http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 428, “Solar Hard X-rays with Insight,” by Wei WANG and Ping ZHANG. A spectacular limb flare introduces Insight/HXMT, a new high-energy observational resource.
No. 429, “Carl Størmer,” by Hugh HUDSON and Lyndsay FLETCHER. Størmer and the theory of particle trapping in magnetic loops.
No. 430, “Sun-as-a-star spectroscopic observations of the line-of-sight velocity of the solar eruption SOL2021-10-28T15:35,” by Yu XU and Hui TIAN. The observation of the full 3D velocity of a CME, for a RHESSI anniversary event.
No. 431, “Thermal/non-thermal with MinXSS and RHESSI,” by Shunsaku NAGASAWA. Time-domain studies of improved X-ray spectra reveal a “super-hot” component.
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.
Dear colleagues,
Registration and abstract submission are CLOSING SOON for the Solar Physics High Energy Research (SPHERE) Workshop, to be held 11–15 July 2022. The workshop will be a hybrid format with online access and two in-person locations: Southwest Research Institute (SwRI) in Boulder, Colorado, USA and Fachhochschule Nordwestschweiz (FHNW) in Windisch, Switzerland.
For full details, please visit the workshop website: https://sphere.boulder.swri.edu
Abstract submission deadline: 17 June 2022
NOTE: please contact the organizers if you will have trouble meeting this deadline and need additional time.
The complete schedule/agenda will be posted ASAP, before the end of June.
Registration deadlines: U.S. – 30 June 2022 | Europe – 11 July 2022 | virtual – 11 July 2022
Registration fee: none
U.S. hotel reservation deadline: 30 June 2022 (through the registration form)
Oral presentation requests will be accepted from early-career researchers (up to 5 years post PhD) and students only – the ongoing pandemic has severely restricted opportunities for young researchers, so we are prioritizing oral presentations for them.
Poster presentations will be accepted from any attendee. Because of the hybrid format, posters must be submitted as PDF for online access, and may also be presented in person (format TBD).
We hope to see you soon in Boulder, Windisch, or online!
– Amir Caspi & Säm Krucker, on behalf of the organizing committee
MAX MILLENNIUM NEWS
8 June 2022
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
Geometric Assumptions in Hydrodynamic Modeling of Coronal and Flaring Loops
-- Reep, Jeffrey W. ; Ugarte-Urra, Ignacio ; Warren, Harry P. ; Barnes, Will T.
Sun-as-a-star Analysis of H-alpha Spectra of a Solar Flare Observed
by SMART/SDDI: Time Evolution of Red Asymmetry and Line Broadening
-- Kosuke Namekata, Kiyoshi Ichimoto, Takako T. Ishii, Kazunari Shibata
Searching for quasi-periodic oscillations in astrophysical transients
using Gaussian processes
-- M. Huシbner, D. Huppenkothen, P. D. Lasky, A. R. Ingiis, C. Ick, D. W. Hogg
Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption
-- Reetika Joshi, Cristina H. Mandrini, Ramesh Chandra, Brigitte Schmieder,
Germa。n D. Cristiani, Cecilia Mac Cormack, Pascal eテゥmoulin, Hebe Cremades
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
Dear colleagues,
Registration and abstract submission is NOW OPEN for the Solar Physics High Energy Research (SPHERE) Workshop, to be held 11–15 July 2022. The workshop will be a hybrid format with online access and two in-person locations: Southwest Research Institute (SwRI) in Boulder, Colorado, USA and Fachhochschule Nordwestschweiz (FHNW) in Windisch, Switzerland.
For full details, please visit the workshop website: https://sphere.boulder.swri.edu
Registration deadline: U.S. – 30th June 2022 | Europe – 11th July 2022
Registration fee: none
U.S. hotel reservation deadline: 30th June 2022 (through the registration form)
Abstract submission deadline: 17th June 2022
NOTE: Please contact the organizers if you will have trouble meeting the abstract deadline and need additional time
Oral presentation requests will be accepted from early-career researchers (up to 5 years post-PhD) and students only – the ongoing pandemic has severely restricted opportunities for young researchers, so we are prioritizing oral presentations for them.
Poster presentations will be accepted from any attendee. Because of the hybrid format, posters must be submitted as PDF for online access, and may also be presented in person (format TBD).
We hope to see you soon in Boulder, Windisch, or online!
– Amir Caspi & Säm Krucker, on behalf of the organizing committee
MAX MILLENNIUM NEWS
1 June 2022
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
Current-sheet Oscillations Caused by Kelvin-Helmholtz Instability
at the Loop Top of Solar Flares
-- Yulei Wang, Xin Cheng, Zining Ren and Mingde Ding
Annihilation of Magnetic Islands at the Top of Solar Flare Loops
-- Yulei Wang, Xin Cheng, Mingde Ding and Quanming Lu
Three-dimensional Magnetic and Thermodynamic Structures of Solar Microflares
-- Li, Z. F., Cheng, X., Chen, F., Chen, J. & Ding, M. D.
