MAX MILLENNIUM NEWS
22 July 2020
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
Statistical Analysis of the Relation between Coronal Mass Ejections
and Solar Energetic Particles
-- Kosuke Kihara, Yuwei Huang, Nobuhiko Nishimura, Nariaki V. Nitta,
Seiji Yashiro, Kiyoshi Ichimoto, Ayumi Asai
Magnetic Flux of Active Regions Determining the Eruptive Character
of Large Solar Flares
-- Ting Li, Yijun Hou, Shuhong Yang, Jun Zhang, Lijuan Liu, Astrid M. Veronig
ase study of multi-temperature coronal jets for emerging flux MHD models
-- Reetika Joshi, Ramesh Chandra, Brigitte Schmieder, Fernando Moreno-Insertis,
Guillaume Aulanier, Daniel Nobrega-Siverio, and Pooja Devi
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, to be held "mostly virtually." I wanted to invite you to consider submitting an abstract to the third-annual installment of our session for next-generation remote-sensing missions. This year the focus has been expanded to include all remote sensing, including imaging, spectroscopy, polarimetry, and combinations of those, plus anything else I'm missing.
Session link and description are below. Deadline is 11:59pm EDT on July 29th (next Wednesday).
We look forward to your exciting submissions!
https://agu.confex.com/agu/fm20/prelim.cgi/Session/103362
SH008 - 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
15 July 2020
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 STIX Aspect System (SAS): The Optical Aspect System
of the Spectrometer/Telescope for Imaging X-Rays (STIX) on Solar Orbiter
-- A. Warmuth, H. Önel, G. Mann, et al.
What determine Solar Flares Producing Interplanetary Type III Radio Bursts?
-- Y. K. Kou, Z. C. Jing, X. Cheng, W. Q. Pan, Y. Liu, C. Li, M. D. Ding
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 July 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
Ambipolar diffusion in the Bifrost code
-- D. Nobrega-Siverio, J. Martinez-Sykora, F. Moreno-Insertis, M. Carlsson
Modeling the quiet Sun cell and network emission with ALMA
-- C. E. Alissandrakis, A. Nindos, T. S. Bastian, S. Patsourakos
Clustering of fast Coronal Mass Ejections during the solar cycles 23 and 24
and implications for CME-CME interactions
-- Jenny M. Rodriguez Gomez, Tatiana Podladchikova, Astrid Veronig,
Alexander Ruzmaikin, Joan Feynman, Anatoly Petrukovich
Magnetic and Velocity Field Topology in Active Regions
of Descending Phase of the Solar Cycle 23
-- R. A. Maurya and A. Ambastha
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
No. 380: “Energy Transport by Accelerated Particles in the Quiet Solar Atmosphere”, by Lars Frogner, Boris Gudiksen, and Helle Bakke. A first study of non-thermal particles integrated into an MHD simulation of the solar atmosphere.
No. 381: “Extreme Ultraviolet Late Phase of Solar Flares”, by Rui LIU. Both arcade and circular-ribbon flares may sometimes spawn EUV late phase emission.
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 be found by searching for their SOLyyyy-mm-dd identifier from this home page.
No. 380: “Energy Transport by Accelerated Particles in the Quiet Solar Atmosphere”, by Lars Frogner, Boris Gudiksen, and Halle Bakke. A first study of non-thermal particles integrated into an MHD simulation of the solar atmosphere.
No. 381: “Extreme Ultraviolet Late Phase of Solar Flares”, by Rui LIU. Both arcade and circular-ribbon flares may sometimes spawn EUV late phase emission.
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 be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
24 June 2020
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
Numerical simulation of solar photospheric jet-like phenomena
caused by magnetic reconnection
-- Yuji Kotani, Kazunari Shibata
Solar Flare-CME Coupling Throughout Two Acceleration Phases of a Fast CME
-- Tingyu Gou, Astrid M. Veronig, Rui Liu, Bin Zhuang, Mateja Dumbovic,
Tatiana Podladchikova, Hamish A. S. Reid, Manuela Temmer, Karin Dissauer,
Bojan Vrsnak, Yuming Wang
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
17 June 2020
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
A new method for estimating global coronal wave properties from their
interaction with solar coronal holes
-- I. Piantschitsch, J. Terradas, M. Temmer
Machine-learning approach to identification of coronal holes in solar disk
images and synoptic maps
-- Egor Illarionov, Alexander Kosovichev, Andrey Tlatov
Multilevel Observations of the Oscillations in the First Active Region
of the New Cycle
-- Andrei Chelpanov and Nikolai Kobanov
Standing MHD Waves in a Magnetic Slab Embedded in an Asymmetric Magnetic
Plasma Environment: Surface Waves
-- William Oxley, Noemi Kinga Zsamberger, Robert Erdelyi
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
No. 380, "Energy transport by accelerated particles in the quiet solar atmosphere,” by Lars Frogner, Boris Gudiksen, and Helle Bakke. A first study of non-thermal particles integrated into an MHD simulation of the solar atmosphere. Click the title to read more.
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 be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
10 June 2020
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
A new facility for airborne solar astronomy: NASA's WB-57
at the 2017 total solar eclipse
-- Amir Caspi, Daniel B. Seaton, Constantine C. C. Tsang, Craig E. DeForest,
Paul Bryans, Edward E. DeLuca, Steven Tomczyk, Joan T. Burkepile,
Thomas 'Tony' Casey, John Collier, Donald 'DD' Darrow, Dominic Del Rosso,
Daniel D. Durda, Peter T. Gallagher, Leon Golub, Matthew Jacyna,
David 'DJ' Johnson, Philip G. Judge, Cary 'Diddle' Klemm, Glenn T. Laurent,
Johanna Lewis, Charles J. Mallini, Thomas 'Duster' Parent, Timothy Propp,
Andrew J. Steffl, Jeff Warner, Matthew J. West, John Wiseman, Mallory Yates,
Andrei N. Zhukov, and the NASA WB-57 2017 Eclipse Observing Team
MinXSS-2 CubeSat mission overview: Improvements from the successful
MinXSS-1 mission
-- James Paul Mason, Thomas N. Woods, Phillip C. Chamberlin, Andrew Jones,
Rick Kohnert, Bennet Schwab, Robert Sewell, Amir Caspi, Christopher S. Moore,
Scott Palo, Stanley C. Solomon, Harry Warren
Lyman alpha Variability During Solar Flares Over Solar Cycle 24
Using GOES-15/EUVS-E
-- Ryan O. Milligan, Hugh S. Hudson, Phillip C. Chamberlin, Iain G. Hannah,
Laura A. Hayes
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