MMScience April 2012

mmscience@solar.physics.montana.edu

7 participants
11 discussions

New EIS nugget
by Lucie Green 29 Nov '12

29 Nov '12

Dear all, We are pleased to announce the release of a new EIS nugget. This month we celebrate one year of the EIS flare catalogue and the dataset that EIS is collecting. Please visit the nugget here: http://msslxr.mssl.ucl.ac.uk:8080/SolarB/nuggets/nugget_2012feb.jsp We welcome nugget contributions from the community. Please contact Lucie Green if you are interested. Dr Lucie Green Mullard Space Science Laboratory Holmbury St. Mary Dorking Surrey RH5 6NT +44 (0)1483 204103 www.mssl.ucl.ac.uk/~lmg

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Announcing a new RHESSI Science Nugget
by Hugh S. Hudson 30 Apr '12

30 Apr '12

No. 174, A Shocking Type II, by Hazel Bain, Sa"m Krucker, and Lindsay Glesener: Global coronal waves getting sorted out. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/A_Shocking_Type_II . Older Nuggets are available at http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets (the current series, 2008-present), and at http://sprg.ssl.berkeley.edu/~tohban/nuggets/ (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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A new UKSP nugget - 22. A huge solar tornado observed by SDO/AIA
by Iain Hannah 29 Apr '12

29 Apr '12

22. A huge solar tornado observed by Solar Dynamic Observatory by Xing Li, Huw Morgan, Drew Leonard and Lauren Jeska, Aberystwyth University A solar twister appears as mass and magnetic flux are injected into the corona http://www.uksolphys.org/?p=4457 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ UKSP Nuggets are published on a monthly basis highlighting solar physics research in the UK. http://www.uksolphys.org/uksp-nuggets Iain Hannah and Lyndsay Fletcher -- ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Dr. Iain G. Hannah Eml: iain.hannah(a)glasgow.ac.uk Astronomy & Astrophysics Group, Tel: +44 (0)141 330 6427 School of Physics & Astronomy, Fax: +44 (0)141 330 5183 Kelvin Building, University of Glasgow, Glasgow, Scotland, UK G12 8QQ Web: http://www.astro.gla.ac.uk/~iain/ ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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New GSFC RHESSI web site
by Kim Tolbert 27 Apr '12

27 Apr '12

I apologize if you get this message twice. It was suggested that I send it to a wider list. The RHESSI team at GSFC is pleased to announce a new RHESSI web site at http://hesperia.gsfc.nasa.gov/rhessi that is compliant with NASA web site standards. Please check it out. Feedback is welcome - send comments tokim.tolbert(a)nasa.gov. The two old RHESSI web sites will not be maintained, but can still be accessed via: http://hesperia.gsfc.nasa.gov/old_hessi - The old RHESSI Home Page http://hesperia.gsfc.nasa.gov/old_rhessidatacenter - The old RHESSI Data& Software Center page Bookmarks to the old top-level pages will direct you to the new site, but bookmarks to lower-level pages will continue to go to the old site. Please modify your bookmarks to use the new site. Kim Tolbert GSFC

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Max Millennium News
by canfield＠mithra.physics.montana.edu 25 Apr '12

25 Apr '12

MAX MILLENNIUM NEWS 25 April 2012 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 Quasi-periodic Fast-mode Wave Trains Within a Global EUV Wave and Sequential Transverse Oscillations Detected by SDO/AIA -- Wei Liu, Leon Ofman, Nariaki V. Nitta, Markus J. Aschwanden, Carolus J. Schrijver, Alan M. Title, and Theodore D. Tarbell Observations of quasi-periodic phenomena associated with a large blowout solar jet -- R. J. Morton, A. K. Srivastava, R. Erd'elyi Coronal Mass Ejection Mass, Energy, and Force Estimates Using STEREO -- Eoin P. Carley, R.T. James McAteer, Peter T. Gallagher Thermal Evolution and Radiative Output of Solar Flares Observed by the EUV Variability Experiment (EVE) -- Chamberlin, P. C., R. O. Milligan, and T. N. Woods Particle dynamics in the reconnecting heliospheric current sheet: solar wind data versus 3D PIC simulations -- Zharkova V.V. and Khabarova O.V. Using a New Sky Brightness Monitor to Observe the Annular Solar Eclipse on 15 January 2010 -- Y. Liu, Y.-D. Shen, X.-F. Zhang, N.-P. Liu Solar origin of in-situ near-relativistic electron spikes observed with SEPT/STEREO -- A. Klassen, R. Gomez-Herrero, B. Heber, Y. Kartavykh, W. Droge, K.-L. Klein 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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New EIS Nugget
by Deborah Baker 24 Apr '12

