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Max Millennium News
by canfield＠mithra.physics.montana.edu 28 Oct '15

28 Oct '15

MAX MILLENNIUM NEWS 28 October 2015 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 Kinetic model of force-free current sheets with non-uniform temperature -- D. Y. Kolotkov, I. Y. Vasko, and V. M. Nakariakov Dynamics of coronal rain and descending plasma blobs in solar prominences: II. Partially ionized case -- Oliver, R., Soler, R., Terradas, J., Zaqarashvili, T. V. CORONAL RAIN IN MAGNETIC ARCADES: REBOUND SHOCKS, LIMIT CYCLES, AND SHEAR FLOWS -- X. Fang, C. Xia, R. Keppens, and T. Van Doorsselaere Modeling of Reflective Propagating Slow-mode Wave in a Flaring Loop -- X. Fang, D. Yuan, T. Van Doorsselaere, R. Keppens, and C. Xia Fast magnetoacoustic wave trains of sausage symmetry in cylindrical waveguides of the solar corona -- S. Shestov, V. M. Nakariakov, S. Kuzin Dynamo in the outer heliosheath: Necessary conditions -- E.S. Belenkaya The Relation between Solar Eruption Topologies and Observed Flare Features II: Dynamical Evolution -- A. Savcheva, E. Pariat, S. McKillop, P. McCauley, E. Hanson, Y. Su, & E. DeLuca 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 canfield at physics.montana.edu

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Max Millennium News
by canfield＠mithra.physics.montana.edu 21 Oct '15

21 Oct '15

MAX MILLENNIUM NEWS 21 October 2015 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 How important are electron beams in driving chromospheric evaporation in the 2014 March 29 flare? -- Marina Battaglia, Lucia Kleint, Sam Krucker, David Graham Evolution of solar active regions: Detecting the emergence of new magnetic field through multifractal segmentation -- A. A. Golovko and I. I. Salakhutdinova Filament Shape and Coronal Magnetic Field Structure -- B. Filippov SOLAR RADIUS VARIATIONS: AN INQUISITIVE WAVELENGTH DEPENDENCE -- Rozelot, J.P., Kosovichev, A., Kilcik, A 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 canfield at physics.montana.edu

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NoRH Science Nuggets
by Kiyoto Shibasaki 17 Oct '15

17 Oct '15

NoRH Science Nuggets The International Consortium for the Continued Operation of Nobeyama Radioheliograph (ICCON, http://hinode.stelab.nagoya-u.ac.jp/ICCON/) is pleased to announce the start of a series of Nobeyama Radioheliograph (NoRH) Science Nuggets.We welcome submission of papers using NoRH data and more broadly papers on solar radio astronomy, solar physics, and related fields.We wish to keep the spirit of Nuggets, “a solid lump; especially: a native lump of precious metal (http://www.merriam-webster.com/dictionary/nugget)” and the nugget papers need to be short and succinct.Please send them in the form of .pdf to the editors, shibasaki.kiyoto@CCNW and masuda@STEL (CCNW: md.ccnw.ne.jp, STEL: stelab.nagoya-u.ac.jp). Kiyoto Shibasaki, Dr. Solar Physics Research Inc. Matsushin 2-24 Kasugai, 486-0931, Japan Satoshi Masuda, Dr. Institute for Space-Earth Environmental Research (former Solar Terrestrial Environment Laboratory) Nagoya University Furo-cho, Chikusa-ku Nagoya, 464-8601, Japan -- ----------------------------------- Kiyoto Shibasaki Solar Physics Research Inc. shibasaki.kiyoto(a)md.ccnet.ne.jp -----------------------------------

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Max Millennium News
by canfield＠mithra.physics.montana.edu 15 Oct '15

