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Announcing four new RHESSI Nugget
by Hugh Hudson 06 Nov '19

06 Nov '19

No. 360: “Searching SOLfully within the Nuggets”, by Hugh Hudson. Using the SOL nomenclature is a good thing. No. 361: “Non-radial jets on the edges of active regions,” by Peter Wyper. The very common jet structures that we see can naturally combine twist and breakout. No. 362: “Can magnetic reconnection cause solar rainstorms?” by Petra Kohutova. Impulsive heating resulting from coronal reconnectino can trigger rain. No.363: “Flare waiting times depend on their magnitudes,” by Hugh Hudson. Surprising new evidence for the build-up and release process. 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.

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Max Millennium News
by Keiji YOSHIMURA 30 Oct '19

30 Oct '19

MAX MILLENNIUM NEWS 30 October 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 A Very Narrow RHESSI X-ray Flare on 25 September 2011 -- Brian R. Dennis, Anne K. Tolbert First Detection of Plasmoids from Breakout Reconnection on the Sun -- Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos, Peter F. Wyper, C. Richard DeVore 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 23 Oct '19

23 Oct '19

MAX MILLENNIUM NEWS 23 October 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 A New Type of Jets in a Polar Limb of Solar Coronal Hole -- Il-Hyun Cho, Yong-Jae Moon, Kyung-Suk Cho, Valery M. Nakariakov, Jin-Yi Lee, Yeon-Han Kim First imaging spectroscopy observations of solar drift pair bursts -- Alexey Kuznetsov, Eduard Kontar Round-Trip Slipping Magnetic Reconnection Observed in a Fan-Spine Jet -- Yuandeng Shen; Zhining Qu; Chengrui Zhou; Yadan Duan; Zehao Tang; 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

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Max Millennium News
by Keiji YOSHIMURA 16 Oct '19

16 Oct '19

MAX MILLENNIUM NEWS 16 October 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 A global two-scale helicity proxy from pi-ambiguous solar magnetic fields -- Axel Brandenburg Multi-layered Kelvin-Helmholtz Instability in the Solar Corona -- Ding Yuan, Yuandeng Shen, Yu Liu, Xueshang Feng, Rony Keppens Magnetohydrodynamic Seismology of Quiet Solar Active Regions -- Sergey A. Anfinogentov; Valery M. Nakariakov 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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Announcing recent RHESSI Science Nuggets
by Hugh Hudson 13 Oct '19

13 Oct '19

No. 358: “The Last Best Flares”, by Hugh Hudson, Ed Cliver, and Brian Dennis. Major flares tend to happen at the very ends of sunspot cycles. No. 359: “Submillimeter Radiation as the Thermal Component of the Neupert Effect,” by Guigue Giménez de Castro: Flare emission at the highest radio frequencies can be bremsstrahlung. No. 360: “Searching SOLfully within the Nuggets,“ by Hugh Hudson: The IAU identifier works well for finding items about a particular event. No. 361: “Non-radial jets on the edges of active regions,” by Peter Wyper: The very common jet structures we see can naturally combine twist and breakout. 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.

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Max Millennium News
by Keiji YOSHIMURA 09 Oct '19

09 Oct '19

MAX MILLENNIUM NEWS 9 October 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 Test magnetohydrostatic extrapolation with radiative MHD simulation of a solar flare -- Xiaoshuai Zhu & Thomas Wiegelmann 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 02 Oct '19

02 Oct '19

MAX MILLENNIUM NEWS 2 October 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 Real-time solar image classification: assessing spectral, pixel-based approaches -- J. Marcus Hughes, Vicki W. Hsu, Daniel B. Seaton, Hazel M. Bain, Jonathan M. Darnel, Larisza Krista Modelling Mg II During Solar Flares. II. Non-equilibrium Effects -- Kerr, Graham S., Carlsson, Mats and Allred, J.C. Calibration of the Instrumental Crosstalk for the Near-IR Imaging Spectropolarimeter at the NST -- K. Ahn and W. Cao On the Source Position and Duration of a Solar Type III Radio Burst Observed by LOFAR -- PeiJin Zhang, SiJie Yu, Eduard Kontar, ChuanBing 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

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Announcing RHESSI Nuggets in September 2019
by Hugh Hudson 02 Oct '19

02 Oct '19

No. 356: “EVE-RHESSI DEM Models and the Low-Energy Cutoff for Non-thermal Electrons”, by Jim McTiernan. Characterizing flare temperature distributions helps to define the non-thermal energy release. No. 357: “Dynamic Processes of the Moreton Wave on 2014 March 29”, by Denis Cabezas and the FMT team. A beautiful chromospheric wave was excited by the best-observed flare ever. No. 358: “The Last Best Flares”, by Hugh Hudson, Ed Cliver, and Brian Dennis. Major flares tend to happen at the very ends of sunspot cycles. No. 359: “Submillimeter Radiation as the Thermal Component of the Neupert Effect.” Flare emission at the highest radio frequencies can be bremsstrahlung. 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.

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Max Millennium News
by Keiji YOSHIMURA 25 Sep '19

25 Sep '19

MAX MILLENNIUM NEWS 25 September 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 Determination of transport coefficients by coronal seismology of flare-induced slow-mode waves: Numerical parametric study of 1D loop model -- Tongjiang Wang, Leon Ofman The Eruption of Outer Spine-like Loops Leading to a Double-stage Circular-ribbon Flare -- Chang Liu, Jeongwoo Lee, and Haimin Wang Non-Stationary Fast-Driven Self-Organized Criticality in Solar Flares -- Markus J. Aschwanden Global Energetics of Solar Flares. IX. Refined Magnetic Modeling -- Markus J. Aschwanden 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 18 Sep '19

18 Sep '19

MAX MILLENNIUM NEWS 18 September 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 The Solar Orbiter SPICE instrument - An extreme UV imaging spectrometer -- The SPICE Consortium 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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