http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 396, “Investigation of Small-Scale Energy Releases in Hard X-rays with FOXSI”, by Subramania ATHIRAY and Juliana VIEVERING: Hard X-rays and high temperatures in the feeblest microflares.
No. 397, "Solar effects in the local interstellar medium”, by Don GURNETT and Hugh HUDSON: Relativistic particle events observed _in situ_ in the local interstellar medium.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
9 December 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
Alfvenic Perturbations in a Sunspot Chromosphere Linked to Fractionated Plasma
in the Corona
-- D. Baker, M. Stangalini, G. Valori, D. H. Brooks, A. S. H. To,
L. van Driel-Gesztelyi, P. Demoulin, D. Stansby, D. B. Jess, S. Jafarzadeh
Analyzing the propagation of EUV waves and their connection with type II radio
bursts by combining numerical simulations and multi-instrument observations
-- A. Koukras, C. Marque, C. Downs, L. Dolla
Three-dimensional simulations of the inhomogeneous Low Solar Wind
-- N. Magyar, V. M. Nakariakov
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
2 December 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
Initiation and Early Kinematic Evolution of Solar Eruptions
-- Cheng, X.; Zhang, J.; Kliem, B.; Torok, T.; Xing, C.; Zhou, Z. J.;
Inhester, B.; Ding, M. D.
Differential rotation of the chromosphere in the He I absorption line
-- KJ Li, JC Xu, JL Xie, and W Feng
Evolution of the Toroidal Flux of CME Flux Ropes during Eruption
-- Xing, C.; Cheng, X.; Ding, M. D.
The Kinematic Evolution of Erupting Structures in Confined Solar Flares
-- Huang, Z. W.; Cheng, X.; Ding, M. D.
Deriving CME density from remote sensing data and
comparison to in-situ measurements
-- M. Temmer, L. Holzknecht, M. Dumbovic, B. Vrsnak, N. Sachdeva,
S.G. Heinemann, K. Dissauer, C. Scolini, E. Asvestari, A. M. Veronig,
S. J. Hofmeister
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
25 November 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
Non-Neutralized Electric Current of Active Regions Explained
as a Projection Effect
-- Xudong Sun, Mark C. M. Cheung
The effect of magnetic field on the damping of slow waves in the solar corona
-- T. J. Duckenfield, D. Y. Kolotkov, and V. M. Nakariakov
Soft X-Ray Observations of Quiescent Solar Active Regions using Novel
Dual-zone Aperture X-ray Solar Spectrometer (DAXSS)
-- Bennet D. Schwab, Robert H. A. Sewell, Thomas N. Woods, Amir Caspi,
James Paul Mason, and Christopher Moore
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
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 393, “Self-Consistent Flare Model”, by Wenzhi RUAN and Rony KEPPENS: Energy trnasport by fast particles made self-consistent with MHD flare modeling.
No. 394, “Probing the solar coronal heating function with slow magnetoacoustic waves," by Dmitriii KOLOTKOV et al.: Coronal heating models meet damped slow magnetoacoustic waves.
No. 395. “What drives impulsive coronal heating?” by Pradeep CHITTA et al.: Impulsive footpoint emissions suggest magnetic reconnection in the chromosphere.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
18 November 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
Proper Orthogonal and Dynamic Mode Decomposition of Sunspot Data
-- A. B. Albidah, W. Brevis, V. Fedun, I. Ballai, D. B. Jess, M. Stangalini,
J. Higham and G. Verth
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
11 November 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 Properties of Superflares on Solar-type Stars:
Results Using All of the Kepler Primary Mission Data
-- Soshi Okamoto, Yuta Notsu, Hiroyuki Maehara, Kosuke Namekata, Satoshi Honda,
Kai Ikuta, Daisaku Nogami, Kazunari Shibata
Turbulent viscosity and effective magnetic Prandtl number
from simulations of isotropically forced turbulence
-- Petri J. Kapyla, Matthias Rheinhardt, Axel Brandenburg, Maarit J. Kapyla
Time and Charge-Sign Dependence of the Heliospheric Modulation of Cosmic Rays
-- O.P.M. Aslam, D. Bisschoff, M. D. Ngobeni, M. S. Potgieter, R. Munini,
M. Boezio, & V. V. Mikhailov
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 November 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
Bayesian Analysis of Quasi-periodic Pulsations in Stellar Flares
-- D. J. Pascoe, A. Smyrli, T. Van Doorsselaere, and A.-M. Broomhall
Cause and Kinematics of a Jetlike CME
-- Reetika Joshi, Yuming Wang, Ramesh Chandra, Quanhao Zhang, Lijuan Liu,
Xiaolei Li
The role of small-scale surface motions in the transfer of twist
to a solar jet from a remote stable flux rope
-- Reetika Joshi, Brigitte Schmieder, Guillaume Aulanier, veronique Bommier,
Ramesh Chandra
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. 390, “Prediction of Solar Cycle 25”, by Leif SVALGAARD. Now we know how big the next solar maximum will be.
No. 391, “Electric Current Neutralization and Eruption”, by Ellis AVALLONE and Xudong SUN. Coronal currents without neutralizing return currents correlate with eruption.
No. 392, “Hot Flare Onsets”, by Hugh HUDSON et al. The pre-impulsive temperatures of solar flares are already hot, 10-15 MK.
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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.