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RHESSI Nuggets in November 2020
by Hugh Hudson 24 Nov '20

24 Nov '20

http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets No. 393, “Self-Consistent Flare Model”, by Wenzhi RUAN and Rony KEPPENS: Energy trnasport by fast particles made self-consistent with MHD flare modeling. No. 394, “Probing the solar coronal heating function with slow magnetoacoustic waves," by Dmitriii KOLOTKOV et al.: Coronal heating models meet damped slow magnetoacoustic waves. No. 395. “What drives impulsive coronal heating?” by Pradeep CHITTA et al.: Impulsive footpoint emissions suggest magnetic reconnection in the chromosphere. 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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.

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Max Millennium News
by Keiji YOSHIMURA 18 Nov '20

18 Nov '20

MAX MILLENNIUM NEWS 18 November 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 Proper Orthogonal and Dynamic Mode Decomposition of Sunspot Data -- A. B. Albidah, W. Brevis, V. Fedun, I. Ballai, D. B. Jess, M. Stangalini, J. Higham and G. Verth 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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recent CESRA nuggets
by Eduard Kontar 17 Nov '20

17 Nov '20

Radio bursts in the 2017 September 6, X9.3 flare by M. Karlicky and J. Rybak http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2725 <http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2725> Magnetic Reconnection during the Post-impulsive Phase of a Long-duration Solar Flare by S. Yu et al. http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2711 <http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2711> -- 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/ <http://www.facebook.com/solarcesra/> and http://twitter.com/CESRA_community <http://twitter.com/CESRA_community>

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Max Millennium News
by Keiji YOSHIMURA 11 Nov '20

11 Nov '20

MAX MILLENNIUM NEWS 11 November 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 Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data -- Soshi Okamoto, Yuta Notsu, Hiroyuki Maehara, Kosuke Namekata, Satoshi Honda, Kai Ikuta, Daisaku Nogami, Kazunari Shibata Turbulent viscosity and effective magnetic Prandtl number from simulations of isotropically forced turbulence -- Petri J. Kapyla, Matthias Rheinhardt, Axel Brandenburg, Maarit J. Kapyla Time and Charge-Sign Dependence of the Heliospheric Modulation of Cosmic Rays -- O.P.M. Aslam, D. Bisschoff, M. D. Ngobeni, M. S. Potgieter, R. Munini, M. Boezio, & V. V. Mikhailov 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 04 Nov '20

04 Nov '20

MAX MILLENNIUM NEWS 4 November 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 Bayesian Analysis of Quasi-periodic Pulsations in Stellar Flares -- D. J. Pascoe, A. Smyrli, T. Van Doorsselaere, and A.-M. Broomhall Cause and Kinematics of a Jetlike CME -- Reetika Joshi, Yuming Wang, Ramesh Chandra, Quanhao Zhang, Lijuan Liu, Xiaolei Li The role of small-scale surface motions in the transfer of twist to a solar jet from a remote stable flux rope -- Reetika Joshi, Brigitte Schmieder, Guillaume Aulanier, veronique Bommier, Ramesh Chandra 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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RHESSI Nuggets in October 2020
by Hugh Hudson 25 Oct '20

25 Oct '20

No. 390, “Prediction of Solar Cycle 25”, by Leif SVALGAARD. Now we know how big the next solar maximum will be. No. 391, “Electric Current Neutralization and Eruption”, by Ellis AVALLONE and Xudong SUN. Coronal currents without neutralizing return currents correlate with eruption. No. 392, “Hot Flare Onsets”, by Hugh HUDSON et al. The pre-impulsive temperatures of solar flares are already hot, 10-15 MK. 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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.

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RHESSI Nuggets in October 2020
by Hugh Hudson 25 Oct '20

25 Oct '20

No. 390, “Prediction of Solar Cycle 25”, by Leif SVALGAARD. Now we know how big the next solar maximum will be. No. 391, “Electric Current Neutralizationand Eruption”, by Ellis AVALLONE and Xudong SUN. Coronal currents without neutralizing return currents correlate with eruption. No. 392, “Hot Flare Onsets”, by Hugh HUDSON et al. The pre-impulsive temperatures of solar flares are already hot, 10-15 MK. 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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.

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Max Millennium News
by Keiji YOSHIMURA 21 Oct '20

21 Oct '20

MAX MILLENNIUM NEWS 21 October 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 Sub-second time evolution of Type III solar radio burst sources at fundamental and harmonic frequencies -- X. Chen, E. P. Kontar, N. Chrysaphi, N. L.S. Jeffrey, M. Gordovskyy, Y. Yan, B. Tan Magnetically coupled atmosphere, fast sausage MHD waves, and forced magnetic field reconnection during the SOL2014-09-10T17:45 flare -- Hana Meszarosova and Peter Gomory 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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RHESSI Science Nuggets in September 2020
by Hugh Hudson 18 Oct '20

18 Oct '20

No. 388, “Submerged Flare Acoustic Sources,” by Juan Camilo BUITRAGA CASAS and Angel MARTINEZ: Flare acoustic radiation emanates from a source _inside_ the Sun. No. 389, “Flare/CME Cartoon Archive,” by Hugh HUDSON. A new edition of the Flare/CME Archive, now packing 0.4 kilotoons. 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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.

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Max Millennium News
by Keiji YOSHIMURA 14 Oct '20

14 Oct '20

MAX MILLENNIUM NEWS 14 October 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 Differential rotation of the solar corona: A new data-adaptive multiwavelength approach -- S. Mancuso, S. Giordano, D. Barghini, D. Telloni Magnetic Helicity Flux across Solar Active Region Photospheres: I. Hemispheric Sign Preference in Solar Cycle 24 -- Sung-Hong Park, K. D. Leka, Kanya Kusano 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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