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Max Millennium News
by canfield＠mithra.physics.montana.edu 11 Feb '15

11 Feb '15

MAX MILLENNIUM NEWS 11 February 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 Temperature and Electron Density Diagnostics of a Candle-flame-shaped Flare -- S. E. Guidoni, D. E. McKenzie, D. W. Longcope, J. E. Plowman, and K. Yoshimura Magnetic axis safety factor of finite beta spheromaks and transition from spheromaks to toroidal magnetic bubbles -- Paul M. Bellan and Roberto Paccagnella 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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IRIS-4 Workshop in May
by Dennis, Brian R. (GSFC-6710) 06 Feb '15

06 Feb '15

IRIS-4 workshop Dates: May 18-22, 2015 Location: Boulder, CO Web Site: www2.hao.ucar.edu/iris-4-workshop<HTTPS://www2.hao.ucar.edu/iris-4-workshop> Program: · Talks and posters · Tutorials on IRIS data analysis and related topics such as optically thick radiative transfer Abstract/early registration deadline: March 6 Adrian N. Daw IRIS Mission Scientist NASA/GSFC Solar Physics Lab Adrian.Daw(a)nasa.gov<mailto:Adrian.Daw@nasa.gov> office: 301-286-2278

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Max Millennium News
by canfield＠mithra.physics.montana.edu 04 Feb '15

04 Feb '15

MAX MILLENNIUM NEWS 04 February 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 KAPPA: A Package for Synthesis of optically thin spectra for the non-Maxwellian kappa-distributions based on the CHIANTI database -- Dzifcakova, E., Dudik, J., Kotrc, P., Farnik, F., Zemanova, A. SWAP Observations of Post-flare Giant Arches in the Long-Duration 14 October 2014 Solar Eruption -- Matthew J. West and Daniel B. Seaton Inverse diffraction for the Atmospheric Imaging Assembly in the Solar Dynamics Observatory -- Gabriele Torre, Richard A Schwartz, Federico Benvenuto, Anna Maria Massone, Michele Piana An explanation for the difference between physical conditions in two ribbons in the July 23, 2002 flare -- N.M. Firstova Are Halo-like Solar Coronal Mass Ejections Merely a Matter of Geometric Projection Effects? -- Ryun-Young Kwon, Jie Zhang, and Angelos Vourlidas Forecasting F10.7 with solar magnetic flux transport modeling -- C. J. Henney, W. A. Toussaint, S. M. White, and C. N. Arge FIP Bias Evolution in a Decaying Active Region -- D. Baker, D. H. Brooks, P. Demoulin, S. L. Yardley, L. van Driel-Gesztelyi, D. M. Long, L. M. Green 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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New UKSP Nugget #54
by Iain Hannah 01 Feb '15

01 Feb '15

54. Assessing the polarization ratio technique for 3D CME reconstructions by Paolo Pagano, Duncan Mackay (University of St Andrews) & Alessandro Bemporad (Turin/INAF) How well can we use METIS coronagraph observations to locate CMEs in space? http://www.uksolphys.org/?p=9265 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ UKSP Nuggets are published on a monthly basis highlighting solar physics research led from the UK. http://www.uksolphys.org/uksp-nuggets Iain Hannah and Lyndsay Fletcher ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Dr. Iain G. Hannah Royal Society Research Fellow, Astronomy & Astrophysics Group, SUPA School of Physics & Astronomy, Kelvin Building, University of Glasgow, Glasgow, UK, G12 8QQ Web: http://www.astro.gla.ac.uk/~iain/ Eml: iain.hannah(a)glasgow.ac.uk<mailto:iain.hannah@glasgow.ac.uk> Tel: +44 (0)141 330 6427 Fax: +44 (0)141 330 5183 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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