24 Apr '12

UCL-MSSL is pleased to announce a new Hinode EIS science nugget for April 2012 entitled: How line widths depend on temperature as well as location by David Williams (UCL - MSSL). April 2012 Nugget: http://msslxr.mssl.ucl.ac.uk:8080/SolarB/nuggets/nugget_2012apr.jsp Nugget Archive: http://msslxr.mssl.ucl.ac.uk:8080/SolarB/eisnuggets.jsp EIS nuggets are published monthly. If you would like to contribute a nugget, please contact Deb Baker or Lucie Green. Dr Deb Baker UCL/MSSL

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Max Millennium News
by canfield＠mithra.physics.montana.edu 18 Apr '12

18 Apr '12

MAX MILLENNIUM NEWS 18 April 2012 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 Expansion of magnetic clouds in the outer heliosphere -- A.M. Gulisano, P. Demoulin, S. Dasso, L. Rodriguez Observation and Simulation of Longitudinal Oscillations of an Active Region Prominence -- Qingmin Zhang, Pengfei Chen, Chun Xia, Rony Keppens Radio pulsating structures with coronal loop contraction -- J. Kallunki, S. Pohjolainen THE n-DISTRIBUTION OF ELECTRONS AND DOUBLE LAYERS IN THE ELECTRON BEAM--RETURN SYSTEM OF SOLAR FLARES -- Marian Karlicky Establishing a Connection Between Active Region Outflows and the Solar Wind: Abundance Measurements with EIS/Hinode -- Brooks, David H., Warren, Harry P. Behavior of Solar Cycles 23 and 24 Revealed by Microwave Observations -- N. Gopalswamy, S.Yashiro, P. Makela, G. Michalek, K. Shibasaki, and D. Hathaway 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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CHIANTI: a new Google Group for discussion of CHIANTI issues
by Peter Young 16 Apr '12

16 Apr '12

Dear colleagues, This message is to inform you that the CHIANTI team have set up a Google Group for discussion of CHIANTI issues. The aim is to provide a forum where CHIANTI users can post questions or comments about CHIANTI, and also where the CHIANTI team can post information about changes to the database and solicit opinions. We feel that the group will provide a valuable new way for CHIANTI users to communicate with the team and with each other. Note that the existing chianti_help e-mail address will remain operational. For those of you with Google accounts, you can monitor the group discussion through your account (look for the 'Groups' section on the Google front page). If you don't have a Google account then you can send and receive messages through your mail tool in a similar fashion to a mailing list. The e-mail address for the group is chianti(a)googlegroups.com. A following message will come from Peter Young giving an invitation to all current members of the CHIANTI mailing list. In this e-mail you will see a button that says "Accept This Invitation". Click on the button to add your e-mail address to the group. If you have colleagues who would be interested in joining the CHIANTI Google Group, please have them contact Peter Young (pyoung9(a)gmu.edu) who will then send out invitations. Regards, Peter Young on behalf of the CHIANTI team

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Announcing a new RHESSI Science Nugget, No. 173
by Hugh S. Hudson 16 Apr '12

16 Apr '12

No. 173, RHESSI and IRIS, by Hugh Hudson: flare gold at the foot of the rainbow. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_and_IRIS. Older Nuggets are available at http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets (the current series, 2008-present), and at http://sprg.ssl.berkeley.edu/~tohban/nuggets/ (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 Keiji YOSHIMURA 11 Apr '12

11 Apr '12

MAX MILLENNIUM NEWS 11 April 2012 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 4pi Models of CMEs and ICMEs -- Kleimann, J. Observations of Multiple Surges Associated with Magnetic Activities in AR10484 on 25 October 2003 -- Wahab Uddin, B. Schmieder, R. Chandra, Abhishek K. Srivastava, Pankaj Kumar, S. Bisht Growing transverse oscillations of a multistranded loop observed by SDO/AIA -- Tongjiang Wang, Leon Ofman, Joseph M. Davila, Yang Su Flows at the Edge of an Active Region: Observation and Interpretation -- C. Boutry, E. Buchlin, J.-C. Vial, S. Regnier Numerical simulations of chromospheric hard X-ray source sizes in solar flares -- M. Battaglia, E. P. Kontar, L. Fletcher, A. L. MacKinnon Observation of Ultrafine Channels of Solar Corona Heating -- Haisheng Ji, Wenda Cao, Philip R. Goode 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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MMScience April 2012