MMScience July 2024

mmscience@solar.physics.montana.edu

3 participants
6 discussions

Max Millennium News
by Keiji YOSHIMURA 31 Jul '24

31 Jul '24

MAX MILLENNIUM NEWS 31 July 2024 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 Multiwavelength Study of on-disk Coronal Hole Jets with IRIS and SDO observations -- Myrto Koletti, Costis Gontikakis, Spiros Patsourakos, Kanaris Tsinganos 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

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Max Millennium News
by Keiji YOSHIMURA 24 Jul '24

24 Jul '24

MAX MILLENNIUM NEWS 24 July 2024 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 Hard X-rays from the deep solar atmosphere: An unusual UV burst with flare properties -- L. P. Chitta, I. G. Hannah, L. Fletcher, H. S. Hudson, P. R. Young, S. Krucker, H. Peter Modeling Time-Variable Elemental Abundances in Coronal Loop Simulations -- Jeffrey W. Reep, John Unverferth, Will T. Barnes, Sherry Chhabra Giant post-flare loops in active regions with extremely strong coronal magnetic fields -- Costas E. Alissandrakis, Gregory D. Fleishman, Viktor V. Fedenev, Stephen M. White, Alexander T. Altyntsev 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

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2024 AGU Session on high-energy solar remote-sensing missions/instruments
by Amir Caspi 23 Jul '24

23 Jul '24

Dear colleagues, There is just over 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 7th (!) 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 July 31 (next Wednesday). Session/submission link and description are below, for your reference. We look forward to your exciting submissions! https://agu.confex.com/agu/agu24/prelim.cgi/Session/227061 SH016 - 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, Milo Buitrago-Casas

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Max Millennium News
by Keiji YOSHIMURA 17 Jul '24

17 Jul '24

MAX MILLENNIUM NEWS 17 July 2024 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 Direct Imaging of a Prolonged Plasma/Current Sheet and Quasiperiodic Magnetic Reconnection on the Sun -- Pankaj Kumar, Judith T. Karpen, Vasyl Yurchyshyn, C. Richard DeVore, Spiro K. Antiochos Study of Particle Acceleration Using Fine Structures and Oscillations in Microwaves from the Electron Cyclotron Maser -- Rohit Sharma, Marina Battaglia, Sijie Yu, Bin Chen, Yingjie Luo, and Sam Krucker ENSO Index Variations and Links with Solar and Volcanic Activity -- V. Zharkova and I. Vasilieva 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

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Max Millennium News
by Keiji YOSHIMURA 03 Jul '24

03 Jul '24

MAX MILLENNIUM NEWS 3 July 2024 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 fast-filament eruption observed in the Hα spectral line. I. Imaging spectroscopy diagnostic -- Denis P. Cabezas, Kiyoshi Ichimoto, Ayumi Asai, Satoru UeNo, Satoshi Morita, Ken-ichi Otsuji, Kazunari Shibata 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

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CESRA solar radio science nuggets in June
by Eduard Kontar 02 Jul '24

02 Jul '24

Energetics of compressive waves in the solar corona by Francesco Azzollini et al https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3783 Data Release of Solar Radio Bursts observed by CBSm at the metric wavelength by Yao Chen et al. https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3773 --- CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are short communications written in language accessible to a non-expert in the specific area and designed to keep solar and heliophysics communities informed and up-to-date about current research. The highlights can be followed, discussed, commented and shared via http://www.facebook.com/solarcesra/ andhttp://twitter.com/CESRA_community

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