The free eclipse app "Eclipse Camera 2019"
This is just a reminder that this app exists, both for IOS and for Android,
and that it can be used to get valuable data from timing C2 and C3. The GPS
capabilities of the mobile phones, plus the existence of the very precise
Kaguya/LRO lunar data, should make this the most precise measurement yet
of the solar radii. The more data the better, and so everybody is encouraged
to let their mobile phone work on this effort. We are hoping for heavy
redundancy to let us approach 1 msec timing precision in the mean.
1) Get the app "Eclipse Camera 2019'. Check it out and identify Equipment
Settings -> Equipment "phone only". Locate the "Eclipse Image Capture"
feature to be prepared.
2) Orient your phone so that the front camera sees the Sun. This can be
quite approximate. Cover it to keep from overheating.
3) One minute before C2 (the app will tell you within a second or two,
depending upon your GPS location), initiate Capture Mode and uncover
the camera. The app will also provide an audible signal prior to C2
as a reminder.
4) Leave the camera alone to do its thing through C3.
5) When you return to Internet range, follow the app's instructions about
upload.
It is also possible to use an external lens with the app. One favorite one
is the Huatop 20x (available on Amazon). This will take interesting coronal
images and also resolve individual Baily's Beads.
This is an outgrowth of the 2017 Megamovie program. See URLs eclipsemega.movie
and https://eclipsecamera.com for more information.
Hugh Hudson and Juan Carlos Martinez Oliveros
3D reconstruction of CME-driven shock-streamer interaction as a coronal
magnetic field diagnostics
by S. Mancuso et al.
http://cesra.net/?p=2212
Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar
Radio Telescopes
by Baolin Tan et al.
http://cesra.net/?p=2229
---------
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
19 June 2019
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
Magnetic Helicity from Multipolar Regions on the Solar Surface
-- Philippe-A. Bourdin, Axel Brandenburg
The width distribution of solar coronal loops and strands - Are we
hitting rock bottom ?
-- Aschwanden,M.J., Peter,H.
Exoplanet predictions based on harmonic orbit resonances
-- Aschwanden,M.J. and Scholkmann,F.
Order out of randomness: Self-organization processes in astrophysics
-- Aschwanden,M.J., Scholkmann,F., Bethune,W., Schmutz,W., Abramenko,W.,
Cheung,M.C.M., Mueller,D., Benz,A.O., Chernov,G., Kritsuk,A.G.,
Scargle,J.D., Melatos,A., Wagoner,R.V., Trimble,V., Green,W.
Convection-driven generation of ubiquitous coronal waves
-- Aschwanden,M.J., Gosic,M., Hurlburt,N.E., and Scullion,E.
The minimum energy principle applied to Parker's coronal braiding
and nanoflaring scenario
-- Aschwanden, M.J. and van Ballegooijen,A.A.
Self-organizing systems in planetary physics: Harmonic resonances
of planet and moon orbits
-- Aschwanden, M.J.
Global energetics of solar flares: VIII. The Low-Energy Cutoff
-- Aschwanden, M.J., Kontar, E.P., and Jeffrey, N.L.S.
Global Energetics of Solar Flares: VII. Aerodynamic Drag in Coronal
Mass Ejections
-- Aschwanden, M.J. and Gopalswamy, N.
Self-organized criticality in solar and stellar flares: Are extreme
events scale-free ?
-- Markus J. Aschwanden
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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 canfield at solar.physics.montana.edu
MAX MILLENNIUM NEWS
12 June 2019
CONTENTS
1. 20TH ANNIVERSARY OF THE FIRST MOTD
2. E-PRINTS POSTED IN THE PAST WEEK
3. FROM THE EDITOR
=====================================================================
1. 20TH ANNIVERSARY OF THE FIRST MOTD
=====================================
> Richard Canfield <richard.canfield at montana.edu>
Exactly twenty years ago, on June 12th, 1999, Dale Gary, Neale
Ranns, and I posted the first Max Millennium Message of the Day
(MOTD), supported by the RHESSI PI team with NASA funding. A year
and a half later, promptly after RHESSI launch, Peter Gallagher
and Bill Marquette sent the first message from the Max Millennium
Chief Observers (MMCOs). These messages continue to this day.
