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Author: James Haick III
Publisher: James Haick
ISBN: 1427696462
Category :
Languages : en
Pages : 30
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Book Description
Jake wakes up to find that it's a completely different world from the day before. All electricity has stopped working. Jake decides to search for his family and friends in hopes to get an explaination of why things are the way they are.
Author: James Haick III
Publisher: James Haick
ISBN: 1427696462
Category :
Languages : en
Pages : 30
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Book Description
Jake wakes up to find that it's a completely different world from the day before. All electricity has stopped working. Jake decides to search for his family and friends in hopes to get an explaination of why things are the way they are.
Author: Hermine Vloemans
Publisher: Springer Science & Business Media
ISBN: 9401022313
Category : Science
Languages : en
Pages : 308
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Book Description
Sudden Ionospheric Disturbances resulting from an interaction of the Solar Flare radiation with the constituents of the upper atmosphere constitute one of the three major aspects of ground level monitoring of solar flares -the other two being optical observations of flares, and the observations of solar bursts in radio wavelengths. SIDs, therefore, form a major part of flare monitoring programme in many observatories. Unlike the other two, however, the ionospheric effects of flares provide one major additional source of interest - the reaction of the ionospheric plasma to an impulsive ionization. The high atmosphere provides a low pressure laboratory without walls in which a host of reactions occur between electrons, ions and neutral particles. The resulting products and their distributions may bear no resemblance to those of the primary neutral constituents or their direct ionization products. The variations with the time of the day, with season and with solar activity that form the bulk of the ionospheric measurements are too slow to allow any insight into the nature of these ionospheric reactions whose lifetimes are often very short. The relaxation time of the ionospheric ionization is only a few minutes or fraction of a minute in the lower ionosphere and in the E-region and is about 30 min to an hour at 300 km. The flares provide a sudden short impulse comparable to these time scales.
Author: Oddbjørn Engvold
Publisher: Elsevier
ISBN: 0128143355
Category : Science
Languages : en
Pages : 524
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Book Description
The Sun as a Guide to Stellar Physics illustrates the significance of the Sun in understanding stars through an examination of the discoveries and insights gained from solar physics research. Ranging from theories to modeling and from numerical simulations to instrumentation and data processing, the book provides an overview of what we currently understand and how the Sun can be a model for gaining further knowledge about stellar physics. Providing both updates on recent developments in solar physics and applications to stellar physics, this book strengthens the solar–stellar connection and summarizes what we know about the Sun for the stellar, space, and geophysics communities. Applies observations, theoretical understanding, modeling capabilities and physical processes first revealed by the sun to the study of stellar physics Illustrates how studies of Proxima Solaris have led to progress in space science, stellar physics and related fields Uses characteristics of solar phenomena as a guide for understanding the physics of stars
Author: S. Matsushita
Publisher: Elsevier
ISBN: 1483222519
Category : Science
Languages : en
Pages : 644
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Book Description
Physics of Geomagnetic phenomena, Volume I covers the significant advances in geomagnetism and the penetrations into the generation of geomagnetic field phenomena. This volume is composed of three chapters. Chapter I deals briefly with the discovery and developments in geomagnetism, followed by discussions on some fundamental topics of the field, including the aurora and geomagnetic storms. This chapter also considers the instruments, geomagnetic stations, and the correlations between geomagnetic indices. Chapter II describes the magnetic properties of minerals and various processes of acquisition of remanent magnetization. This chapter also provides palaeomagnetic data for the direction and intensity of the geomagnetic field in ancient times. Chapter III explores geomagnetic variations caused by solar flares and eclipses. This book will prove useful to physicists, students in upper atmospheric and space topics, and scientists in allied fields with a background in geomagnetism.
Author: James Haick III
Publisher: James Haick
ISBN: 1427696454
Category :
Languages : en
Pages : 36
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Book Description
It seemed like just another normal day for the story's main character, Jake Clifford. Little did he, or any one else, know that an x-class Solar Flare was heading straight for Earth. This looks like it will be the last "normal" day Jake and his friends will have in a long, long time.
