No. 372: “Heating of the Solar Photosphere during a White-Light Flare”, by Jan Jurčak: the best-ever spectrum of the flaring photosphere.
No. 373: "SOL2017-09-04 (M5.5) 2017 as a Source of Relativistic Electrons and Protons,” by Alexei Struminsky: Flare-accelerated particles, rather than SEPs, energize sustained gamma-ray emission.
No. 374: "Using overlappogram data to find hot flare plasma,” by Louise Harra: imaging Fe XXIV at high resolution with the EIS slot data
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets for these and others. Comments about specific flares can be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
25 March 2020
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
Counter-streaming strahls and heat flux dropouts as possible signatures
of local particle acceleration in the solar wind
-- O. Khabarova, V. Zharkova, Q. Xia, and O. E. Malandraki
New Star Observations with NuSTAR: Flares from Young Stellar Objects
in the rho Ophiuchi Cloud Complex in Hard X-Rays
-- Juliana T. Vievering, Lindsay Glesener, Brian W. Grefenstette, and
David M. Smith
Accelerated Electrons Observed Down to <7 keV in a NuSTAR Solar Microflare
-- Lindsay Glesener, Sam Krucker, Jessie Duncan, Iain G. Hannah,
Brian W. Grefenstette, Bin Chen, David M. Smith, Stephen M. White, and
Hugh Hudson
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
18 March 2020
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
Magnetic helicity dissipation and production in an ideal MHD code
-- Axel Brandenburg, Evan Scannapieco
Magnetic twist profile inside magnetic clouds derived with a superposed
epoch analysis
-- Lanabere V., Dasso S., Demoulin P., Janvier M., Rodriguez L. and
Masias-Meza J.J.
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 keiji.yoshimura at montana.edu
Spectral Structures of Type II Solar Radio Bursts and Solar Energetic
Particles
by K. Iwai
http://cesra.net/?p=2514
The multi-thermal chromosphere: inversions of ALMA and IRIS data
by J. M. da Silva Santos et al.
http://cesra.net/?p=2484
Evolution of Coronal and Interplanetary Shock Waves Inferred from a
Radio Burst
by Khaled Alielden
http://cesra.net/?p=2474
--
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are short
communications written in language accessible to a non-expert in the
specific area and designed to keep solar and heliophysics communities
informed and up-to-date about current research. The highlights can be
followed, discussed, commented and shared via
http://www.facebook.com/solarcesra/ and http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
11 March 2020
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
Properties of ICME-Induced Forbush decreases at Earth and Mars
-- Freiherr von Forstner, J.L., Guo, J., Wimmer-Schweingruber, R.F., Dumbovic,
M., Janvier, M., Demoulin, P., Veronig, A., Temmer, M., Papaioannou, A.,
Dasso, S., Hassler, D.M., Zeitlin, C.J.,
Can Sub-Photospheric Magnetic Reconnection Change the Elemental Composition
in the Solar Corona?
-- Baker, D., van Driel-Gesztelyi, L., Brooks, D. H., Demoulin, P., Valori, G.,
Long, D.M., Laming, J.M., To, S.H., James, A.W.
White-light Emission and Chromospheric Response by an X1.8-class Flare
on 2012 October 23
-- Kyoko Watanabe and Shinsuke Imada
Helicity and winding fluxes as indicators of twisted flux emergence
-- MacTaggart, D., Prior, C.
Magnetic connectivity between the light bridge and penumbra in a sunspot
-- Song Feng, Yuhu Miao, Ding Yuan, Zhongquan Qu, Valery M. Nakariakov
Response of SDO/HMI observables to heating of the solar atmosphere
by precipitating high-energy electrons
-- Viacheslav M Sadykov, Alexander G Kosovichev, Irina N Kitiashvili,
Graham S Kerr
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
4 March 2020
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
3He-Rich Solar Energetic Particles: Solar Sources
-- Bucik, R.
