http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 418 , “A Non-PFSS Global Coronal Model,” by Oliver RICE and Anthony YEATES. Modeling as convenient as PFSS but much more realistic
No. 419, “Thomson scattering near sunspots,” by Pascal SAINT-HILAIRE et al.: Completing the modeling of low-coronal Thomson polarimetry - 91 years after Minnaert
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 for these and others. Comments about specific flares can often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
27 October 2021
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
Evaluating Pointing Strategies for Future Solar Flare Missions
-- A. R. Inglis, J. Ireland, A. Y. Shih, S. D. Christe
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
20 October 2021
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
Common origin of quasi-periodic pulsations in microwave and decimetric
solar radio bursts
-- Larisa Kashapova, Dmitrii Kolotkov, Elena Kupriyanova,
Anastasiia Kudriavtseva, Chengming Tan, Hamish Reid
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
13 October 2021
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
Thomson scattering in the lower corona in the presence of sunspots
-- Pascal Saint-Hilaire, Juan-Carlos Martinez Oliveros, Hugh S. Hudson
The Spatial and Temporal Variations of Turbulence in a Solar Flare
-- Morgan Stores, Natasha L. S. Jeffrey, Eduard P. Kontar
Investigations of Sizes and Dynamical Motions of Solar Photospheric Granules
by a Novel Granular Segmenting Algorithm
-- Liu Yanxiao, Jiang Chaowei, Yuan Ding, Zuo Pingbing, Wang Yi, Cao Wenda
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 keiji.yoshimura at montana.edu
Dear All
We would like to remind you that an online science meeting on "Particle Acceleration in Solar Flares and the Plasma Universe" will be held during November 15-19, 2021.
This meeting is open to everyone who is interested in particle energization in space, solar, and astrophysical plasma environments. It is driven by the recent development of a next generation solar X-ray/gamma-ray mission named “PhoENiX” (to be proposed to JAXA for a launch slot in early 2030s). While this mission is designed to study particle acceleration and heating in solar flares, we wish to have interdisciplinary discussions because we believe the scientific results of the PhoENiX mission will make a significant impact not only on solar physics but also on space physics and astrophysics. Examples of invited talks include “multi-wavelength observations of solar flares”, “roles of magnetic reconnection in high-energy phenomena in different plasma environments”, and “theory and simulations of particle acceleration and fundamental plasma processes”.
The meeting will be held during November 15-19, 2021 as a virtual, online-only event. The deadline for the abstract is 23:59 JST on October 19, 2021 while registration is open until November 15. For more information, please check the workshop website: https://indico.ipmu.jp/event/395/
Best regards
Mitsuo (on behalf of SOC)
Scientific Organizing Committee:
Lindsay Glesener, Fan Guo, Tomoko Kawate, Dmitry Khangulyan, Säm Krucker, Noriyuki Narukage, Mitsuo Oka, Kathy Reeves, Taro Sakao, Tadayuki Takahashi, Yohko Tsuboi
MAX MILLENNIUM NEWS
6 October 2021
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
Millennial oscillations of solar irradiance and magnetic field
at Earth in 600-2600
-- Valentina Zharkova
Plasma turbulence generated in 3D current sheet with magnetic islands
-- Zharkova V. and Xia, Q,
Simultaneous ALMA-Hinode-IRIS observations on footpoint signatures
of a soft X-ray loop-like microflare
-- Shimizu, T., Shimojo, M., and Abe, M.
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 keiji.yoshimura at montana.edu
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 416, “X-rays from a Type I Radio Burst,” by R. RAMESH. X-ray identification of the last remaining meter-wave burst type.
No. 417, “Manifold Nonthermality,” by Marina BATTAGLIA et al. Even weak events involve multple instances of nonthermality.
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 for these and others. Comments about specific flares can often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
29 September 2021
CONTENTS
1. CALL FOR PAPERS
"The Sun Seen with the ALMA - First Results"
2. E-PRINTS POSTED IN THE PAST WEEK
3. FROM THE EDITOR
=====================================================================
1. CALL FOR PAPERS
------------------
> From Costas Alissandrakis (calissan(a)uoi.gr)
Article collection on first results of solar observations with ALMA
We would like to draw the attention of colleagues and ask for contributions
to an article collection on "The Sun Seen with the Atacama Large mm and
sub-mm Array (ALMA) - First Results", to be published in Frontiers in
Astronomy and Space Sciences/Frontiers in Stellar and Solar Physics as a
Research Topic.
