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Max Millennium News
by Keiji YOSHIMURA 17 Apr '19

17 Apr '19

MAX MILLENNIUM NEWS 17 April 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 Why Does the Solar Corona Abnormally Rotate Faster Than the Photosphere? -- KJ Li, JC Xu, ZQ Yin, W Feng Impacts On Proton Fluxes Observed During Different Interplanetary Conditions -- Binod Adhikari, Niraj Adhikari, Binil Aryal, Narayan P. Chapagain, and Ildiko Horvath Coronal Loop Seismology Using Standing Kink Oscillations With a Lookup Table -- David J. Pascoe, Alan W. Hood and Tom Van Doorsselaere Data-Optimized Coronal Field Model: I. Proof of Concept -- K. Dalmasse, A. Savcheva, S. E. Gibson, Y. Fan, D. W. Nychka, N. Flyer, N. Mathews, E. E. DeLuca Coronal Bright Points -- Maria S. Madjarska 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 canfield at physics.montana.edu

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Max Millennium News
by Keiji YOSHIMURA 10 Apr '19

10 Apr '19

MAX MILLENNIUM NEWS 10 April 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 Difference of source regions between fast and slow coronal mass ejections -- B. Filippov Invited Review: Signatures of Magnetic Flux Ropes in the Low Solar Atmosphere Observed in High Resolution -- Haimin Wang and Chang Liu 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 canfield at physics.montana.edu

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Max Millennium News
by richard.canfield＠montana.edu 03 Apr '19

03 Apr '19

MAX MILLENNIUM NEWS 03 April 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 Do Kepler superflare stars really include slowly-rotating Sun-like stars ? - Results using APO 3.5m telescope spectroscopic observations and Gaia-DR2 data -- Yuta Notsu, Hiroyuki Maehara, Satoshi Honda, Suzanne L. Hawley, James R. A. Davenport, Kosuke Namekata, Shota Notsu, Kai Ikuta, Daisaku Nogami, Kazunari Shibata Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona -- Pakorn Wongwaitayakornkul, Magnus A. Haw, Hui Li, Paul M. Bellan Magnetic Field Dynamics and Varying Plasma Emission in Large-scale Coronal Loops -- S. Sahin, V. Yurchyshyn , P. Kumar, A. Kilcik, K. Ahn, and X. Yang Nonlinear Evolution of Ion Kinetic Instabilities in the Solar Wind -- Leon Ofman What determines the X-ray intensity and duration of a solar flare? -- Jeffrey W. Reep & Kalman J. Knizhnik 2. FROM THE EDITOR ================== The Max Millennium program exists to enhance all aspects of solar activity 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 richard.canfield at montana.edu

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CESRA nuggets in March 2019
by Eduard Kontar 02 Apr '19

02 Apr '19

Large area solar flare ribbons as the model to explain puzzling millimeter emission by G.G. Motorina et al.* http://cesra.net/?p=2157 Short-period Waves in Flare Loops: Possible Vehicle for Flare Energy Transport by Sijie Yu et al http:/cesra.net/?p=2166

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Max Millennium News
by richard.canfield＠montana.edu 27 Mar '19

27 Mar '19

MAX MILLENNIUM NEWS 27 March 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 Fast Magnetoacoustic Wave Trains with Time-dependent Drivers -- Goddard, C. R., Nakariakov, V. M., Pascoe, D. J. 2. FROM THE EDITOR ================== The Max Millennium program exists to enhance all aspects of solar activity 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 richard.canfield at montana.edu

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RHESSI Nuggets in March 2019
by Hugh Hudson 24 Mar '19

24 Mar '19

No. 347, “Persistent quasi-periodic pulsations detected during the large X8.2 solar flare,” by Laura Hayes and Peter Gallagher: The most beautiful flare has the most beautiful pulsations! No. 346, “Is the coronal magnetic field braiding?” by Markus Aschwanden. An iconic cartoon does not relate well to the observations. 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

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Max Millennium News
by richard.canfield＠montana.edu 20 Mar '19

