Kepa
A Type II Radio Burst without a Coronal Mass Ejection
-- Su, W., Cheng, X., Ding, M. D., Chen, P. F., and Sun, J. Q.
Imaging and Spectroscopic Diagnostics on the Formation of Two
Magnetic Flux Ropes Revealed by SDO/AIA and IRIS
-- X. Cheng, M. D. Ding, C. Fang
The Relationship Between Solar Coronal X-Ray Brightness and Active
Region Magnetic Fields: A Study Using High-Resolution Hinode
Observations
-- Soumitra Hazra, Dibyendu Nandy, B Ravindra
Sign Singularity and Flares in Solar Active Region NOAA 11158
-- L. Sorriso-Valvo, G. De Vita, M. D. Kazachenko, S. Krucker,
L. Primavera, S. Servidio, A. Vecchio, B. T. Welsch, G. H. Fisher,
F. Lepreti, and V. Carbone
X-ray and EUV Observations of Simultaneous Short and Long Period
Oscillations in Hot Coronal Arcade Loops
-- Pankaj Kumar, Valery M. Nakariakov, Kyung-Suk Cho
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
55. On the plasma and magnetic field structure of prominence legs
by Peter Levens, Nicolas Labrosse (University of Glasgow), Brigitte Schmieder (Observatoire de Paris) & Arturo López Ariste (IRAP, Toulouse)
Can we unweave the magnetic field from the twisted plasma in prominences?
http://www.uksolphys.org/?p=9654
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~