What to Do When Your Temper Flares


Book Description

What to Do When Your Temper Flares guides children and their parents through the cognitive-behavioral techniques used to treat problems with anger. Engaging examples, lively illustrations, and step-by-step instructions teach children a set of "anger dousing" methods aimed at cooling angry thoughts and controlling angry actions, resulting in calmer, more effective kids. This interactive self-help book is the complete resource for educating, motivating, and empowering children to work toward change.







Flare


Book Description

The Steel family won’t go down on his watch… Rory Pike never imagined she’d fall for a Steel, but she has—Brock Steel, a renowned womanizer, no less. While passion flares between them, Rory knows they’re on different pages in life. She’s older and ready to settle down. Brock? Not so much. Brock is enamored with Rory, but he’s content to simply live in the moment, especially with everything that’s currently going down in his personal life. Brock’s discovery that his father has kept important information from him—information that could lead to the downfall of his famous family—leads him to question everything he’s known since he was a child. Rory has her own problems as well, and when they converge with Brock’s in the form of one person, the mysteries surrounding the Steel family deepen. Rory and Brock are determined to find the truth…no matter what the cost.







Solar and Stellar Flares


Book Description

concert at Dinkelspiel Auditorium 'An Evening of Songs and Arias' hosted by Dr Kip Cranna of San Francisco Opera, produced and directed by Elizabeth Tucker, and featuring soprano Ellie Holt Murray, mezzo-soprano Marsha Sims; tenor Richard Walker, and baritone David Taft Kekuewa, with piano accompaniment by Mark Haffner, staff coach for San Francisco Opera. Two scientific themes clearly emerged from this conference: (1) the key to progress in flare research lies in a multispectral approach with as much temporal resolution as the photon fluxes allow; and (2) the key to understanding the physics lies in a dynamic interaction between solar and stellar investigations and investigators. During the eight sessions solar and stellar topics were balanced and intermixed in 33 invited and oral presentations. We are particularly pleased that these proceedings will be the springboard to publication of solar-stellar articles in the journal Solar Physics. In addition, 115 very exciting posters were also displayed and a companion volume containing many of these is available as a publication of the Catania Astrophysical Observatory. We dedicate this book to the Solar Maximum Mission and to the Flare Star Consor tium. To all our solar-stellar friends and colleagues: 'Thank you!' BERNHARD M. HAISCH and MARCELLO RODONO 28 March. 1989 AN OVERVIEW OF SOLAR AND STELLAR FLARE RESEARCH BERNHARD M. HAlSCH Div. 91-30. Bldg. 255. Lockheed Palo Alto Research Laboratory. 3251 Hanover St .• Palo Alto. CA 94304. U.S.A.







Flare Observations in the IRIS Era: What Have We Learned, and What’s Next?


Book Description

Since its launch in 2013, IRIS has observed more than 10 X-class, over 100 M-class and more than 600 C-class flares at unprecedented spatial and temporal resolution. Thanks to the rich diagnostics that cover the physical conditions of the solar atmosphere from the photosphere to the hottest parts of the flaring corona, IRIS observations have provided exciting new results and constraints on flare heating models, significantly expanding our knowledge of how flares are triggered, and how the non-thermal energy is released, propagates downward from the corona, and is deposited in the low atmosphere. At the same time, the new discoveries provided by IRIS have raised new unresolved questions and new challenges for theoretical models. For instance, current hydrodynamic models still cannot fully explain many features observed by IRIS during both the impulsive and gradual phases such as the dynamics of the evaporative/condensation flows, the large line broadenings, and the puzzling complex and broad chromospheric lines. In addition, important questions remain regarding the details of the energy propagation and dissipation in flares, the importance of Alfvén waves vs electron-beam and thermal conduction heating, and the effects from large-scale reconfiguration of the magnetic field during flares.




Solar Flare Magnetic Fields and Plasmas


Book Description

This volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models of the solar interior and atmosphere, (2) The connection between observed radiation processes occurring during flares and the underlying flare energy release and transport mechanisms, (3) The global balance of forces and momenta that occur during flares, (4) The data-analysis and theoretical tools needed to understand and assimilate vector magnetogram observations and (5) Connecting flare and CME phenomena to the topological properties of the magnetic field in the Solar Atmosphere. The role of the Sun’s magnetic field is a major emphasis of this book, which was inspired by a workshop honoring Richard C. (Dick) Canfield. Dick has been making profound contributions to these areas of research over a long and productive scientific career. Many of the articles in this topical issue were first presented as talks during this workshop and represent substantial original work. The workshop was held 9 – 11 August 2010, at the Center Green campus of the National Center for Atmospheric Research (NCAR) in Boulder, Colorado. This volume is aimed at researchers and graduate students active in solar physics, solar-terrestrial physics and magneto-hydrodynamics. Previously published in Solar Physics journal, Vol. 277/1, 2012.




Flare Stars in Star Clusters, Associations, and the Solar Vicinity


Book Description

Some 70 papers present the flare star problem from both a physical and evolutionary aspect, and represent an interaction between investigators working on flare stars in clusters and associations, and those working on the UV Ceti stars in solar vicinity. The variety of perspectives reveal a physical similarity among several non-stable phenomena, and suggest that the different manifestations of stellar activity result from the release of some unknown kind of energy in the outer layers of young stars. The papers deal not only with different aspects of flare stars, but also with such related objects as T Tauri stars, fluors, and Herbig-Haro objects. Annotation copyrighted by Book News, Inc., Portland, OR




Flare Stars


Book Description

Flare Stars covers the significant progress in photoelectric, photographic, and spectral observations of flare stars. Flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes believed to be due to extremely intense flares. This book is composed of 16 chapters and begins with an overview of flare stars and the hypothesis of infrared photon transformation. The succeeding chapters deal with the inverse Compton Effect, X-ray radiation and the theory of the transition radiation and its importance to the T Tauri type stars and peculiar objects. These topics are followed by analysis of the photometric and colorimetric flare data based on the fast-electron hypothesis. Other chapters consider the theory of the chromophore of flare stars and the general laws for the behavior of flare stars in stellar association and for T Tauri type stars. The remaining chapters explore the observational data that have shed light on the problems of radio emission and flare dynamics. These chapters also describe the great cosmogonic importance of stellar flares, particularly for understanding the nature and the true character of energy sources within the stars. This book will be of great value to astronomers and researchers.