MAX MILLENNIUM NEWS
6 September 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
Deciphering The Slow-rise Precursor of a Major Coronal Mass Ejection
-- Cheng, X.; Xing, C.; Aulanier, G.; Solanki, S. K.; Peter, H.; Ding, M. D.
Three-dimensional Turbulent Reconnection within Solar Flare Current Sheet
-- Wang, Yulei; Cheng, Xin; Ding, Mingde; Liu, Zhaoyuan; Liu, Jian; Zhu, Xiaojue
Sequential Remote Brightenings and Co-spatial Fast Downflows
during Two Successive Flares
-- Bitao Wang, Xin Cheng, Chuan Li, Jun Chen, Mingde Ding
A Model for Confined Solar Eruptions Including External Reconnection
-- Chen, Jun; Cheng, Xin; Kliem, Bernhard; Ding, MingDe
The eruption of a magnetic flux rope observed by Solar Orbiter and Parker Solar Probe
-- David M. Long, Lucie M. Green, Francesco Pecora, David H. Brooks,
Hanna Strecker, David Orozco-Suarez, Laura A. Hayes, Emma E. Davies,
Ute V. Amerstorfer, Marilena Mierla, David Lario, David Berghmans,
Andrei N. Zhukov, Hannah T. Rudisser
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
30 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
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
MAX MILLENNIUM NEWS
26 July 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
New cases of super-flares on slowly rotating solar-type stars
and large amplitude super-flares in G- and M-type main-sequence stars
-- A. K. Althukair, D. Tsiklauri
Constraints on the variable nature of the slow solar wind
with the Wide-Field Imager on board the Parker Solar Probe
-- Patsourakos, S., Vourlidas, A., Nindos, A.
Prediction of short stellar activity cycles using derived and established
empirical relations between activity and rotation periods
-- A. K. Althukair, D. Tsiklauri
Torsional oscillations within a magnetic pore in the solar photosphere
-- Marco Stangalini, Robertus Erdelyi, Callum Boocock, David Tsiklauri,
Christopher J. Nelson , Dario Del Moro, Francesco Berrilli
and Marianna B. Korsos
Stereoscopic disambiguation of vector magnetograms:
first applications to SO/PHI-HRT data
-- G. Valori, D. Calchetti, A. Moreno Vacas, E. Pariat, S.K. Solanki,
P. Loschl, J. Hirzberger, S. Parenti, K. Albert, N. Albelo Jorge,
A. Alvarez-Herrero, T. Appourchaux, L.R. Bellot Rubio, J. Blanco Rodriguez,
A. Campos-Jara, A. Feller, A. Gandorfer, P. Garcia Parejo, D. Germerott,
L. Gizon, J.M. Gomez Cama, L. Guerrero, P. Gutierrez-Marques, F. Kahil,
M. Kolleck, A. Korpi-Lagg, D. Orozco Suarez, I. Perez-Grande,
E. Sanchis Kilders, J. Schou, U. Schuhle, J. Sinjan, J. Staub, H. Strecker,
J.C. del Toro Iniesta, R. Volkmer, J. Woch
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,
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
Dear Colleagues,
We would like to invite all of you to submit presentations to
the AGU session “Solar Flare Onset and Energy Release” at the AGU Fall
Meeting in San Francisco, CA on Dec. 11-15. The deadline for submitting an
abstract is Aug. 2.
Link to the session description and abstract submission:
https://agu.confex.com/agu/fm23/prelim.cgi/Session/188262.
Invited Speakers:
Vanessa Polito (Bay Area Environmental Research Institute)
Xiaocan Li (Dartmouth College).
We look forward to seeing you in San Francisco!
Organizers: Joel Dahlin, Jim Drake, Fan Guo, Kathy Reeves & Julie Vievering
- Joel Dahlin