MAX MILLENNIUM NEWS
25 May 2022
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
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
MAX MILLENNIUM NEWS
4 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
Quasiperiodic Energy Release and Jets at the Base of Solar Coronal Plumes
-- Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest,
Nour E. Raouafi, C. Richard DeVore
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
27 April 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
The Coupling of an EUV Coronal Wave and Ion Acceleration
in a Fermi-LAT Behind-the-Limb Solar Flare
-- Melissa Pesce-Rollins, Nicola Omodei, Sam Krucker, Niccolo' Di Lalla,
Wen Wang, Andrea F. Battaglia, Alexander Warmuth, Astrid M. Veronig and
Luca Baldini
Reconciling Power Law Slopes in Solar Flare and Nanoflare Size Distributions
-- Markus J. Aschwanden
A Model of Homologous Confined and Ejective Eruptions Involving Kink Instability
and Flux Cancellation
-- Alshaimaa Hassanin; Bernhard Kliem; Norbert Seehafer; Tibor Torok
Detection of stellar-like abundance anomalies in the slow solar wind
-- David H. Brooks, Deborah Baker, Lidia van Driel-Gesztelyi, Harry P. Warren,
Stephanie L. Yardley
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
20 April 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
Magnetosheath jet occurrence rate in relation to CMEs and SIRs
-- Florian Koller, Manuela Temmer, Luis Preisser, Ferdinand Plaschke,
Paul Geyer, Lan K Jian, Owen Wyn Roberts, Heli Hietala, Adrian T. LaMoury
Microwave Perspective on Magnetic Breakout Eruption
-- Jeongwoo Lee
Observations of Extremely Strong Magnetic Fields in Active Region NOAA 12673
Using GST Magnetic Field Measurement
-- Vsevolod Lozitsky, Vasyl Yurchyshyn, Kwangsu Ahn, and Haimin 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
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
Fundamental electromagnetic emissions by a weak electron beam in solar
wind plasmas with density fluctuations
by C. Krafft and P. Savoini
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3239
---
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.
Hi All,
In case you hadn’t seen it and were still debating where to submit your abstract, I wanted to remind you about session 23 before the TESS abstract deadline tomorrow: “Investigating the Solar Chromosphere at Millimeter Wavelengths”.
Meeting website:
https://aas.org/meetings/tess2022
If you have any science results utilizing millimeter wavelength observations, or that could benefit from millimeter wavelength observations, we encourage you to submit an abstract.
Thank you, and we hope to see you in Bellevue!
Adam, on behalf of the ALMA Solar Development Team
23. Title: Investigating the Solar Chromosphere at Millimeter Wavelengths
Conveners: Adam Kobelski (NASA Marshall Space Flight Center), Gianna Cauzzi (National Solar Observatory)
One of the most notable new developments in the study of the solar chromosphere is the ability to obtain high resolution observations of the Sun at millimeter wavelengths using the Atacama Large Millimeter Array (ALMA).
This interferometric imaging array of 64 dishes, located at an altitude of 5000 meters in Chile, is currently able to observe the Sun at frequencies from 90 GHz to 370 GHz (~ 0.85 – 3.0 mm wavelengths), achieving spatial resolutions as high as 0.6”, with 1 s cadence.
The millimeter continuum is emitted by electrons over much of the range from the temperature minimum to the transition region, and provides a direct measure of the local temperature. Thus, ALMA data provide important new diagnostics for studying the spatio-temporal structure and dynamics of the solar chromosphere. Over the past few years, the community has made significant progress in the processing and interpretation of this interferometric data. and numerous studies have used these data to probe various features and processes in the solar atmosphere. Within this session, we aim to introduce the community to both novel science results obtained by this new facility and to highlight future scientific opportunities enabled by ALMA, especially those in coordination with ground and spaced based instruments. We invite contributions from previous users of ALMA about their results, but also presentations of studies of the solar chromosphere that would potentially benefit from the additional temperature and magnetic field diagnostics from these millimeter observations. Two featured talks will provide a broad overview of solar ALMA science, including the potential for observations of solar activity and flares, and provide guidance for potential new users of the facility, with the goal of inspiring a broader participation in this exciting science.