No. 347, “Persistent quasi-periodic pulsations detected during the large X8.2 solar flare,” by Laura Hayes and Peter Gallagher: The most beautiful flare has the most beautiful pulsations!
No. 346, “Is the coronal magnetic field braiding?” by Markus Aschwanden. An iconic cartoon does not relate well to the observations.
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
MAX MILLENNIUM NEWS
20 March 2019
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
Three-dimensional reconstruction of CME-driven shock-streamer
interaction from radio observations: a different take on the
diagnostics of coronal magnetic fields
-- S. Mancuso, F. Frassati, A. Bemporad, D. Barghini
The soft X-ray spectrometer polarimeter SolpeX
-- J. Sylwester; M. Steslicki; J. Bakala; S. Plocieniak; Å. Szaforz;
M. Kowalinski; D. Scislowski; P. Podgórski; T. Mrozek; J. Barylak;
A. Makowsk; M. Siarkowski; Z. Kordylewski; B. Sylwester; S. Kuzin;
A. Kirichenko; A. Pertsov; S. Bogachev
Variable emission mechanism of a Type IV radio burst
-- D. E. Morosan, E. K. J. Kilpua, E. P. Carley, and C. Monstein
Inference of magnetic field strength and density from damped
transverse coronal waves
-- I. Arregui, M. Montes-Solis, A. Asensio Ramos
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 March 2019
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
Frequency-Distance Structure of Solar Radio Sources Observed by
LOFAR
-- Mykola Gordovskyy, Eduard Kontar, Philippa Browning, and
Alexey Kuznetsov
The birth of a coronal mass ejection
-- Tingyu Gou, Rui Liu, Bernhard Kliem, Yuming Wang, and
Astrid M. Veronig
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
Dear Colleagues,
We are pleased to announce registration/abstract submission for the next
CESRA Workshop,
“CESRA2019: The Sun and the inner heliosphere”
which will be held on July 8th – 12th, 2019, at Telegrafenberg, Potsdam,
Germany.
http://meetings.aip.de/cesra2019/cms/
CESRA, the Community of European Solar Radio Astronomers, organizes
triennial workshops on investigations of the solar atmosphere using
radio and other observations. Although special emphasis is given to
radio diagnostics, the workshop topics are of interest to a large
community of solar physicists. The format of the workshop will combine
plenary sessions and working group sessions, with invited review talks,
oral contributions, and posters.
To register and to submit the abstract please follow the link:
http://meetings.aip.de/cesra2019/registration/
The CESRA 2019 workshop will place an emphasis on linking the Sun with
the heliosphere, motivated by the launch of Parker Solar Probe in 2018
and the upcoming launch of Solar Orbiter in 2020. It will provide the
community with a forum for discussing the first relevant science results
and future science opportunities, as well as on opportunity for
evaluating how to maximize science return by combining space-borne
observations with the wealth of data provided by new and future
ground-based radio instruments, such as ALMA, E-OVSA, EVLA, LOFAR,
MUSER, MWA, and SKA, and by the large number of well-established radio
observatories.
On behalf of the CESRA Board and the local SOC representatives,
Eduard Kontar, Gottfried Mann, Alexander Warmuth
MAX MILLENNIUM NEWS
06 March 2019
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
Properties of slow magnetoacoustic oscillations of solar coronal
loops by multi-instrumental observations
-- Nakariakov, V. M., Kosak, M. K., Kolotkov, D. Y., Anfinogentov,
S. A., Kumar, P., Moon, Y.-J.
Persistent Quasi-Periodic Pulsations During a Large X-Class Solar
Flare
-- Laura A. Hayes, Peter T. Gallagher, Brian R. Dennis, Jack Ireland,
Andrew Inglis, and Diana E. Morosan
Magnetic helicity and fluxes in an inhomogeneous α squared dynamo
-- A. Brandenburg
Properties of the Diffuse Emission around Warm Loops in Solar Active
Regions
-- David H. Brooks
Comparative Study of Microwave Polar Brightening, Coronal Holes, and
Solar Wind Over the Solar Poles
-- Ken'ichi Fujiki, Kiyoto Shibasaki, Seiji Yashiro, Munetoshi
Tokumaru, Kazumasa Iwai, Satoshi Masuda
3He-rich Solar Energetic Particles from Sunspot Jets
-- Radoslav Bucik, Mark E. Wiedenbeck, Glenn M. Mason, Raul
Gomez-Herrero, Nariaki V. Nitta, Linghua Wang
Relative magnetic field line helicity
-- K. Moraitis, E. Pariat, G. Valori, K. Dalmasse
Forbush decreases and Geomagnetic Storms during a Highly
Disturbed Solar and Interplanetary Period, 4-10 September 2017
-- B. Badruddin, O. P. M. Aslam, M. Derouich, H. Asiri and K. Kudela
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
Source Imaging of a Moving Type-IV Solar Radio Burst and its Role in
Tracking Coronal Mass Ejection From the Inner to the Outer Corona
by Y. Chen et al.