15 Oct '15

MAX MILLENNIUM NEWS 15 October 2015 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 Thermosphere and geomagnetic response to interplanetary coronal mass ejections observed by ACE and GRACE: Statistical results -- S. Krauss, M. Temmer, A.M. Veronig, O. Baur, H. Lammer Electric current filamentation at a non-potential magnetic null-point due to pressure perturbation -- P. Jelinek, M. Karlicky, K. Murawski Evidence of thermal conduction suppression in hot coronal loops: Supplementary results -- Tongjiang Wang, Leon Ofman, Xudong Sun, Elena Provornikova, Joseph M. Davila IRIS Si IV line profiles: An indication for the plasmoid instability during small-scale magnetic reconnection on the Sun -- Davina Innes, LiJia Guo, YiMin Huang, Amitava Bhattacharjee 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 canfield at physics.montana.edu

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Max Millennium News
by canfield＠mithra.physics.montana.edu 07 Oct '15

07 Oct '15

MAX MILLENNIUM NEWS 07 October 2015 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 Thresholded Power Law Size Distributions of Instabilities in Astrophysics -- Markus J. Aschwanden 2D MHD and 1D HD models of a solar flare - a comprehensive comparison of the results -- R. Falewicz, P. Rudawy, K. Murawski, A. K. Srivastava Large-scale Globally Propagating Coronal Waves -- Alexander Warmuth The appearance, motion, and disappearance of three-dimensional magnetic null points -- Nicholas A. Murphy, Clare E. Parnell, and Andrew L. Haynes 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 canfield at physics.montana.edu

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Max Millennium News
by canfield＠mithra.physics.montana.edu 30 Sep '15

30 Sep '15

MAX MILLENNIUM NEWS 30 September 2015 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 Spectroscopic observations and modelling of impulsive Alfven waves along a polar coronal jet -- P. Jelinek, A. K. Srivastava, K. Murawski, P. Kayshap and B. N. Dwivedi A Circular-ribbon Solar Flare Following an Asymmetric Filament Eruption -- Chang Liu, Na Deng, Rui Liu, Jeongwoo Lee, Etienne Pariat, Thomas Wiegelmann, Yang Liu, Lucia Kleint, Haimin Wang Investigation of Umbral Dots with the New Vacuum Solar Telescope -- Kaifan Ji, Xia Jiang, Song Feng, Yunfei Yang, Hui Deng, Feng Wang Cut-off period for slow magnetoacoustic waves in coronal plasma structures -- A.N. Afanasyev, V. M. Nakariakov Flare processes evolution and polarization changes of fine structures of solar radio emission in the April 11, 2013 event -- Gennady Chernov, Robert Sych, Baolin Tan, Yihua Yan, Chengming Tan, Qijun Fu, Marian Karlicky and Valery Fomichev Model of Local Oscillations in Sunspots -- Yu. D. Zhugzhda and R.A.Sych Sunspot waves and flare energy release -- R. Sych, M. Karlicky, A. Altyntsev, J. Dudik and L. Kashapova MHD waves in sunspots -- Robert Sych Magnetic Reconnection Rates and Energy Release in a Confined X-class Flare -- Astrid M. Veronig, Wolfgang Polanec Flare processes evolution and polarization changes of fine structures of solar radio emission in the April 11, 2013 event -- Gennady Chernov, Robert Sych, Baolin Tan, Yihua Yan, Chengming Tan, Qijun Fu, Marian Karlicky and Valery Fomichev 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 canfield at physics.montana.edu

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Max Millennium News
by canfield＠mithra.physics.montana.edu 23 Sep '15