Their effectiveness has been documented in "Performance of Major
Flare Watches from the Max Millennium Program" (2001 - 2010),
Bloomfield, D. S.; Gallagher, P. T.; Marquette, W. H.; Milligan,
R. O.; Canfield, R. C. 2016SoPh..291..411B 2016/02
It is my pleasure to acknowledge the following solar physicists for
their MMCO service over these 20 years, in order of their initial
posts on http://solar.physics.montana.edu/hypermail/mmmotd/date.html
* Peter Gallagher, 700 messages, 2001 - 2009
* Bill Marquette, 2482 messages, 2001 - present
* James McAteer, 617 messages, 2003 - 2009
* Ryan Milligan, 1171 messages, 2007 - present
* Shaun Bloomfield, 869 messages, 2008 - present
* Claire Raftery, 125 messages, 2009 - 2012
* Paul Higgins, 199 messages, 2012 - 2015
* Ying Li, 395 messages, 2015 - present
* Aoife McCloskey, 60 messages, 2018 - present
Please join me in thanking these generous colleagues for their
service to our community using mmchiefobserver (at) gmail.com
2. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
A Wavelet Based Approach to Solar-Terrestrial Coupling
-- Ch. Katsavrias, A. Hillaris, P. Preka--Papadema
Interplanetary Type IV Bursts
-- Alexander Hillaris, Constantine Bouratzis, Alexander Nindos
High resolution observations with Artemis-IV and the NRH. I. Type
IV associated narrow-band bursts
-- C. Bouratzis, A. Hillaris, C.E. Alissandrakis, P. Preka-Papadema,
X. Moussas, C. Caroubalos, P. Tsitsipis, A. Kontogeorgos
Detection of spike-like structures near the front of type-II bursts
-- A.S. Armatas, C. Bouratzis, A. Hillaris, C.E. Alissandrakis,
P. Preka-Papadema, X. Moussas, E. Mitsakou, P. Tsitsipis,
A. Kontogeorgos
High resolution observations with Artemis-JLS, (II) Type
IV associated intermediate drift bursts
-- C. Bouratzis, A. Hillaris, C.E. Alissandrakis, P. Preka-Papadema,
X. Moussas, C. Caroubalos, P. Tsitsipis, A. Kontogeorgos
Oscillation of a small H-alpha surge in a solar polar coronal hole
-- Cho, K.-S., Cho, I.-H., Nakariakov, V.M., Yurchyshyn, V.B., Yang, H.,
Kim, Y.-H., Kumar, P., Magara, T.
Radio Observations of the January 20, 2005 X-Class Event
-- C. Bouratzis, P. Preka-Papadema, A. Hillaris, P. Tsitsipis,
A. Kontogeorgos, V. G. Kurt X. Moussas
Fine Structure of Metric Type-IV Radio Bursts Observed with
the ARTEMIS-IV Radio Spectrograph: Association with Flares
and Coronal Mass Ejections
-- C. Bouratzis, A. Hillaris, C. E. Alissandrakis,
P. Preka-Papadema, X. Moussas, C. Caroubalos, P. Tsitsipis,
A. Kontogeorgos
Spectral Analysis of the September 2017 Solar Energetic
Particle Events
-- A. Bruno, E.R. Christian, G.A. de Nolfo, I.G. Richardson, J.M. Ryan
Solar Energetic Particle Events Observed by the PAMELA Mission
-- A. Bruno, G. A. Bazilevskaya, M. Boezio, E. R. Christian,
G. A. de Nolfo, M. Martucci, M. Merge', V. V. Mikhailov, R.
Munini, I. G. Richardson, J. M. Ryan, S. Stochaj, O. Adriani, G. C.
