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Last Call for Abstracts for AOGS Session ST27 New Insights Into The Physics Of White-light Flares
by Juan Carlos Martínez Oliveros 29 Feb '16

29 Feb '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 was extended to 4 March 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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Last 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 29 Feb '16

29 Feb '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 was extended to 4 March 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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New UKSP Nugget #65
by Iain Hannah 26 Feb '16

26 Feb '16

65. EUV irradiances across a solar cycle by Giulio Del Zanna (Cambridge) SOHO’s CDS spectrometer can be used to study the Sun’s impact on the Earth. http://www.uksolphys.org/?p=11189 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 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 24 Feb '16

24 Feb '16

MAX MILLENNIUM NEWS 24 February 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 Oscillation of newly formed loops after magnetic reconnection in the solar chromosphere -- Shuhong Yang, Yongyuan Xiang Resolving the Fan-Spine Reconnection Geometry of a Small-Scale Chromospheric Jet Event with the New Solar Telescope -- Zhicheng Zeng, Bin Chen, Haisheng Ji, Philip R. Goode, Wenda Cao Impulsivity Parameter for Solar Flares -- W. G. Fajardo-Mendieta (1 and 2), J. C. Martinez-Oliveros (3), J. D. Alvarado-Gomez (4 and 5), B. Calvo-Mozo (1) ((1) Observatorio Astronomico Nacional, Universidad Nacional de Colombia, Bogota, Colombia, (2) Departamento de Fisica, Universidad Nacional de Colombia (3) Space Sciences Laboratory, UC Berkeley (4) European Southern Observatory (5) Universitats-Sternwarte Munchen, Ludwig-Maximilians-Universitat) Structure and Stability of Magnetic Fields in Solar Active Region 12192 Based on Nonlinear Force-Free Field Modeling -- S. Inoue, K. Hayashi, & K. Kusano Long-lived energetic particle source regions on the Sun -- Bucik, R.; Innes, D. E.; Chen, N. H.; Mason, G. M.; Gomez-Herrero, R.; Wiedenbeck, M. E. Multi-spacecraft Observations of Recurrent 3He-rich Solar Energetic Particles -- Bucik, R.; Innes, D. E.; Mall, U.; Korth, A.; Mason, G. M.; Gomez-Herrero, R. Observations of EUV Waves in 3He-rich Solar Energetic Particle Events -- Bucik, R.; Innes, D. E.; Guo, L.; Mason, G. M.; Wiedenbeck, M. E. 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's upcoming fifth anneal
by Shih, Albert Y. (GSFC-6710) 22 Feb '16

22 Feb '16

To RHESSI collaborators: RHESSI has been successfully operating in space for over 14 years now, and it is once again time to rejuvenate the detectors through an "anneal" procedure. RHESSI's germanium detectors will be heated up from their operating temperature of ~130 K to ~70 deg C (~343 K), held at that temperature for ten days, and then cooled back down. The detectors degrade steadily over time due to radiation damage from charged particles, and heating up the germanium restores lost sensitivity and resolution. These detectors have been previously annealed four times, most recently in 2014. We plan to start the anneal on February 23 (UT), and the entire procedure is estimated to take about two months. During this time period, RHESSI will be unable to make X-ray or gamma-ray observations. If you have any questions about this anneal, please feel free to contact me. Albert Shih RHESSI Deputy Mission Scientist ————— Albert Y. Shih Solar Physics Laboratory, Code 671 NASA Goddard Space Flight Center Greenbelt, MD 20771 Office: 301-286-1843

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Max Millennium News
by canfield＠mithra.physics.montana.edu 17 Feb '16

17 Feb '16

MAX MILLENNIUM NEWS 17 February 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 Chromospheric evaporation flows and density changes deduced from Hinode/EIS during an M1.6 flare -- Gomory, P.; Veronig, A. M.; Su, Y.; Temmer, M.; Thalmann, J. K. EUV Flickering of Solar Coronal Loops: A New Diagnostic of Coronal Heating -- Tajfirouze, E.; Reale, F.; Peres, G.; Testa, P. Time-resolved Emission from Bright Hot Pixels of an Active Region Observed in the EUV Band with SDO/AIA and Multi-stranded Loop Modeling -- Tajfirouze, E.; Reale, F.; Petralia, A.; Testa, P. THE NONLINEAR EVOLUTION OF A TWIST IN A MAGNETIC SHOCKTUBE -- Thomas Williams, Youra Taroyan, Viktor Fedun 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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Announcing RHESSI Science Nugget No. 267
by Hugh Hudson 17 Feb '16

17 Feb '16

“When the Earth’s atmosphere becomes dynamic…”, by Temmer, Krauss, and Veronig: The Earth’s atmosphere reacts strongly to the occurrence of flares and CMEs. 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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Chromo AID - 3rd circular
by Hugh Hudson 15 Feb '16

15 Feb '16

This workshop, "The Sun's Chromosphere in the Era of ALMA, IRIS, and DKIST," will take place March 15-18 in Boulder, CO (USA). See http://www.nso.edu/workshops/SunAID and its links for full details. The workshop aims at exploiting new data and simulations from existing facilities in anticipation of the revolutionary capabilities of ALMA and DKIST. The program is complete and includes practical demonstrations as well as planning aids for the first ALMA solicitation for solar proposals. Some additional registrations (and poster presentations) would be welcome.

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Max Millennium News
by Keiji YOSHIMURA 10 Feb '16

10 Feb '16

MAX MILLENNIUM NEWS 10 February 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 Three-Year Global Survey of Coronal Null Points from Potential-Field-Source-Surface (PFSS) Modeling and Solar Dynamics Observatory (SDO) Observations -- M. S. Freed, D. W. Longcope, and D. E. McKenzie Analysis of Flows Inside Quiescent Prominences as Captured by Hinode/Solar Optical Telescope -- M. S. Freed, D. E. McKenzie, D. W. Longcope, and M. Wilburn Ground-based Observations of the Solar Sources of Space Weather (Invited Review) -- Astrid M. Veronig, W. Poetzi Irreversible Rapid Changes of Magnetic Field Associated with the 2012 October 23 Circular Near-limb X1.8 Flare -- Dandan Ye, Chang Liu and Haimin Wang Tracing the Chromospheric and Coronal Magnetic Field with AIA, IRIS, IBIS, and ROSA Data -- Aschwanden, M.J., Reardon, K., and Jess, D. 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 canfield＠mithra.physics.montana.edu 03 Feb '16

03 Feb '16

MAX MILLENNIUM NEWS 03 February 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 The Vertical Current Approximation Nonlinear Force-Free Field Code - Description, Performance Tests, and Measurements of Magnetic Energies Dissipated in Solar Flares -- Markus J. Aschwanden High--cadence observations of spicular-type events on the Sun -- J. Shetye, J.G. Doyle, E. Scullion, C. J. Nelson, D. Kuridze, V. Henriques, F. Woeger, T. Ray Transition-region/Coronal Signatures and Magnetic Setting of Sunspot Penumbral Jets: Hinode (SOT/FG), Hi-C, and SDO/AIA Observations -- Tiwari, Sanjiv K.; Moore, Ronald L.; Winebarger, Amy R.; Alpert, Shane E. 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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