20 Mar '19

MAX MILLENNIUM NEWS 20 March 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 Three-dimensional reconstruction of CME-driven shock-streamer interaction from radio observations: a different take on the diagnostics of coronal magnetic fields -- S. Mancuso, F. Frassati, A. Bemporad, D. Barghini The soft X-ray spectrometer polarimeter SolpeX -- J. Sylwester; M. Steslicki; J. Bakala; S. Plocieniak; Å. Szaforz; M. Kowalinski; D. Scislowski; P. PodgÃ³rski; T. Mrozek; J. Barylak; A. Makowsk; M. Siarkowski; Z. Kordylewski; B. Sylwester; S. Kuzin; A. Kirichenko; A. Pertsov; S. Bogachev Variable emission mechanism of a Type IV radio burst -- D. E. Morosan, E. K. J. Kilpua, E. P. Carley, and C. Monstein Inference of magnetic field strength and density from damped transverse coronal waves -- I. Arregui, M. Montes-Solis, A. Asensio Ramos 2. FROM THE EDITOR ================== The Max Millennium program exists to enhance all aspects of solar activity 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 richard.canfield at montana.edu

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Max Millennium News
by richard.canfield＠montana.edu 13 Mar '19

13 Mar '19

MAX MILLENNIUM NEWS 13 March 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 Frequency-Distance Structure of Solar Radio Sources Observed by LOFAR -- Mykola Gordovskyy, Eduard Kontar, Philippa Browning, and Alexey Kuznetsov The birth of a coronal mass ejection -- Tingyu Gou, Rui Liu, Bernhard Kliem, Yuming Wang, and Astrid M. Veronig 2. FROM THE EDITOR ================== The Max Millennium program exists to enhance all aspects of solar activity 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 richard.canfield at montana.edu

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CESRA Workshop 2019: - registration and abstract submission are open
by Eduard Kontar 13 Mar '19

13 Mar '19

Dear Colleagues, We are pleased to announce registration/abstract submission for the next CESRA Workshop, “CESRA2019: The Sun and the inner heliosphere” which will be held on July 8th – 12th, 2019, at Telegrafenberg, Potsdam, Germany. http://meetings.aip.de/cesra2019/cms/ CESRA, the Community of European Solar Radio Astronomers, organizes triennial workshops on investigations of the solar atmosphere using radio and other observations. Although special emphasis is given to radio diagnostics, the workshop topics are of interest to a large community of solar physicists. The format of the workshop will combine plenary sessions and working group sessions, with invited review talks, oral contributions, and posters. To register and to submit the abstract please follow the link: http://meetings.aip.de/cesra2019/registration/ The CESRA 2019 workshop will place an emphasis on linking the Sun with the heliosphere, motivated by the launch of Parker Solar Probe in 2018 and the upcoming launch of Solar Orbiter in 2020. It will provide the community with a forum for discussing the first relevant science results and future science opportunities, as well as on opportunity for evaluating how to maximize science return by combining space-borne observations with the wealth of data provided by new and future ground-based radio instruments, such as ALMA, E-OVSA, EVLA, LOFAR, MUSER, MWA, and SKA, and by the large number of well-established radio observatories. On behalf of the CESRA Board and the local SOC representatives, Eduard Kontar, Gottfried Mann, Alexander Warmuth

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Max Millennium News
by richard.canfield＠montana.edu 06 Mar '19

06 Mar '19

MAX MILLENNIUM NEWS 06 March 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 Properties of slow magnetoacoustic oscillations of solar coronal loops by multi-instrumental observations -- Nakariakov, V. M., Kosak, M. K., Kolotkov, D. Y., Anfinogentov, S. A., Kumar, P., Moon, Y.-J. Persistent Quasi-Periodic Pulsations During a Large X-Class Solar Flare -- Laura A. Hayes, Peter T. Gallagher, Brian R. Dennis, Jack Ireland, Andrew Inglis, and Diana E. Morosan Magnetic helicity and fluxes in an inhomogeneous α squared dynamo -- A. Brandenburg Properties of the Diffuse Emission around Warm Loops in Solar Active Regions -- David H. Brooks Comparative Study of Microwave Polar Brightening, Coronal Holes, and Solar Wind Over the Solar Poles -- Ken'ichi Fujiki, Kiyoto Shibasaki, Seiji Yashiro, Munetoshi Tokumaru, Kazumasa Iwai, Satoshi Masuda 3He-rich Solar Energetic Particles from Sunspot Jets -- Radoslav Bucik, Mark E. Wiedenbeck, Glenn M. Mason, Raul Gomez-Herrero, Nariaki V. Nitta, Linghua Wang Relative magnetic field line helicity -- K. Moraitis, E. Pariat, G. Valori, K. Dalmasse Forbush decreases and Geomagnetic Storms during a Highly Disturbed Solar and Interplanetary Period, 4-10 September 2017 -- B. Badruddin, O. P. M. Aslam, M. Derouich, H. Asiri and K. Kudela 2. FROM THE EDITOR ================== The Max Millennium program exists to enhance all aspects of solar activity 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 richard.canfield at montana.edu

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