Dear colleagues,
There is one week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the fourth-annual installment of our session for next-generation remote-sensing missions. Like last year, this year the focus includes all remote sensing, including imaging, spectroscopy, polarimetry, and combinations of those, plus anything else I'm missing. Given the imminent Decadal Survey, we encourage submissions with an eye both for near-term _and_ long-term (decadal or beyond) timescales for development.
Session link and description are below. Deadline is 11:59pm EDT on Aug 4th (next Wednesday).
We look forward to your exciting submissions!
https://agu.confex.com/agu/fm21/prelim.cgi/Session/121896
SH017 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond
Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; MinXSS; SphinX; the FOXSI, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories such as NuSTAR, Fermi, ALMA, and VLA, have significantly advanced our understanding of these phenomena. They have also shown the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes.
This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot and non-thermal) aspects of the Sun, and the science enabled by such new observations.
--- Amir Caspi, Lindsay Glesener, Jenna Samra, & Athiray Panchapakesan
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 411, “Flare Pulsations and the Heliosphere” by Brendan CLARKE et al.; flare pulsations turn out to link closely to structures in the distant heliosphere.
No. 412, “The Morphology of Flare Time Profiles,” by Larisa KASHAPOVA et al.; systematic comparison of solar and stellar flaring time profiles.
No. 413, “Impulsive and Gradual Eruptive Game Flares and Associated CMEs,” by Alexey STRUMINSKY et al.; Extreme behavior of flare/CME events explained by environment.
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
21 July 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Temperature in Solar Sources of 3He-rich Solar Energetic Particles
and Relation to Ion Abundances
-- Bucik, R., Mulay, S. M., Mason, G. M., Nitta, N. V., Desai, M. I., Dayeh, M. A.
The long period of 3He-rich solar energetic particles measured
by Solar Orbiter 2020 November 17–23
-- Bucik, R., Mason, G. M., Gomez-Herrero, R., Lario, D., Balmaceda, et al.
Tracing H-alpha Fibrils through Bayesian Deep Learning
-- Haodi Jiang, Ju Jing, Jiasheng Wang, Chang Liu, Qin Li, Yan Xu,
Jason T. L. Wang, Haimin Wang
Energetics and 3-D Structure of Elementary Events in Solar Coronal Heating
-- G. Einaudi, R.B. Dahlburg, I. Ugarte-Urra, J.W. Reep, A.F. Rappazzo, M. Velli
Forecasting the Remaining Duration of an Ongoing Solar Flare
-- Jeffrey W. Reep & Will T. Barnes
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
14 July 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
A fundamental mechanism of solar eruption initiation
-- Chaowei Jiang, Xueshang Feng, Rui Liu, XiaoLi Yan, Qiang Hu,
Ronald L. Moore, Aiying Duan, Jun Cui, Pingbing Zuo, Yi Wang & Fengsi Wei
Thermal Trigger for Solar Flares III: Effect of the Oblique Layer Fragmentation
-- Leonid Ledentsov
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
As part of wrapping up the RHESSI mission (2002 - 2018), we are generating a final Mission Archive in order to ensure the continued availability of the RHESSI science data in the future.
The data archive and associated documentation will be hosted at the Solar Data Analysis Center (SDAC) (https://umbra.nascom.nasa.gov/) at Goddard. The latest RHESSI data analysis software and ancillary database files will continue to be available on SSW.
In addition to the Level-0 and quicklook data files, a number of prepared products are also being archived at the SDAC, allowing both experienced and inexperienced users to view and analyze RHESSI data. These prepared products (which are in various states of completeness) include images of more than 75,000 flares in optimized time/energy bins, and fine and coarse resolution energy spectra and visibility data. The images can be viewed online and imagecube FITS files are available to download. The spectra and visibilities are provided in standard FITS files that can be downloaded and used in the RHESSI software environment, or read with standard FITS readers for stand-alone processing.
For access to the archive products, please go to the RHESSI web site at https://hesperia.gsfc.nasa.gov/rhessi/ and click on the 'Mission Archive' tab (on the far right). This will take you to a summary of the products, their current status, and links to the various archives.
Kim Tolbert and Brian Dennis
MAX MILLENNIUM NEWS
7 July 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Measurements of Coronal Magnetic Field Strengths in Solar Active Region Loops
-- David H. Brooks, Harry P. Warren, Enrico Landi
Characteristic time of stellar flares on Sun-like stars
-- Y Yan, H He, C Li, A Esamdin, B L Tan, L Y Zhang, H 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
30 June 2021
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
M-dwarf's Chromosphere, Corona and Wind Connection via the Nonlinear Alfven Wave
-- Takahito Sakaue and Kazunari Shibata
Bayesian evidence for a nonlinear damping model for coronal loop oscillations
-- I. Arregui
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. 409, “Nonequilibrium Ionization of Flare Plasma Observed by Hinode/EIS” by Shinsuke IMADA: Evidence for Nonequilibrium Ionization of Flare Plasma Observed by Hinode/EIS.
No. 410, “STIX, the Hard X-Ray Telescope on board Solar Orbiter” by Andrea Francesco BATTAGLIA and Säm KRUCKER: STIX is operational and producing great 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 often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
MAX MILLENNIUM NEWS
23 June 2021
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
Small-scale Turbulent Motion of the Plasma in a Solar Filament
as the Precursor of Eruption
-- Daikichi Seki, Kenichi Otsuji, Hiroaki Isobe, Giulio Del Zanna,
Takako T. Ishii, Takahito Sakaue, Kiyoshi Ichimoto, Kazunari Shibata
Validation of the PDFI_SS method for electric field inversions
using a magnetic flux emergence simulation
-- Andrey N. Afanasyev, Maria D. Kazachenko, Yuhong Fan, George H. Fisher,
Benoit Tremblay
Investigation on the Spatiotemporal Structures of Supra-Arcade Spikes
-- Rui Liu & Yuming Wang
Magnetic helicity and energy budget around large confined and
eruptive solar flares
-- Manu Gupta, J. K. Thalmann, A. M. Veronig
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
16 June 2021
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
One dimensional prominence threads: I. Equilibrium models
-- J. Terradas, M. Luna, R. Soler, R. Oliver, M. Carbonell, J. L Ballester
Time-dependent properties of sunspot groups I. Lifetime and asymmetric evolution
-- E. Forgacs-Dajka, L. Dobos, I. Ballai
Investigating Remote-sensing Techniques to Reveal Stealth Coronal Mass Ejections
-- Erika Palmerio, Nariaki V. Nitta, Tamitha Mulligan, Marilena Mierla,
Jennifer O'Kane, Ian G. Richardson, Suvadip Sinha, Nandita Srivastava,
Stephanie L. Yardley, Andrei N. Zhukov
ALMA observations of the variability of the quiet Sun at millimeter wavelengths
-- A. Nindos, S. Patsourakos, C.E. Alissandrakis, T.S. Bastian
The Poissonian origin of power laws in solar flare waiting time distributions
-- Aschwanden,M.J., Johnson,J.R., and Nurhan,Y.
Correlation of the sunspot number and the waiting time distribution
of solar flares, coronal mass ejections, and solar wind switchback events
observed with the Parker Solar Probe
-- Aschwanden, M.J. and Dudok de Wit, T.
Self-organized criticality in stellar flares
-- Aschwanden, M.J.and Guedel, M.
Finite system-size effectrs in self-organizing criticality systems
-- Aschwanden, M.J.
Global energetics of solar flares.
XII. Energy scaling laws
-- Aschwanden, M.J.
Global energetics of solar flares.
XI. Flare magnitude predictions of the GOES class
-- Aschwanden, M.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