Dear All
We are announcing an online science meeting on "Particle Acceleration in Solar Flares and the Plasma Universe" to 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. 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
8 September 2021
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
Global Nature of Solar Coronal Shock Waves shown by Inconsistency
between EUV Waves and Type II Radio Bursts
-- Aarti Fulara, Ryun-Young Kwon
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
1 September 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Solar surges related to UV bursts: Characterization through k-means,
inversions and density diagnostics
-- D. Nobrega-Siverio, S. L. Guglielmino, A. Sainz Dalda
A revised cone model and its application to non-radial prominence eruptions
-- Q. M. Zhang
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. 414, “Confined or Eruptive?”, by Ting LI, Anqin CHEN, Yijun HOU, Astrid M. VERONIG, Shuhong YANG, and Jun ZHANG: Increased magnetic flux reduces the eruptivity of a solar active region.
No. 415, “Do Hot Onsets Predict Flare Magnitudes”? by Hugh HUDSON: Maybe we can tell how big a flare is going to be from its initial development.
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
25 August 2021
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
Zonal harmonics of solar magnetic field for solar cycle forecast
-- V.N. Obridko, D.D. Sokoloff, V.V. Pipin, A.S. Shibalvaa, I.M. Livshits
TESS observations of flares and quasi-periodic pulsations from low mass stars
and potential impact on exoplanets
-- Gavin Ramsay, Dmitrii Kolotkov, Gerry Doyle, Lauren Doyle
Kink oscillations of coronal loops
-- V. M. Nakariakov, S. A. Anfiinogentov, P. Antolin, R. Jain, D. Y. Kolotkov,
E. G. Kupriyanova, D. Li, N. Magyar, G. Nistico, D. J. Pascoe,
A. K. Srivastava, J. Terradas, S. Vasheghani Farahani, G. Verth, D. Yuan,
I. V. Zimovets
First Frequency-Time-Resolved Imaging Spectroscopy Observations
of Solar Radio Spikes
-- Daniel L. Clarkson, Eduard P. Kontar, Mykola Gordovskyy, Nicolina Chrysaphi,
Nicole Vilmer
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
18 August 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. SERVER MAINTENANCE
3. 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
Magnetic Flux and Magnetic Non-potentiality of Active Regions
in Eruptive and Confined Solar Flares
-- Ting Li, Anqin Chen, Yijun Hou, Astrid M. Veronig, Shuhong Yang and Jun Zhang
Observations of shock propagation through turbulent plasma in the solar corona
-- Eoin P. Carley, Baptiste Cecconi, Hamish A. Reid, Carine Briand,
Sasikumar Raja, Sophie Masson, Vladimir V. Dorovskyy, Caterina Tiburzi,
Nicole Vilmer, Pietro Zucca, Philippe Zarka, Michel Tagger,
Jean-Mathias Griessmeier, Stéphane Corbel, Gilles Theureau, Alan Loh,
Julien Girard
The Formation and Lifetime of Outflows in a Solar Active Region
-- David H. Brooks, Louise Harra, Stuart D. Bale, Krzysztof Barczynski,
Cristina Mandrini, Vanessa Polito, and Harry P. Warren
Localised acceleration of energetic particles by a weak shock in the solar corona
-- Long, D. M., Reid, H. A. S., Valori, G., O'Kane, J.
2. SERVER MAINTENANCE
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The server for the E-print archive and the MMScience e-mail list will be down
from 16:00UT on 2021/08/20 due to maintenance work. It will take, at least,
a few hours before the server will be back.
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
MAX MILLENNIUM NEWS
11 August 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
Stereoscopic Measurements of Coronal Doppler Velocities
-- O, Podladchikova, L. Harra, K.Barczynski, C.Mandrini, F. Auchere,
D. Berghmans, E. Buchlin, L. Dolla, M. Mierla, S. Parenti, L. Rodriguez
Multi-wavelength Observations of a Metric Type-II Event
-- Alissandrakis, C. E. ; Nindos, A. ; Patsourakos, S. ; Hillaris, A.
A physics-based method that can predict imminent large solar flares
-- Kanya Kusano, Tomoya Iju, Yumi Bamba, Satoshi Inoue
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
4 August 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
The Solar Memory From Hours to Decades
-- Aschwanden, M.J. and Johnson, J.R.
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 colleagues,
A reminder that AGU abstracts are due tomorrow -- Wednesday, Aug 4 -- at 11:59pm EDT. If you have not yet done so, please consider submitting to our next-generation solar session, SH017. Any and all submissions are welcome, and I am happy to answer questions if you have any.
Details and link are below.
Cheers!
--- Amir
On 07/27/2021, 10:42 AM, "Amir Caspi" <amir(a)boulder.swri.edu> wrote:
Dear colleagues,
There is one week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the fourth-annual installment of our session for next-generation remote-sensing missions. Like last year, this year the focus includes all remote sensing, including imaging, spectroscopy, polarimetry, and combinations of those, plus anything else I'm missing. Given the imminent Decadal Survey, we encourage submissions with an eye both for near-term _and_ long-term (decadal or beyond) timescales for development.
Session link and description are below. Deadline is 11:59pm EDT on Aug 4th (next Wednesday).
We look forward to your exciting submissions!
https://agu.confex.com/agu/fm21/prelim.cgi/Session/121896
SH017 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond
Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; MinXSS; SphinX; the FOXSI, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories such as NuSTAR, Fermi, ALMA, and VLA, have significantly advanced our understanding of these phenomena. They have also shown the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes.
This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot and non-thermal) aspects of the Sun, and the science enabled by such new observations.
--- Amir Caspi, Lindsay Glesener, Jenna Samra, & Athiray Panchapakesan
MAX MILLENNIUM NEWS
28 July 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Solar chromosphere heating and generation of plasma outflows
by impulsively generated two-fluid Alfven waves
-- M. Pelekhata, K. Murawski, S. Poedts
Radio evidence for a shock wave reflected by a coronal hole
-- S. Mancuso, A. Bemporad, F. Frassati, D. Barghini, S. Giordano, D. Telloni,
C. Taricco
Hemispheric sunspot numbers 1874 - 2020
-- A.M. Veronig, S. Jain, T. Podladchikova, W. Potzi, F. Clette
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