MMScience April 2019

mmscience@solar.physics.montana.edu

4 participants
7 discussions

CESRA2019 workshop - deadline May 1, 2019
by Eduard Kontar 25 Apr '19

25 Apr '19

Dear CESRA Colleagues, Please note the approaching deadline for CESRA2019 workshop - May 1, 2019 https://meetings.aip.de/cesra2019/cms/registration/ If you have not submitted abstract/registered please do so now. The details are below: ******************** 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. https://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: https://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 -- The CESRA highlights can be followed, discussed etc at https://twitter.com/CESRA_community https://www.facebook.com/solarcesra/

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Max Millennium News
by Keiji YOSHIMURA 24 Apr '19

24 Apr '19

MAX MILLENNIUM NEWS 24 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 Flare reconnection-driven magnetic field and Lorentz force variations at the Sun's surface -- Krzysztof Barczynski, Guillaume Aulanier, Sophie Masson, Michael S. Wheatland 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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RHESSI Nuggets in April 2019
by Hugh Hudson 23 Apr '19

23 Apr '19

No. 349, “Warm UV Loops Heated by Small-Scale Cancellation Events,” by S. Şahin and V. Yurchyshyn: Precisely locating warm coronal loops helps identify the source(s) of excitation. No. 348, “Multiple Regions of Shock-accelerated Particles during a Solar Coronal Mass Ejection,” by D. Morosan: LOFAR identifies herringbone sources within the flank of the SOL2017-09-10 shock - no joke. 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 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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MMScience April 2019