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
26 February 2020
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
Statistical Study of Hard X-Ray Emitting Electrons Associated
with Flare-related Coronal Jets
-- Sophie Musset, Mariana Jeunon, Lindsay Glesener
Rapid Evolution of Type II Spicules Observed in Goode Solar Telescope
On-Disk H-alpha Images
-- V. Yurchyshyn, W. Cao, V. Abramenko, X. Yang, K.-S. Cho
Diagnostics of plasma ionisation using torsional Alfven waves
-- Istvan Ballai
Nonequilibrium ionization and ambipolar diffusion in solar magnetic flux
emergence processes
-- D. Nobrega-Siverio, F. Moreno-Insertis, J. Martinez-Sykora, M. Carlsson,
M. Szydlarski
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 keiji.yoshimura at montana.edu
The Solar Dynamics Observatory (SDO) invites you to the SDO 2020 Science Workshop: A Decade of Discovery, to be held October 12-16, 2020, at the Hyatt Regency in Vancouver, BC, Canada. All members of the science community are welcome and encouraged to attend.
The ten years since the launch of SDO has seen many papers in wide ranges of science results from this mission. As Solar Cycle 25 begins its rise to maximum, we will get together to discuss what we learned about the Sun and anticipate what the new cycle will look like.
The invited speakers who will introduce themed sessions spanning SDO‘s wide range of research topics are:
Junwei Zhao: Subsurface Flows, the Dynamo, and the Solar Cycle
Stan Solomon: Phun with Photons: Response of atmospheres to EUV variability
Paulo Simoes: Short-term Solar Variability
Aimee Norton: Magnetic Flux in the SDO Era: From Emergence to Eruption
KD Leka: SDO for Space Weather: Science and Applications
Dan Seaton: The SDO Corona and Beyond
Patrick Antolin: Energy and Mass Transfer Between the Corona and the Chromosphere
Xudong Sun: Vector Magnetic Field: Progress and Prospects
There will also be one day of parallel mini-workshops and an EUV calibration workshop.
Registration, abstract submission, and other information about SDO 2020 will be made available at http://sdo2020.lws-sdo-workshops.org/.
The Hyatt Regency can be explored at https://www.hyatt.com/en-US/hotel/canada/hyatt-regency-vancouver/yvrrv
We are assessing the need for childcare during this workshop. Please send your care requirements to William.D.Pesnell (at) NASA.gov.
Ryan Milligan
On behalf of the SDO 2020 Science Organizing Committee
===============================
STFC Ernest Rutherford Fellow
Astrophysics Research Centre
School of Mathematics and Physics
Queen’s University Belfast
E-mail: r.milligan(a)qub.ac.uk
Tel: +44 (0)2890 973465
Skype: ryanmilligan
Twitter: @ryanomilligan
Instagram: @ryanomilligan
ORCID: orcid.org/0000-0001-5031-1892
===============================
No. 370: "The Temporal and Spatial Extension of Gamma-ray Emission from the Sun”, by Nat Gopalswamy. Sustained solar γ-rays and solar cosmic rays coincide.
No. 371: "Hot Cusp-Shaped Confined Solar Flare,” by Aaron Hernandez-Perez. A major flare may have a prominent hot cusp without the help of any eruption.
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets for these and others. Comments about specific flares can be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
19 February 2020
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
Electron Beams Cannot Directly Produce Coronal Rain
-- Jeffrey W. Reep, Patrick Antolin, Stephen J. Bradshaw
Magnetic Structure of an Erupting Filament
-- Wang, S., Jenkins, J.M., Martinez Pillet, V., Beck,C., Long, D.M.,
Prasad Choudhary, D., Muglach, K., McAteer, R.T.J.
The Distribution of Time Delays Between Nanoflares
in Magnetohydrodynamic Simulations
-- Kalman J. Knizhnik & Jeffrey W. Reep
Data-driven MHD Simulation of the Formation and Initiation
of a Large-scale Pre-flare Magnetic Flux Rope in Solar Active Region 12371
-- Wen He, Chaowei Jiang, Peng Zou, Aiying Duan, Xueshang Feng, Pingbing Zuo,
Yi Wang
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 keiji.yoshimura at montana.edu