MMScience January 2016

mmscience@solar.physics.montana.edu

4 participants
9 discussions

Second Call for Abstracts for AOGS Session ST27 New Insights Into The Physics Of White-light Flares
by Juan Carlos Martínez Oliveros 27 Jan '16

27 Jan '16

Dear All, We invite contributions to the session (ID#: ST27) “New Insights Into The Physics Of White-light Flares” at the AOGS meeting in Beijing, 31 Jul to 5 Aug, 2016. Details on the session follow. We would like to remind you that the abstract submission deadline is 19 February 2016. Abstracts can be submitted using the following link: http://www.asiaoceania.org/aogs2016/public.asp?page=abstract.htm Best regards, Juan Carlos Martinez Oliveros Hugh S Hudson Lucia Kleint Mingde Ding --------------------------------------------- Session Title: New Insights Into The Physics Of White-light Flares Session Description: The white-light continuum of a solar flare was the first manifestation of a flare ever detected, and this continuum emission contains a large fraction of the total luminous energy of a flare. Thus its identification has always posed an important problem for solar and stellar physics. A zoo of phenomena accompanies these events and their analysis can provide a wealth of information about the solar atmosphere. The focus of the discussion is the manifestation in the visible continuum of flares, from the corona to the solar interior and how multi wavelength observations (RHESSI, IRIS, SDO, Hinode, infrared, NoRH, OVSA) can help our understanding of the mechanics of momentum and energy transfer in the solar atmosphere.

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Max Millennium News
by canfield＠mithra.physics.montana.edu 27 Jan '16

27 Jan '16

MAX MILLENNIUM NEWS 27 January 2016 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 Coronal Magnetic Fields Derived from Simultaneous Microwave and EUV Observations and Comparison with the Potential Field Model -- S. Miyawaki, K. Iwai, K. Shibasaki, D. Shiota, and S. Nozawa Ultra-narrow Negative Flare Front Observed in Helium-10830 A using the 1.6 m New Solar Telescope -- Yan Xu, Wenda Cao, Mingde Ding, Lucia Kleint, Jiangtao Su, Chang Liu, Haisheng Ji, Jongchul Chae, Ju Jing, Kyuhyoun Cho, Kyungsuk Cho, Dale Gary, and Haimin Wang The Impact of the Revised Sunspot Record on Solar Irradiance Reconstructions -- G. Kopp, N. Krivova, J. Lean, and C.J. Wu 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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15th RHESSI workshop
by Eduard Kontar 26 Jan '16

26 Jan '16

The next RHESSI Workshop (number XV in the series) will be held in Graz, Austria, from July 26-30, 2016. This workshop is now open for registration/abstract submission athttp://rhessi15.uni-graz.at/en/ <http://rhessi15.uni-graz.at/en/> This workshop will consist of a blend of plenary sessions (at the beginning and end), with topical sessions in between. Topics include integration of RHESSI and IRIS observations, analysis of RHESSI/Fermi data, the SXR and EUV response of the solar atmosphere to flare heating, joint radio/HXR studies, next steps in RHESSI imaging, and theory and modeling of flare processes. <http://rhessi15.uni-graz.at/en/>

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Max Millennium News
by canfield＠mithra.physics.montana.edu 20 Jan '16

20 Jan '16

MAX MILLENNIUM NEWS 20 January 2016 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 Observations of multiple blobs in homologous solar coronal jets in closed loops -- Q. M. Zhang, H. S. Ji, and Y. N. Su Intense bipolar structures from stratified helical dynamos -- Dhrubaditya Mitra, A. Brandenburg, N. Kleeorin, I. Rogachevskii 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 canfield＠mithra.physics.montana.edu 13 Jan '16

13 Jan '16

MAX MILLENNIUM NEWS 13 January 2016 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 Radiative transfer in cylindrical threads with incident radiation VII. Multi-thread models -- N. Labrosse and A.S. Rodger Sources of Quasi-Periodic Pulses in the 18 August 2012 Flare -- A. Altyntsev, N. Meshalkina, H. Meszarosova, M. Karlicky, V. Palshin, S. Lesovoi Alfvenic Wave Heating of the Upper Chromosphere in Flares -- Reep, J.W., & Russell, A.J.B. Thermal and non-thermal emission from reconnecting twisted coronal loops -- R. F. Pinto, M. Gordovskyy, P.K. Browning and N. Vilmer 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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New UKSP Nugget #64
by Iain Hannah 08 Jan '16

08 Jan '16

64. 3D Electron Density Distributions in the Solar Corona during Solar Minimum by Judith de Patoul and Claire Foullon (Exeter) and Pete Riley (Predictive Science) A new tomographic method promises better solar wind models http://www.uksolphys.org/?p=10950 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 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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Call for abstracts to the session ST26 Multiwavelength and In-situ Observations Of CME and Flare Evolution and Dynamics at AOGS 2016
by Juan Carlos Martínez Oliveros 07 Jan '16

07 Jan '16

Dear All, We invite contributions to the session (ID#: ST26) “Multiwavelength and In-situ Observations of CME and Flare Evolution and Dynamics” at the AOGS meeting in Beijing from July 31 to August 5, 2016. Details on the session follow. We would like to remind you that the abstract submission deadline is 19 February 2016. Abstracts can be submitted using the following link: http://www.asiaoceania.org/aogs2016/public.asp?page=abstract.htm Best regards, Juan Carlos Martinez Oliveros Ying Liu Hazel Bain David Sundkvist --------------------------------------------- Session Title: *Multiwavelength and In-situ Observations Of CME and Flare Evolution and Dynamics* Session Description: Flares and CMEs are two spectacular manifestations of the explosive release of magnetic energy in the solar atmosphere. The released magnetic energy is transformed into kinetic and thermal energy and radiations. The focus of this session is to discuss how multi-wavelength observations and in situ measurements from current (IRIS, SDO, RHESSI, Hinode, NoRH, NRH, OVSA, STEREO, Wind, ACE) and future (Solar Orbiter, Solar Probe Plus) instruments and theoretical modeling can help our understanding of the mechanics, dynamics and evolution of these phenomena in the corona and interplanetary space.

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Max Millennium News
by canfield＠mithra.physics.montana.edu 06 Jan '16

06 Jan '16

MAX MILLENNIUM NEWS 06 January 2016 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 Injection of solar energetic particles into both loop legs of a magnetic cloud -- Nina Dresing, Raul Gomez-Herrero, Bernd Heber, Miguel Angel Hidalgo, Andreas Klassen, Manuela Temmer, Astrid Veronig X-ray Source Heights in a Solar Flare: Thick-target versus Thermal Conduction Front Heating -- Reep, J.W., Bradshaw, S.J., Holman, G.D. 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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Call for Abstract for AOGS Session ST27 New Insights Into The Physics Of White-light Flares
by Juan Carlos Martínez Oliveros 04 Jan '16

04 Jan '16

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MMScience January 2016