23 Sep '15

MAX MILLENNIUM NEWS 23 September 2015 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 Benchmark Test of Differential Emission Measure Codes and Multi-Thermal Energies in Solar Active Regions -- Aschwanden,M.J., Boerner,P., Caspi,A., McTiernan,J.M., Ryan,D., and Warren,H.P. Multiwavelength Observations of a Slow Raise, Multi-Step X1.6 Flare and the Associated Eruption -- Yurchyshyn, V., Kumar, P., Cho, K.S., Lim, E.K., & Abramenko, V. Active region upflows: 1. Multi-instrument observations -- K. Vanninathan, M.S. Madjarska, K. Galsgaard, Z.Huang, J.G. Doyle Active region upflows: 2. Data driven MHD modeling -- K. Galsgaard, M. S. Madjarska, K. Vanninathan, Z. Huang, M. Presmann A Statistical Study of Distant Consequences of Large Solar Energetic Events -- C.J. Schrijver, P.A. Higgins Coronal response to an EUV wave from DEM analysis -- K. Vanninathan, A.M. Veronig, K. Dissauer, M.S. Madjarska, I.G. Hannah, E.P. Kontar 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 canfield at physics.montana.edu

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RHESSI Science Nuggets in September
by Hugh Hudson 21 Sep '15

21 Sep '15

No. 262, "Fine Structure in Flare Soft X-ray Light Curves," by Brian Dennis and Kim Tolbert: A tool that we’ve had since 1976 now gives us surprisingly precise new information. No. 261, "Photospheric Electric Fields and Energy Fluxes in the Eruptive Active Region NOAA 11158,” by Maria Kazachenko. Flares need magnetic energy; we can now measure its arrival as Poynting flux across the solar photosphere. No. 260, “RHESSI and General Relativity,” by Bill Thompson and Hugh Hudson. General-relativistic corrections to RHESSI source positions. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets listing the current series, 2008-present, and http://sprg.ssl.berkeley.edu/~tohban/nuggets/ for the original series, 2005-2008. We publish these at roughly two-week intervals and welcome contributions, which should be related, at least loosely, to RHESSI science.

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Max Millennium News
by canfield＠mithra.physics.montana.edu 16 Sep '15

16 Sep '15

MAX MILLENNIUM NEWS 16 September 2015 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 apparent mass of a coronal mass ejection increase? -- Feng, Li; Wang, Yuming; Shen, Fang; Shen, Chenglong; Inhester, Bernd; Lu, Lei; Gan, Weiqun Radial Flow Pattern of a Slow Coronal Mass Ejection -- Feng, Li; Inhester, Bernd; Gan, Weiqun Heating and cooling of coronal loops observed by SDO -- Li, L. P., Peter, H., Chen, F., and Zhang, J. APPEARANCES AND STATISTICS OF CORONAL CAVITIES DURING THE ASCENDING PHASE OF SOLAR CYCLE 24 -- N. Karna, W. D. Pesnell, and J. Zhang STUDY OF THE 3D GEOMETRIC STRUCTURE AND TEMPERATURE OF A CORONAL CAVITY USING THE LIMB SYNOPTIC MAP METHOD -- N. Karna, J. Zhang, W. Dean Pesnell, and S. A. Hess Webber Application of Kernel Based Machine Learning to Inversion Problem of Photospheric Magnetic Fields -- Fei Teng Hard X-Ray Imaging of Individual Spectral Components in Solar Flares -- Amir Caspi, Albert Y. Shih, James M. McTiernan, Sam Krucker 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 canfield at physics.montana.edu

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Max Millennium News
by canfield＠mithra.physics.montana.edu 09 Sep '15

09 Sep '15

MAX MILLENNIUM NEWS 09 September 2015 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 Model comparison for the density structure across solar coronal waveguides -- I. Arregui, R. Soler, A. Asensio Ramos Evidence of thermal conduction suppression in a solar flaring loop by coronal seismology of slow-mode waves -- Tongjiang Wang, Leon Ofman, Xudong Sun, Elena Provornikova, Joseph M. Davila The Role of Erupting Sigmoid in Triggering a Flare with Parallel and Large-Scale Quasi-Circular Ribbons -- Navin Chandra Joshi, Chang Liu, Xudong Sun, Haimin Wang, Tetsuya Magara, Y.-J. Moon Damped transverse oscillations of interacting coronal loops -- Roberto Soler and Manuel Luna 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 canfield at physics.montana.edu

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