Barbarino, R. Bellotti, E. A. Bogomolov, M. Bongi, V. Bonvicini,
S. Bottai, F. Cafagna, D. Campana, P. Carlson, M. Casolino,
G. Castellini, C. De Santis, V. Di Felice, A. M. Galper,
A. V. Karelin, S. V. Koldashov, S. Koldobskiy, S. Y. Krutkov,
A. N. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, A. G. Mayorov,
W. Menn, E. Mocchiutti, A. Monaco, N. Mori, G. Osteria, B. Panico,
P. Papini, M. Pearce, P. Picozza, M. Ricci, S. B. Ricciarini,
M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi,
E. Vannuccini, G. I. Vasilyev, S. A. Voronov, Y. T. Yurkin,
G. Zampa, N. Zampa
COMPARING LONG-DURATION GAMMA-RAY FLARES AND HIGH-ENERGY SOLAR
ENERGETIC PARTICLES
-- G. A. de Nolfo, A. Bruno, J. M. Ryan, S. Dalla,
J. Giacalone, I. G. Richardson, E. R. Christian, S. J. Stochaj,
G. A. Bazilevskaya, M. Boezio, M. Martucci, V. V. Mikhailov,
R. Munini
Characteristics of ephemeral coronal holes
-- A. R. Inglis, R. E. O'Connor, W. D. Pesnell, M. S. Kirk, N. Karna
The Role of Energy Diffusion in the Deposition of Energetic Electron
Energy in Solar and Stellar Flares
-- Natasha L. S. Jeffrey, Eduard P. Kontar, Lyndsay Fletcher
3. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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 canfield at solar.physics.montana.edu
MAX MILLENNIUM NEWS
05 June 2019
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
Spectroscopy and Differential Emission Measure diagnostics of a
coronal dimming associated with a fast halo CME
-- Astrid M. Veronig, Peter Gomory, Karin Dissauer, Manuela Temmer,
Kamalam Vanninnathan
Evolution of Magnetic Helicity in Solar Cycle 24
-- V.V. Pipin, A.A. Pevtsov, Yang Liu, A.G. Kosovichev
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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 canfield at solar.physics.montana.edu
MAX MILLENNIUM NEWS
29 May 2019
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
Damping of Propagating Kink Waves in the Solar Corona
-- Ajay K. Tiwari, Richard J. Morton, Stephane Rggnier, and
James A. McLaughlin
Non-equilibrium ionization effects on solar EUV and X-ray imaging
observations
-- Jin-Yi Lee, John C. Raymond, Katharine K. Reeves, Chengcai Shen,
Yong-Jae Moon, and Yeon-Han Kim
Linear waves in a non-equilibrium ionisation partially ionised plasma
-- Istvan Ballai
How Many Twists Do Solar Coronal Jets Release?
-- Jiajia Liu, Yuming Wang, Robertus Erdélyi
Different Signatures of Chromospheric Evaporation in Two Solar Flares
Observed with IRIS
-- Y. Li, M. D. Ding, J. Hong, H. Li, W. Q. Gan
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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 canfield at solar.physics.montana.edu
No. 351, “The Cosmic-Ray Shadow and Coronal Magnetism”, by Frederik Tenholt: Measuring the coronal magnetic field in Antarctica.
No. 350, “Kristian Birkeland”, by Hugh Hudson and Lyndsay Fletcher: Space weather a century ago.
See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets .
We publish these at roughly two-week intervals and welcome contributions,
which should be related, at least loosely, to RHESSI science.
The effect of scattering on the apparent positions of solar radio
sources observed by LOFAR
by Mykola Gordovskyy
http://cesra.net/?p=2206
High‐Frequency Communications Response to Solar Activity in September
2017 as Observed by Amateur Radio Networks
by Nathan A. Frissell
http://cesra.net/?p=2198
----
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/http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
22 May 2019
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 Physical Nature of Spiral Wave Patterns in Sunspots
-- Juhyung Kang, Jongchul Chae, V. M. Nakariakov, Kyuhyoun Cho,
Hannah Kwak, Kyeore Lee
Predicting Solar Flares Using a Long Short-Term Memory Network
-- Hao Liu, Chang Liu, Jason T. L. Wang, Haimin Wang
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
15 May 2019
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
Coronal loop transverse oscillations excited by different driver
frequencies
-- Andrey Afanasyev, Konstantinos Karampelas, Tom Van Doorsselaere
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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 richard.canfield at montana.edu