28 Jan '15

MAX MILLENNIUM NEWS 28 January 2015 CONTENTS 1. CHANGES IN THE MAX MILLENNIUM CHIEF OBSERVER TEAM 2. E-PRINTS POSTED IN THE PAST WEEK 3. FROM THE EDITOR ===================================================================== 1. CHANGES IN THE MAX MILLENNIUM CHIEF OBSERVER TEAM ---------------------------------------------------- > From Dick Canfield <canfield at physics.montana.edu> The volunteer team of scientists who collectively serve as the Max Millennium Chief Observer keep abreast of solar activity on a daily basis. They work together to select the most appropriate observing targets and observing plans, using their expertise at solar activity forecasting. They send out their recommendations to several hundred solar scientists via the Max Millennium Message of the Day e-mail list. Paul Higgins (Trinity College Dublin / LMSAL) has been a valuable member of the Max Millennium Chief Observer team for the last two years. Paul joined the team in March 2013, building on his PhD studies of the relationship between dynamic sunspot group properties and the occurrence of flares. He sent out his last Message of the Day on January 11th. We will miss his knowledgeable and proactive approach to flare forecasting. Many thanks, Paul, for a job well done. Ying Li (Nanjing University / Montana State University) will join the MM_CO team in March. She finished her PhD Thesis "Observations and Modeling of Solar Flare Atmospheric Dynamics" in 2013. Her research interests include heating and dynamics in solar flares: EUV & UV spectroscopy, multi-wavelength data analysis, and theoretical modeling. Welcome, Ying! 2. E-PRINTS POSTED IN THE PAST WEEK ----------------------------------- > http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl Wave heating of the solar atmosphere -- I. Arregui Perturbations of gyrosynchrotron emission polarization from solar flares by sausage modes: forward modelling -- Reznikova V.E., Van Doorsselaere T., and Kuznetsov A.A. Relative drifts and temperature anisotropies of protons and $ α particles in the expanding solar wind -- 2.5D hybrid simulations -- Maneva, Y., Ofman, L., Vinas, A.-F. Constraining hot plasma in a non-flaring solar active region with FOXSI hard X-ray observations -- Ishikawa, Shin-nosuke; Glesener, Lindsay; Christe, Steven; Ishibashi, Kazunori; Brooks, David H.; Williams, David R.; Shimojo, Masumi; Sako, Nobuharu; Krucker, S First Images from the Focusing Optics X-Ray Solar Imager -- Krucker, Sam; Christe, Steven; Glesener, Lindsay; Ishikawa, Shin-nosuke; Ramsey, Brian; Takahashi, Tadayuki; Watanabe, Shin; Saito, Shinya; Gubarev, Mikhail; Kilaru, Kiranmayee; Tajima, Hiroyasu; Tanaka, Takaaki; Turin, Paul; McBride, Stephen; Glaser, David; Fermin, Jose; White, Stephen; Lin, Robert Prominence seismology using the period ratio of transverse thread oscillations -- R. Soler, M. Goossens, J. L. Ballester 3. 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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Announcing RHESSI Science Nugget No. 245
by Hugh Hudson 26 Jan '15

26 Jan '15

"Flare Heating by Mildly Non-thermal Particles," by Jeffrey Reep. Sorting out nonthermal distributions via HYDRAD simulations. 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 21 Jan '15

21 Jan '15

MAX MILLENNIUM NEWS 21 January 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 Key Aspects of Coronal Heating -- James A. Klimchuk 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 14 Jan '15

14 Jan '15

MAX MILLENNIUM NEWS 14 January 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 Ion Heating in Inhomogeneous Expanding Solar Wind Plasma: The Role of Parallel and Oblique Ion-Cyclotron Waves -- Ozak, N.; Ofman, L.; Vilas, A.-F. Three-dimensional multi-fluid model of a coronal streamer belt with a tilted magnetic dipole -- L. Ofman, E. Provornikova, L. Abbo, and S. Giordano Solar Magnetic Flux Ropes i -- Boris Filippov, Olesya Martsenyuk, Abhishek K. Srivastava, and Wahab Uddin Extreme Ultra-Violet Spectroscopy of the Flaring Solar Chromosphere -- Ryan O. Milligan Soft X-ray emission in kink-unstable coronal loops -- R. F. Pinto, N. Vilmer, A. S. Brun The energetics of a global shock wave in the low solar corona -- David M. Long, Deborah Baker, David R. Williams, Eoin P. Carley, Peter T. Gallagher, Pietro Zucca Prominence Activation by Coronal Fast Mode Shock -- Takuya Takahashi, Ayumi Asai, Kazunari Shibata 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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Announcing RHESSI Science Nugget No. 244
by Hugh Hudson 12 Jan '15

12 Jan '15

"Above-the-Looptop Sources," by Mitsuo Oka and Sa"m Krucker. Electron distribution functions in coronal sources explained. 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 07 Jan '15

07 Jan '15

MAX MILLENNIUM NEWS 07 January 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 New analytical and numerical models of solar coronal loop: I. Application to forced vertical kink oscillations -- Murawski, K.; Solov'ev, A.; Kraskiewicz, J.; Srivastava, A. K. Torsional Alfven Waves in Solar Magnetic Flux Tubes of Axial Symmetry -- Murawski, K.; Solov'ev, A.; Musielak, Z. E.; Srivastava, A. K.; Kraskiewicz, J. Structure and Evolution of Magnetic Fields Associated with Solar Eruptions -- Haimin Wang and Chang Liu 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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