http://cesra.net/?p=2143
Temperature constraints from inversions of synthetic solar optical,
UV and radio spectra
by J. M. da Silva Santos et al*
http://cesra.net/?p=2131
—-
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are short
communications written in language accessible to a non-expert in the
specific area and designed to keep solar and heliophysics communities
informed and up-to-date about current research. The highlights can be
followed, discussed, commented and shared via
http://www.facebook.com/solarcesra/ and http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
27 February 2019
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
Helical Twisting Number and Braiding Linkage Number of Solar Coronal
Loops
-- Markus J. Aschwanden
Small-scale motions in solar filaments as the precursors of eruptions
-- Daikichi SEKI, Kenichi OTSUJI, Hiroaki ISOBE, Takako T. ISHII,
Kiyoshi ICHIMOTO and Kazunari SHIBATA
Modeling of Heliospheric Modulation of Cosmic-Ray Positrons in
a Very Quiet Heliosphere
-- O. P. M. Aslam, D. Bisschoff, M. S. Potgieter, M. Boezio, and
R. Munini
Interpreting magnetic helicity flux in solar flux emergence
-- Prior, C. and MacTaggart, D.
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 February 2019
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
Transient Inverse-FIP Plasma Composition Evolution within a Confined
Solar Flare
-- Deborah Baker, Lidia van Driel-Gesztelyi, David H. Brooks,
Gherardo Valori, Alexander W. James, J. Martin Laming, David M. Long,
Pascal Demoulin, Lucie M. Green, Sarah A. Matthews, Katalin Olah,
Zsolt Kovari
The Role of a Tiny Brightening in a Huge Geo-effective Solar Eruption
Leading to the St Patrick's Day Storm
-- Yumi Bamba, Satoshi Inoue, and Keiji Hayashi
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. 345, “A Energetic Pre-flare: Electron Distributions in Magnetic Reconnection Outflows,” by Marina BATTAGLIA, Eduard KONTAR, and Galina MOTORINA. Assessing energy partition in a very interesting pre-impulsive flare development.
No. 344, “Linear Polarization in H-alpha Flares,” by Tomoko KAWATE and Yoichiro HANAOKA. H-alpha polarization (perhaps implying electron beams) is rarely observable, but in one case there are suggstive results.
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
MAX MILLENNIUM NEWS
13 February 2019
CONTENTS
0. A MILESTONE, AND THANKS, FOR THE E-PRINT ARCHIVE
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
0. A MILESTONE, AND THANKS, FOR THE E-PRINT ARCHIVE
===================================================
<richard.canfield at montana.edu>
This week the Max Millennum Solar Physics E-Print Archive logged it's
4000th submission! That's trivial on the scale of the Cornell/LANL
arXiv, of course, but it demonstrates empirically what we all know --
there is value to us in an archive that is specific to a
subdiscipline -- solar and heliospheric actvity, in this case.
It gives me great pleasure to thank Alisdair Davey for his seminal
role in creating the E-Print Archive in mid-2000 and maintaining it
ever since. I searched the Max Millennium Science Mail Archive
to get a sense of the duration of his committment. I found that
the Max Millennium News message announcing the availability of the
enhanced E-Print archive came shortly after a message from Bob Lin,
reporting that RHESSI had been reconfirmed for flight after the
spacecraft was severely damaged as the result of the shake table
malfunction during a vibration test!
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
A basal contribution from p-modes to the Alfvénic wave flu in the
Sun's Corona
-- R. J. Morton, M. Weberg, J. A. McLaughlin
Multiwavelength Study of Equatorial Coronal-Hole Jets
-- Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos,
Peter F. Wyper, C. Richard DeVore, Craig E. DeForest
Non-thermal hydrogen Lyman line and continuum emission in solar
flares generated by electron beams
-- Druett, M.K. and Zharkova V.V.
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