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