Grow-up of a Filament Channel by Intermittent Small-scale Magnetic Reconnection
-- Li, H. T., Cheng, X., Guo, J. H., Yan, X. L., Wang, L. F., Zhong, Z.,
Li, C. & Ding, M. D.
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 May 2022
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 solar jet formation and their associated waves and instabilities
-- Samuel Skirvin, Gary Verth, Jose Juan Gonzalez-Aviles, Sergiy Shelyag,
Rahul Sharma, Francisco S. Guzman, Istvan Ballai, Eamon Scullion,
Suzana Silva, Viktor Fedun
Invited Review: Short-term Variability with the Observations
from the Helioseismic and Magnetic Imager (HMI)
Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism
-- Maria D. Kazachenko, Marcel F. Corchado-Albelo, Cole A. Tamburri,
Brian T. Welsch
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
Two recent solar radio science nuggets are available online:
Langmuir-Slow Extraordinary Mode Magnetic Signature Observations with
Parker Solar Probe
by A. Larosa et al
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3267
LOFAR size and shape measurements of solar metric radio burst sources
by Gordovskyy et al
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3260
------
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
18 May 2022
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 first look at the submillimeter Sun with ALMA
-- C. E. Alissandrakis, T. S. Bastian, and A. Nindos
Data-driven modeling of solar coronal magnetic field evolution and eruptions
-- Chaowei Jiang, Xueshang Feng, Yang Guo, Qiang Hu
Properties and Energetics of Magnetic Reconnection: I. Evolution of Flare Ribbons
-- J. Qiu & J. Cheng
A new look at the frequency-dependent damping of slow-mode waves in the solar corona
-- Dmitrii Y. Kolotkov, Valery M. Nakariakov
What determines active region coronal plasma composition?
-- Teodora Mihailescu, Deborah Baker, Lucie M. Green, Lidia van Driel-Gesztelyi,
David M. Long, David H. Brooks, Andy S. H. To
Characteristics and evolution of sheath and leading edge structures
of interplanetary coronal mass ejections in the inner heliosphere
based on Helios and Parker Solar Probe observations
-- Manuela Temmer and Volker Bothmer
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
Dear colleagues,
The Solar Physics High Energy Research (SPHERE) Workshop -- formerly known as the RHESSI workshop, and now motivated by SolO/STIX, MinXSS, EOVSA, and many other current and upcoming missions -- will be held 11–15 July 2022. The workshop will be a hybrid format with online access and two in-person locations: Southwest Research Institute (SwRI) in Boulder, Colorado, USA and Fachhochschule Nordwestschweiz (FHNW) in Windisch, Switzerland.
The workshop agenda will include plenary topical sessions, held jointly between all locations, featuring invited talks and facilitated, open discussions on targeted science questions. This interactive format is intended to foster both broader and deeper collaboration and understanding amongst our community, to propel progress and enhance success by breaking down silos both within the high-energy solar physics and among solar and space physics in general. Additional independent morning (EU) and afternoon (US) sessions will feature tutorials, posters, early-career talks, and open collaboration.
Registration is required, and U.S. hotel accommodations (for the contract hotel) will be handled through the registration form. Abstracts for posters and early-career presentations, and suggestions for open topical discussions, will be solicited soon.
The workshop website at https://sphere.boulder.swri.edu is operational with preliminary information, including travel information, and will be updated soon with registration information and deadlines.
We hope to see you soon in Boulder, Windisch, or online!
– Amir Caspi & Säm Krucker, on behalf of the organizing committee
MAX MILLENNIUM NEWS
11 May 2022
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
Slow magnetoacoustic oscillations in stellar coronal loops
-- Lim, D., Nakariakov, V.M., Moon, Y.-J.
Kink Oscillation of a Flux Rope During a Failed Solar Eruption
-- Pankaj Kumar, Valery M. Nakariakov, Judith T. Karpen, C. Richard DeVore,
Kyung-Suk Cho
A publicly available multi-observatory data set of an enhanced network patch
from the Photosphere
-- Adam R. Kobelski, Lucas A. Tarr, Sarah A. Jaeggli, Nicholas Luber,
Harry P. Warren and Sabrina Savage
Type IV Radio Bursts and Associated Active Regions in the Sunspot Cycle 24
-- Anshu Kumari
Theory of Fluid Instabilities in Partially Ionized Plasmas: An Overview
-- R. Soler, J. L. Ballester
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