MAX MILLENNIUM NEWS
30 August 2023
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
Comprehensive radiative MHD simulations of eruptive flares
above collisional polarity inversion lines
-- Matthias Rempel, Georgios Chintzoglou, Mark C.M. Cheung, Yuhong Fan,
Lucia Kleint
An Anisotropic Density Turbulence Model from the Sun to 1 au
Derived From Radio Observations
-- Kontar, Eduard P. ; Emslie, A. Gordon ; Clarkson, Daniel L. ; Chen, Xingyao ;
Chrysaphi, Nicolina ; Azzollini, Francesco ; Jeffrey, Natasha L. S. ;
Gordovskyy, Mykola
Comparison of damping models for kink oscillations of coronal loops
-- Zhong, Y., Kolotkov, D.Y., Zhong, S., Nakariakov, V.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
MAX MILLENNIUM NEWS
23 August 2023
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
On the three-dimensional relation between the coronal dimming,
erupting filament and CME. Case study of the 28 October 2021 X1.0 event
-- Chikunova, G., Podladchikova, T., Dissauer, K., Veronig, A. M.,
Dumbovic, M., Temmer, M., Dickson E. C.
Polarisation of decayless kink oscillations of solar coronal loops
-- Zhong, S., Nakariakov, V.M., Kolotkov, D.Y., Chitta, L.P., Antolin, P.,
Verbeeck, C., Berghmans, D.
CME Propagation Through the Heliosphere:
Status and Future of Observations and Model Development
-- M. Temmer, C. Scolini, I. G. Richardson, S. G. Heinemann, E. Paouris,
A. Vourlidas, M. M. Bisi, et al.
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
16 August 2023
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
30-min Decayless Kink Oscillations in a Very Long Bundle of
Solar Coronal Plasma Loops
-- Sihui Zhong, Valery M. Nakariakov, Yuhu Miao, Libo Fu, Ding Yuan
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
2 August 2023
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 Role of High-Frequency Transverse Oscillations in Coronal Heating
-- Daye Lim, Tom Van Doorsselaere, David Berghmans, Richard J. Morton,
Vaibhav Pant, and Sudip Mandal
ARTop: an open-source tool for measuring Active Region Topology
at the solar photosphere
-- K. Alielden, D. MacTaggart, Q. Ming, C. Prior and B. Raphaldini
Spectral Observations and Modeling of a Solar White-light Flare
Observed by CHASE
-- De-Chao Song, Jun Tian, Y. Li, M. D. Ding, Yang Su, Sijie Yu, Jie Hong,
Ye Qiu, Shihao Rao, Xiaofeng Liu, Qiao Li, Xingyao Chen, Chuan Li, Cheng Fang
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 gentle reminder that there is just one day left to submit abstracts to AGU (due tomorrow, Weds, Aug 2 at 11:59pm ET). We hope you'll consider session SH011, details below. =)
Thanks!
--- Amir
On 07/26/2023, 9:57 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 6th (!) annual installment of our session for next-generation missions, instruments, technology, and science studying high-energy processes on the Sun. This includes theory/modeling to drive new measurements/missions!
We welcome a broad range of topics on missions, mission concepts, enabling technology, new measurements/data, driving theories and models ... and especially encourage an eye for medium- and long-term outlook.
Deadline to submit is 11:59pm EDT on Aug 2nd (next Wednesday). Session/submission link and description are below, for your reference.
We look forward to your exciting submissions!
https://agu.confex.com/agu/fm23/prelim.cgi/Session/188319
SH011 - 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; SolO; MinXSS; SphinX; Chandrayaan-2; the FOXSI, MaGIXS, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories including NuSTAR, Fermi, ALMA, and VLA; have significantly advanced our understanding of these phenomena. They have also highlighted 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/non-thermal) aspects of the Sun, and the science enabled by such new observations.
--- Amir Caspi, on behalf of Chris Moore, Julie Vievering, P.S. Athiray, Shaheda Begum Shaik