Author: James Haick III
Publisher: Simon and Schuster
ISBN: 1949514773
Category : Comics & Graphic Novels
Languages : en
Pages : 160
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Book Description
"The world has been plunged into darkness and society as we know it has launched into chaos. Jake Clifford was just a regular guy - a man trying to achieve greatness in his career and a father doing his best to be the man his daughter deserved. That is, until a solar flare makes contact with Earth, wiping out all electricity and modern technology with one fatal blow. Now, Jake must adapt to this new world hoping to one day be reunited with his daughter who was states away when the lights went out." --
Author: Hermann J. Schaefer
Publisher:
ISBN:
Category : Proton beams
Languages : en
Pages : 24
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Book Description
The proton energy spectra for the Class 2 solar flare of February 5, 1965, as reported by a polar orbit satellite at five different times during the two-day period of enhanced intensity, are evaluated in terms of tissue depth doses for a semi-infinite slab with 0.1 g/sq cm shielding and for the Gemini and Apollo shield distribution. Maximum dose rates for the tissue surface are 714 millirads/hour, 81 and 11 millirads/hour, respectively. For the unidirectional beams, half value layers range from 2.6 to 5.6 millimeters of tissue. The integral flare dose over forty-four hours is 8.3 rads for the tissue surface behind 0.1 g/sq cm shielding. (Author).
Author: Rob Lopez
Publisher:
ISBN: 9781521856574
Category :
Languages : en
Pages : 242
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Book Description
The biggest solar flare since the 1859 Carrington Event is about to bring the world to its knees.When a huge plasma ejection from the sun hits the Earth's atmosphere, the resulting EMP pulse fries electricity grids and disables fragile electronics. Transmission wires melt, transformers explode and modern vehicles cease working. In less than a minute, the world is taken back two centuries.Lauren Nolan is attending a seminar in New York when the blackout hits and the transportation system grinds to a halt. Trapped in the panic that envelops the metropolis, Ellen worries for her children, five hundred miles away in North Carolina. Unable to get word to them, she faces a harrowing journey on her own.Sergeant Rick Nolan is overseas on a covert ops mission against terrorists. When the solar storm wipes out his communications and his air cover, he and his team find themselves on the same level as the enemy that surrounds them. Caught in a desperate fight for survival, Rick thinks about his family. How is he going to make it back alive?Trapped in their hometown of Charlotte, the two Nolan children witness society's terrifying collapse as water pumps fail, food runs short and the law ceases to exist. Frightened and bewildered, they wonder if they'll ever see their parents again.Solar Storm is Book 1 of an EMP, post-apocalyptic series about family survival and the challenges entailed. Contains moderate language and graphic action scenes.
Author: National Research Council
Publisher: National Academies Press
ISBN: 0309068851
Category : Science
Languages : en
Pages : 96
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Book Description
A major objective of the International Space Station is learning how to cope with the inherent risks of human spaceflightâ€"how to live and work in space for extended periods. The construction of the station itself provides the first opportunity for doing so. Prominent among the challenges associated with ISS construction is the large amount of time that astronauts will be spending doing extravehicular activity (EVA), or "space walks." EVAs from the space shuttle have been extraordinarily successful, most notably the on-orbit repair of the Hubble Space Telescope. But the number of hours of EVA for ISS construction exceeds that of the Hubble repair mission by orders of magnitude. Furthermore, the ISS orbit has nearly twice the inclination to Earth's equator as Hubble's orbit, so it spends part of every 90-minute circumnavigation at high latitudes, where Earth's magnetic field is less effective at shielding impinging radiation. This means that astronauts sweeping through these regions will be considerably more vulnerable to dangerous doses of energetic particles from a sudden solar eruption. Radiation and the International Space Station estimates that the likelihood of having a potentially dangerous solar event during an EVA is indeed very high. This report recommends steps that can be taken immediately, and over the next several years, to provide adequate warning so that the astronauts can be directed to take protective cover inside the ISS or shuttle. The near-term actions include programmatic and operational ways to take advantage of the multiagency assets that currently monitor and forecast space weather, and ways to improve the in situ measurements and the predictive power of current models.
Author: Constance Sawyer
Publisher:
ISBN:
Category :
Languages : en
Pages : 43
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Book Description