With the roll-out of solar observing capabilities in 2016, the Atacama
Large mm and sub-mm Array (ALMA) has been regularly observing the Sun with
unprecedented spatial (~1") and temporal resolution (1s) in this wavelength
range. The goal of this Research Topic is to make an assessment of what we
have learned so far from ALMA observations of the Sun and thus put in
perspective ALMA’s contribution to our understanding of the physical
processes in the solar atmosphere while, at the same time, serve as a guide
to future work. An additional goal is to identify
observational/computational aspects that need to be addressed and thus help
to improve the quality and value of the observations. To this end, it will
include both review articles and original works.
Submission deadlines: 29 October 2021 for abstracts, 28 February 2022 for manuscripts
Editors: Costas Alissandrakis, Tim Bastian, Masumi Shimojo and Alexander Nindos
For more information and submission details see
https://www.frontiersin.org/research-topics/24755/
2. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Multiple electron acceleration instances during a series of solar
-- Marina Battaglia, Rohit Sharma, Yingjie Luo, Bin Chen, Sijie Yu, Sam Krucker
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Successively Detected
in a Solar Eruption
-- Zhou, Xinping ; Shen, Yuandeng ; Su, Jiangtao ; Tang, Zehao ;
Zhou, Chengrui ; Duan, Yadan ; Tan, Song
Sympathetic Filament Eruptions within a Fan-spine Magnetic System
-- Zhou, Chengrui ; Shen, Yuandeng ; Zhou, Xinping ; Tang, Zehao ; Duan, Yadan ;
Tan, Song
3. 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 keiji.yoshimura at montana.edu
Dear colleagues,
Here is a workshop announcement that should be of interest to some of you.
Best regards,
--Pascal
The need for a high-performance solar radio telescope in the United
States has been recognized for many years. The FASR concept represents
such a telescope, one that provides high-resolution imaging over a broad
range of frequencies, sufficient to probe the solar atmosphere from the
mid-chromosphere to the mid-corona, with high time and spectral
resolution. EOVSA implemented many FASR design elements and, as such,
has served as a valuable pathfinder instrument, spectacularly validating
both the fundamental concept of time-resolved broadband imaging
spectroscopy and the science it enables. In the meantime, science and
technology have advanced and the need for full implementation of the
FASR concept has only grown more important
In anticipation of upcoming funding opportunities, this workshop is
being convened from 2021 Dec 1-3 to highlight progress in solar physics
over the past decade, and to take stock of the unique contributions
enabled by the current suite of new radio instruments, to refine the
science goals and requirements of a next-generation solar radio
facility. The workshop will provide a forum to discuss relevant new and
emerging technologies that will enable this new science. We invite
colleagues with an interest in solar physics and radio technology, and
from other fields that would stand to benefit, to help explore the
frontiers of science and technology that will guide updates and
refinements to the FASR concept.
The workshop will be virtual, hosted from the University of California
Berkeley's Space Sciences Laboratory (LOC: Pascal Saint-Hilaire, Milo
Buitrago-Casas, Jim McTiernan, Gelu Nita). The Scientific and Technical
Organizing Committee is composed of Marin Anderson (JPL), Tim Bastian
(NRAO), Bin Chen (NJIT), James Drake (UMD), Dale Gary (NJIT), Lindsay
Glesener (UMN), Gregg Hallinan (Caltech), Jonathon Kocz (UCB), Haosheng
Lin (U. Hawaii), Sophie Musset (ESA), Dan Werthimer (UCB). Website and
registration are at https://fasr21.ssl.berkeley.edu/. Deadline for
contributions is November 1st, 2021. There is no deadline for participation.
--
=======================================================================
Pascal Saint-Hilaire pascal(a)ssl.berkeley.edu
Space Sciences Laboratory phone: +510-643-4618
University of California, Berkeley
7 Gauss Way
Berkeley, CA-94720-7450 http://sprg.ssl.berkeley.edu/~shilaire/
=======================================================================