No. 380: “Energy Transport by Accelerated Particles in the Quiet Solar Atmosphere”, by Lars Frogner, Boris Gudiksen, and Helle Bakke. A first study of non-thermal particles integrated into an MHD simulation of the solar atmosphere.
No. 381: “Extreme Ultraviolet Late Phase of Solar Flares”, by Rui LIU. Both arcade and circular-ribbon flares may sometimes spawn EUV late phase emission.
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.
No. 380: “Energy Transport by Accelerated Particles in the Quiet Solar Atmosphere”, by Lars Frogner, Boris Gudiksen, and Halle Bakke. A first study of non-thermal particles integrated into an MHD simulation of the solar atmosphere.
No. 381: “Extreme Ultraviolet Late Phase of Solar Flares”, by Rui LIU. Both arcade and circular-ribbon flares may sometimes spawn EUV late phase emission.
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
24 June 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
Numerical simulation of solar photospheric jet-like phenomena
caused by magnetic reconnection
-- Yuji Kotani, Kazunari Shibata
Solar Flare-CME Coupling Throughout Two Acceleration Phases of a Fast CME
-- Tingyu Gou, Astrid M. Veronig, Rui Liu, Bin Zhuang, Mateja Dumbovic,
Tatiana Podladchikova, Hamish A. S. Reid, Manuela Temmer, Karin Dissauer,
Bojan Vrsnak, Yuming 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
MAX MILLENNIUM NEWS
17 June 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
A new method for estimating global coronal wave properties from their
interaction with solar coronal holes
-- I. Piantschitsch, J. Terradas, M. Temmer
Machine-learning approach to identification of coronal holes in solar disk
images and synoptic maps
-- Egor Illarionov, Alexander Kosovichev, Andrey Tlatov
Multilevel Observations of the Oscillations in the First Active Region
of the New Cycle
-- Andrei Chelpanov and Nikolai Kobanov
Standing MHD Waves in a Magnetic Slab Embedded in an Asymmetric Magnetic
Plasma Environment: Surface Waves
-- William Oxley, Noemi Kinga Zsamberger, Robert Erdelyi
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
No. 380, "Energy transport by accelerated particles in the quiet solar atmosphere,” by Lars Frogner, Boris Gudiksen, and Helle Bakke. A first study of non-thermal particles integrated into an MHD simulation of the solar atmosphere. Click the title to read more.
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
10 June 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
A new facility for airborne solar astronomy: NASA's WB-57
at the 2017 total solar eclipse
-- Amir Caspi, Daniel B. Seaton, Constantine C. C. Tsang, Craig E. DeForest,
Paul Bryans, Edward E. DeLuca, Steven Tomczyk, Joan T. Burkepile,
Thomas 'Tony' Casey, John Collier, Donald 'DD' Darrow, Dominic Del Rosso,
Daniel D. Durda, Peter T. Gallagher, Leon Golub, Matthew Jacyna,
David 'DJ' Johnson, Philip G. Judge, Cary 'Diddle' Klemm, Glenn T. Laurent,
Johanna Lewis, Charles J. Mallini, Thomas 'Duster' Parent, Timothy Propp,
Andrew J. Steffl, Jeff Warner, Matthew J. West, John Wiseman, Mallory Yates,
Andrei N. Zhukov, and the NASA WB-57 2017 Eclipse Observing Team
MinXSS-2 CubeSat mission overview: Improvements from the successful
MinXSS-1 mission
-- James Paul Mason, Thomas N. Woods, Phillip C. Chamberlin, Andrew Jones,
Rick Kohnert, Bennet Schwab, Robert Sewell, Amir Caspi, Christopher S. Moore,
Scott Palo, Stanley C. Solomon, Harry Warren
Lyman alpha Variability During Solar Flares Over Solar Cycle 24
Using GOES-15/EUVS-E
-- Ryan O. Milligan, Hugh S. Hudson, Phillip C. Chamberlin, Iain G. Hannah,
Laura A. Hayes
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
First observation of a transitioning Type II solar radio burst using the
Low-Frequency Array (LOFAR) by Nicolina Chrysaphi et al.
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2579
Loss-cone instability modulation due to a magnetohydrodynamic sausage
mode oscillation in the solar corona by E. P. Carley et al.
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2559
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.